The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array
The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Abbasi, R.U. [verfasserIn] |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2015transfer abstract |
|---|
| Schlagwörter: |
|---|
| Umfang: |
18 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells - 2012transfer abstract, Amsterdam [u.a.] |
|---|---|
| Übergeordnetes Werk: |
volume:68 ; year:2015 ; pages:27-44 ; extent:18 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.astropartphys.2015.02.008 |
|---|
| Katalog-ID: |
ELV029098270 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | ELV029098270 | ||
| 003 | DE-627 | ||
| 005 | 20230625165840.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 180603s2015 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1016/j.astropartphys.2015.02.008 |2 doi | |
| 028 | 5 | 2 | |a GBVA2015015000015.pica |
| 035 | |a (DE-627)ELV029098270 | ||
| 035 | |a (ELSEVIER)S0927-6505(15)00034-1 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | |a 540 | |
| 082 | 0 | 4 | |a 540 |q DE-600 |
| 082 | 0 | 4 | |a 620 |q VZ |
| 082 | 0 | 4 | |a 690 |q VZ |
| 084 | |a 50.92 |2 bkl | ||
| 100 | 1 | |a Abbasi, R.U. |e verfasserin |4 aut | |
| 245 | 1 | 4 | |a The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array |
| 264 | 1 | |c 2015transfer abstract | |
| 300 | |a 18 | ||
| 336 | |a nicht spezifiziert |b zzz |2 rdacontent | ||
| 337 | |a nicht spezifiziert |b z |2 rdamedia | ||
| 338 | |a nicht spezifiziert |b zu |2 rdacarrier | ||
| 520 | |a The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. | ||
| 520 | |a The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. | ||
| 650 | 7 | |a Energy spectrum |2 Elsevier | |
| 650 | 7 | |a Ultra high energy |2 Elsevier | |
| 650 | 7 | |a Hybrid |2 Elsevier | |
| 650 | 7 | |a Telescope Array |2 Elsevier | |
| 650 | 7 | |a Cosmic rays |2 Elsevier | |
| 700 | 1 | |a Abe, M. |4 oth | |
| 700 | 1 | |a Abu-Zayyad, T. |4 oth | |
| 700 | 1 | |a Allen, M.G. |4 oth | |
| 700 | 1 | |a Anderson, R. |4 oth | |
| 700 | 1 | |a Azuma, R. |4 oth | |
| 700 | 1 | |a Barcikowski, E. |4 oth | |
| 700 | 1 | |a Belz, J.W. |4 oth | |
| 700 | 1 | |a Bergman, D.R. |4 oth | |
| 700 | 1 | |a Blake, S.A. |4 oth | |
| 700 | 1 | |a Cady, R. |4 oth | |
| 700 | 1 | |a Chae, M.J. |4 oth | |
| 700 | 1 | |a Cheon, B.G. |4 oth | |
| 700 | 1 | |a Chiba, J. |4 oth | |
| 700 | 1 | |a Chikawa, M. |4 oth | |
| 700 | 1 | |a Cho, W.R. |4 oth | |
| 700 | 1 | |a Fujii, T. |4 oth | |
| 700 | 1 | |a Fukushima, M. |4 oth | |
| 700 | 1 | |a Goto, T. |4 oth | |
| 700 | 1 | |a Hanlon, W. |4 oth | |
| 700 | 1 | |a Hayashi, Y. |4 oth | |
| 700 | 1 | |a Hayashida, N. |4 oth | |
| 700 | 1 | |a Hibino, K. |4 oth | |
| 700 | 1 | |a Honda, K. |4 oth | |
| 700 | 1 | |a Ikeda, D. |4 oth | |
| 700 | 1 | |a Inoue, N. |4 oth | |
| 700 | 1 | |a Ishii, T. |4 oth | |
| 700 | 1 | |a Ishimori, R. |4 oth | |
| 700 | 1 | |a Ito, H. |4 oth | |
| 700 | 1 | |a Ivanov, D. |4 oth | |
| 700 | 1 | |a Jui, C.C.H. |4 oth | |
| 700 | 1 | |a Kadota, K. |4 oth | |
| 700 | 1 | |a Kakimoto, F. |4 oth | |
| 700 | 1 | |a Kalashev, O. |4 oth | |
| 700 | 1 | |a Kasahara, K. |4 oth | |
| 700 | 1 | |a Kawai, H. |4 oth | |
| 700 | 1 | |a Kawakami, S. |4 oth | |
| 700 | 1 | |a Kawana, S. |4 oth | |
| 700 | 1 | |a Kawata, K. |4 oth | |
| 700 | 1 | |a Kido, E. |4 oth | |
| 700 | 1 | |a Kim, H.B. |4 oth | |
| 700 | 1 | |a Kim, J.H. |4 oth | |
| 700 | 1 | |a Kim, J.H. |4 oth | |
| 700 | 1 | |a Kitamura, S. |4 oth | |
| 700 | 1 | |a Kitamura, Y. |4 oth | |
| 700 | 1 | |a Kuzmin, V. |4 oth | |
| 700 | 1 | |a Kwon, Y.J. |4 oth | |
| 700 | 1 | |a Lan, J. |4 oth | |
| 700 | 1 | |a Lim, S.I. |4 oth | |
| 700 | 1 | |a Lundquist, J.P. |4 oth | |
| 700 | 1 | |a Machida, K. |4 oth | |
| 700 | 1 | |a Martens, K. |4 oth | |
| 700 | 1 | |a Matsuda, T. |4 oth | |
| 700 | 1 | |a Matsuyama, T. |4 oth | |
| 700 | 1 | |a Matthews, J.N. |4 oth | |
| 700 | 1 | |a Minamino, M. |4 oth | |
| 700 | 1 | |a Mukai, K. |4 oth | |
| 700 | 1 | |a Myers, I. |4 oth | |
| 700 | 1 | |a Nagasawa, K. |4 oth | |
| 700 | 1 | |a Nagataki, S. |4 oth | |
| 700 | 1 | |a Nakamura, T. |4 oth | |
| 700 | 1 | |a Nonaka, T. |4 oth | |
| 700 | 1 | |a Nozato, A. |4 oth | |
| 700 | 1 | |a Ogio, S. |4 oth | |
| 700 | 1 | |a Ogura, J. |4 oth | |
| 700 | 1 | |a Ohnishi, M. |4 oth | |
| 700 | 1 | |a Ohoka, H. |4 oth | |
| 700 | 1 | |a Oki, K. |4 oth | |
| 700 | 1 | |a Okuda, T. |4 oth | |
| 700 | 1 | |a Ono, M. |4 oth | |
| 700 | 1 | |a Oshima, A. |4 oth | |
| 700 | 1 | |a Ozawa, S. |4 oth | |
| 700 | 1 | |a Park, I.H. |4 oth | |
| 700 | 1 | |a Pshirkov, M.S. |4 oth | |
| 700 | 1 | |a Rodriguez, D.C. |4 oth | |
| 700 | 1 | |a Rubtsov, G. |4 oth | |
| 700 | 1 | |a Ryu, D. |4 oth | |
| 700 | 1 | |a Sagawa, H. |4 oth | |
| 700 | 1 | |a Sakurai, N. |4 oth | |
| 700 | 1 | |a Sampson, A.L. |4 oth | |
| 700 | 1 | |a Scott, L.M. |4 oth | |
| 700 | 1 | |a Shah, P.D. |4 oth | |
| 700 | 1 | |a Shibata, F. |4 oth | |
| 700 | 1 | |a Shibata, T. |4 oth | |
| 700 | 1 | |a Shimodaira, H. |4 oth | |
| 700 | 1 | |a Shin, B.K. |4 oth | |
| 700 | 1 | |a Shin, H.S. |4 oth | |
| 700 | 1 | |a Smith, J.D. |4 oth | |
| 700 | 1 | |a Sokolsky, P. |4 oth | |
| 700 | 1 | |a Springer, R.W. |4 oth | |
| 700 | 1 | |a Stokes, B.T. |4 oth | |
| 700 | 1 | |a Stratton, S.R. |4 oth | |
| 700 | 1 | |a Stroman, T.A. |4 oth | |
| 700 | 1 | |a Suzawa, T. |4 oth | |
| 700 | 1 | |a Takamura, M. |4 oth | |
| 700 | 1 | |a Takeda, M. |4 oth | |
| 700 | 1 | |a Takeishi, R. |4 oth | |
| 700 | 1 | |a Taketa, A. |4 oth | |
| 700 | 1 | |a Takita, M. |4 oth | |
| 700 | 1 | |a Tameda, Y. |4 oth | |
| 700 | 1 | |a Tanaka, H. |4 oth | |
| 700 | 1 | |a Tanaka, K. |4 oth | |
| 700 | 1 | |a Tanaka, M. |4 oth | |
| 700 | 1 | |a Thomas, S.B. |4 oth | |
| 700 | 1 | |a Thomson, G.B. |4 oth | |
| 700 | 1 | |a Tinyakov, P. |4 oth | |
| 700 | 1 | |a Tkachev, I. |4 oth | |
| 700 | 1 | |a Tokuno, H. |4 oth | |
| 700 | 1 | |a Tomida, T. |4 oth | |
| 700 | 1 | |a Troitsky, S. |4 oth | |
| 700 | 1 | |a Tsunesada, Y. |4 oth | |
| 700 | 1 | |a Tsutsumi, K. |4 oth | |
| 700 | 1 | |a Uchihori, Y. |4 oth | |
| 700 | 1 | |a Udo, S. |4 oth | |
| 700 | 1 | |a Urban, F. |4 oth | |
| 700 | 1 | |a Vasiloff, G. |4 oth | |
| 700 | 1 | |a Wong, T. |4 oth | |
| 700 | 1 | |a Yamane, R. |4 oth | |
| 700 | 1 | |a Yamaoka, H. |4 oth | |
| 700 | 1 | |a Yamazaki, K. |4 oth | |
| 700 | 1 | |a Yang, J. |4 oth | |
| 700 | 1 | |a Yashiro, K. |4 oth | |
| 700 | 1 | |a Yoneda, Y. |4 oth | |
| 700 | 1 | |a Yoshida, S. |4 oth | |
| 700 | 1 | |a Yoshii, H. |4 oth | |
| 700 | 1 | |a Zollinger, R. |4 oth | |
| 700 | 1 | |a Zundel, Z. |4 oth | |
| 773 | 0 | 8 | |i Enthalten in |n Elsevier Science |t Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |d 2012transfer abstract |g Amsterdam [u.a.] |w (DE-627)ELV016257995 |
| 773 | 1 | 8 | |g volume:68 |g year:2015 |g pages:27-44 |g extent:18 |
| 856 | 4 | 0 | |u https://doi.org/10.1016/j.astropartphys.2015.02.008 |3 Volltext |
| 912 | |a GBV_USEFLAG_U | ||
| 912 | |a GBV_ELV | ||
| 912 | |a SYSFLAG_U | ||
| 912 | |a GBV_ILN_20 | ||
| 912 | |a GBV_ILN_252 | ||
| 936 | b | k | |a 50.92 |j Meerestechnik |q VZ |
| 951 | |a AR | ||
| 952 | |d 68 |j 2015 |h 27-44 |g 18 | ||
| 953 | |2 045F |a 540 | ||
| author_variant |
r a ra |
|---|---|
| matchkey_str |
abbasiruabemabuzayyadtallenmgandersonraz:2015----:hhbieegsetuotlsoerasidermee |
| hierarchy_sort_str |
2015transfer abstract |
| bklnumber |
50.92 |
| publishDate |
2015 |
| allfields |
10.1016/j.astropartphys.2015.02.008 doi GBVA2015015000015.pica (DE-627)ELV029098270 (ELSEVIER)S0927-6505(15)00034-1 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Abbasi, R.U. verfasserin aut The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array 2015transfer abstract 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays Elsevier Abe, M. oth Abu-Zayyad, T. oth Allen, M.G. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Chae, M.J. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, W.R. oth Fujii, T. oth Fukushima, M. oth Goto, T. oth Hanlon, W. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Honda, K. oth Ikeda, D. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ito, H. oth Ivanov, D. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kawata, K. oth Kido, E. oth Kim, H.B. oth Kim, J.H. oth Kim, J.H. oth Kitamura, S. oth Kitamura, Y. oth Kuzmin, V. oth Kwon, Y.J. oth Lan, J. oth Lim, S.I. oth Lundquist, J.P. oth Machida, K. oth Martens, K. oth Matsuda, T. oth Matsuyama, T. oth Matthews, J.N. oth Minamino, M. oth Mukai, K. oth Myers, I. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nonaka, T. oth Nozato, A. oth Ogio, S. oth Ogura, J. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Okuda, T. oth Ono, M. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, B.K. oth Shin, H.S. oth Smith, J.D. oth Sokolsky, P. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T.A. oth Suzawa, T. oth Takamura, M. oth Takeda, M. oth Takeishi, R. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tokuno, H. oth Tomida, T. oth Troitsky, S. oth Tsunesada, Y. oth Tsutsumi, K. oth Uchihori, Y. oth Udo, S. oth Urban, F. oth Vasiloff, G. oth Wong, T. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yashiro, K. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zollinger, R. oth Zundel, Z. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:68 year:2015 pages:27-44 extent:18 https://doi.org/10.1016/j.astropartphys.2015.02.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 68 2015 27-44 18 045F 540 |
| spelling |
10.1016/j.astropartphys.2015.02.008 doi GBVA2015015000015.pica (DE-627)ELV029098270 (ELSEVIER)S0927-6505(15)00034-1 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Abbasi, R.U. verfasserin aut The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array 2015transfer abstract 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays Elsevier Abe, M. oth Abu-Zayyad, T. oth Allen, M.G. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Chae, M.J. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, W.R. oth Fujii, T. oth Fukushima, M. oth Goto, T. oth Hanlon, W. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Honda, K. oth Ikeda, D. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ito, H. oth Ivanov, D. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kawata, K. oth Kido, E. oth Kim, H.B. oth Kim, J.H. oth Kim, J.H. oth Kitamura, S. oth Kitamura, Y. oth Kuzmin, V. oth Kwon, Y.J. oth Lan, J. oth Lim, S.I. oth Lundquist, J.P. oth Machida, K. oth Martens, K. oth Matsuda, T. oth Matsuyama, T. oth Matthews, J.N. oth Minamino, M. oth Mukai, K. oth Myers, I. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nonaka, T. oth Nozato, A. oth Ogio, S. oth Ogura, J. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Okuda, T. oth Ono, M. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, B.K. oth Shin, H.S. oth Smith, J.D. oth Sokolsky, P. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T.A. oth Suzawa, T. oth Takamura, M. oth Takeda, M. oth Takeishi, R. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tokuno, H. oth Tomida, T. oth Troitsky, S. oth Tsunesada, Y. oth Tsutsumi, K. oth Uchihori, Y. oth Udo, S. oth Urban, F. oth Vasiloff, G. oth Wong, T. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yashiro, K. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zollinger, R. oth Zundel, Z. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:68 year:2015 pages:27-44 extent:18 https://doi.org/10.1016/j.astropartphys.2015.02.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 68 2015 27-44 18 045F 540 |
| allfields_unstemmed |
10.1016/j.astropartphys.2015.02.008 doi GBVA2015015000015.pica (DE-627)ELV029098270 (ELSEVIER)S0927-6505(15)00034-1 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Abbasi, R.U. verfasserin aut The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array 2015transfer abstract 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays Elsevier Abe, M. oth Abu-Zayyad, T. oth Allen, M.G. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Chae, M.J. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, W.R. oth Fujii, T. oth Fukushima, M. oth Goto, T. oth Hanlon, W. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Honda, K. oth Ikeda, D. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ito, H. oth Ivanov, D. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kawata, K. oth Kido, E. oth Kim, H.B. oth Kim, J.H. oth Kim, J.H. oth Kitamura, S. oth Kitamura, Y. oth Kuzmin, V. oth Kwon, Y.J. oth Lan, J. oth Lim, S.I. oth Lundquist, J.P. oth Machida, K. oth Martens, K. oth Matsuda, T. oth Matsuyama, T. oth Matthews, J.N. oth Minamino, M. oth Mukai, K. oth Myers, I. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nonaka, T. oth Nozato, A. oth Ogio, S. oth Ogura, J. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Okuda, T. oth Ono, M. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, B.K. oth Shin, H.S. oth Smith, J.D. oth Sokolsky, P. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T.A. oth Suzawa, T. oth Takamura, M. oth Takeda, M. oth Takeishi, R. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tokuno, H. oth Tomida, T. oth Troitsky, S. oth Tsunesada, Y. oth Tsutsumi, K. oth Uchihori, Y. oth Udo, S. oth Urban, F. oth Vasiloff, G. oth Wong, T. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yashiro, K. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zollinger, R. oth Zundel, Z. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:68 year:2015 pages:27-44 extent:18 https://doi.org/10.1016/j.astropartphys.2015.02.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 68 2015 27-44 18 045F 540 |
| allfieldsGer |
10.1016/j.astropartphys.2015.02.008 doi GBVA2015015000015.pica (DE-627)ELV029098270 (ELSEVIER)S0927-6505(15)00034-1 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Abbasi, R.U. verfasserin aut The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array 2015transfer abstract 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays Elsevier Abe, M. oth Abu-Zayyad, T. oth Allen, M.G. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Chae, M.J. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, W.R. oth Fujii, T. oth Fukushima, M. oth Goto, T. oth Hanlon, W. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Honda, K. oth Ikeda, D. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ito, H. oth Ivanov, D. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kawata, K. oth Kido, E. oth Kim, H.B. oth Kim, J.H. oth Kim, J.H. oth Kitamura, S. oth Kitamura, Y. oth Kuzmin, V. oth Kwon, Y.J. oth Lan, J. oth Lim, S.I. oth Lundquist, J.P. oth Machida, K. oth Martens, K. oth Matsuda, T. oth Matsuyama, T. oth Matthews, J.N. oth Minamino, M. oth Mukai, K. oth Myers, I. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nonaka, T. oth Nozato, A. oth Ogio, S. oth Ogura, J. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Okuda, T. oth Ono, M. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, B.K. oth Shin, H.S. oth Smith, J.D. oth Sokolsky, P. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T.A. oth Suzawa, T. oth Takamura, M. oth Takeda, M. oth Takeishi, R. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tokuno, H. oth Tomida, T. oth Troitsky, S. oth Tsunesada, Y. oth Tsutsumi, K. oth Uchihori, Y. oth Udo, S. oth Urban, F. oth Vasiloff, G. oth Wong, T. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yashiro, K. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zollinger, R. oth Zundel, Z. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:68 year:2015 pages:27-44 extent:18 https://doi.org/10.1016/j.astropartphys.2015.02.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 68 2015 27-44 18 045F 540 |
| allfieldsSound |
10.1016/j.astropartphys.2015.02.008 doi GBVA2015015000015.pica (DE-627)ELV029098270 (ELSEVIER)S0927-6505(15)00034-1 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Abbasi, R.U. verfasserin aut The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array 2015transfer abstract 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays Elsevier Abe, M. oth Abu-Zayyad, T. oth Allen, M.G. oth Anderson, R. oth Azuma, R. oth Barcikowski, E. oth Belz, J.W. oth Bergman, D.R. oth Blake, S.A. oth Cady, R. oth Chae, M.J. oth Cheon, B.G. oth Chiba, J. oth Chikawa, M. oth Cho, W.R. oth Fujii, T. oth Fukushima, M. oth Goto, T. oth Hanlon, W. oth Hayashi, Y. oth Hayashida, N. oth Hibino, K. oth Honda, K. oth Ikeda, D. oth Inoue, N. oth Ishii, T. oth Ishimori, R. oth Ito, H. oth Ivanov, D. oth Jui, C.C.H. oth Kadota, K. oth Kakimoto, F. oth Kalashev, O. oth Kasahara, K. oth Kawai, H. oth Kawakami, S. oth Kawana, S. oth Kawata, K. oth Kido, E. oth Kim, H.B. oth Kim, J.H. oth Kim, J.H. oth Kitamura, S. oth Kitamura, Y. oth Kuzmin, V. oth Kwon, Y.J. oth Lan, J. oth Lim, S.I. oth Lundquist, J.P. oth Machida, K. oth Martens, K. oth Matsuda, T. oth Matsuyama, T. oth Matthews, J.N. oth Minamino, M. oth Mukai, K. oth Myers, I. oth Nagasawa, K. oth Nagataki, S. oth Nakamura, T. oth Nonaka, T. oth Nozato, A. oth Ogio, S. oth Ogura, J. oth Ohnishi, M. oth Ohoka, H. oth Oki, K. oth Okuda, T. oth Ono, M. oth Oshima, A. oth Ozawa, S. oth Park, I.H. oth Pshirkov, M.S. oth Rodriguez, D.C. oth Rubtsov, G. oth Ryu, D. oth Sagawa, H. oth Sakurai, N. oth Sampson, A.L. oth Scott, L.M. oth Shah, P.D. oth Shibata, F. oth Shibata, T. oth Shimodaira, H. oth Shin, B.K. oth Shin, H.S. oth Smith, J.D. oth Sokolsky, P. oth Springer, R.W. oth Stokes, B.T. oth Stratton, S.R. oth Stroman, T.A. oth Suzawa, T. oth Takamura, M. oth Takeda, M. oth Takeishi, R. oth Taketa, A. oth Takita, M. oth Tameda, Y. oth Tanaka, H. oth Tanaka, K. oth Tanaka, M. oth Thomas, S.B. oth Thomson, G.B. oth Tinyakov, P. oth Tkachev, I. oth Tokuno, H. oth Tomida, T. oth Troitsky, S. oth Tsunesada, Y. oth Tsutsumi, K. oth Uchihori, Y. oth Udo, S. oth Urban, F. oth Vasiloff, G. oth Wong, T. oth Yamane, R. oth Yamaoka, H. oth Yamazaki, K. oth Yang, J. oth Yashiro, K. oth Yoneda, Y. oth Yoshida, S. oth Yoshii, H. oth Zollinger, R. oth Zundel, Z. oth Enthalten in Elsevier Science Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells 2012transfer abstract Amsterdam [u.a.] (DE-627)ELV016257995 volume:68 year:2015 pages:27-44 extent:18 https://doi.org/10.1016/j.astropartphys.2015.02.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 68 2015 27-44 18 045F 540 |
| language |
English |
| source |
Enthalten in Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells Amsterdam [u.a.] volume:68 year:2015 pages:27-44 extent:18 |
| sourceStr |
Enthalten in Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells Amsterdam [u.a.] volume:68 year:2015 pages:27-44 extent:18 |
| format_phy_str_mv |
Article |
| bklname |
Meerestechnik |
| institution |
findex.gbv.de |
| topic_facet |
Energy spectrum Ultra high energy Hybrid Telescope Array Cosmic rays |
| dewey-raw |
540 |
| isfreeaccess_bool |
false |
| container_title |
Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
| authorswithroles_txt_mv |
Abbasi, R.U. @@aut@@ Abe, M. @@oth@@ Abu-Zayyad, T. @@oth@@ Allen, M.G. @@oth@@ Anderson, R. @@oth@@ Azuma, R. @@oth@@ Barcikowski, E. @@oth@@ Belz, J.W. @@oth@@ Bergman, D.R. @@oth@@ Blake, S.A. @@oth@@ Cady, R. @@oth@@ Chae, M.J. @@oth@@ Cheon, B.G. @@oth@@ Chiba, J. @@oth@@ Chikawa, M. @@oth@@ Cho, W.R. @@oth@@ Fujii, T. @@oth@@ Fukushima, M. @@oth@@ Goto, T. @@oth@@ Hanlon, W. @@oth@@ Hayashi, Y. @@oth@@ Hayashida, N. @@oth@@ Hibino, K. @@oth@@ Honda, K. @@oth@@ Ikeda, D. @@oth@@ Inoue, N. @@oth@@ Ishii, T. @@oth@@ Ishimori, R. @@oth@@ Ito, H. @@oth@@ Ivanov, D. @@oth@@ Jui, C.C.H. @@oth@@ Kadota, K. @@oth@@ Kakimoto, F. @@oth@@ Kalashev, O. @@oth@@ Kasahara, K. @@oth@@ Kawai, H. @@oth@@ Kawakami, S. @@oth@@ Kawana, S. @@oth@@ Kawata, K. @@oth@@ Kido, E. @@oth@@ Kim, H.B. @@oth@@ Kim, J.H. @@oth@@ Kitamura, S. @@oth@@ Kitamura, Y. @@oth@@ Kuzmin, V. @@oth@@ Kwon, Y.J. @@oth@@ Lan, J. @@oth@@ Lim, S.I. @@oth@@ Lundquist, J.P. @@oth@@ Machida, K. @@oth@@ Martens, K. @@oth@@ Matsuda, T. @@oth@@ Matsuyama, T. @@oth@@ Matthews, J.N. @@oth@@ Minamino, M. @@oth@@ Mukai, K. @@oth@@ Myers, I. @@oth@@ Nagasawa, K. @@oth@@ Nagataki, S. @@oth@@ Nakamura, T. @@oth@@ Nonaka, T. @@oth@@ Nozato, A. @@oth@@ Ogio, S. @@oth@@ Ogura, J. @@oth@@ Ohnishi, M. @@oth@@ Ohoka, H. @@oth@@ Oki, K. @@oth@@ Okuda, T. @@oth@@ Ono, M. @@oth@@ Oshima, A. @@oth@@ Ozawa, S. @@oth@@ Park, I.H. @@oth@@ Pshirkov, M.S. @@oth@@ Rodriguez, D.C. @@oth@@ Rubtsov, G. @@oth@@ Ryu, D. @@oth@@ Sagawa, H. @@oth@@ Sakurai, N. @@oth@@ Sampson, A.L. @@oth@@ Scott, L.M. @@oth@@ Shah, P.D. @@oth@@ Shibata, F. @@oth@@ Shibata, T. @@oth@@ Shimodaira, H. @@oth@@ Shin, B.K. @@oth@@ Shin, H.S. @@oth@@ Smith, J.D. @@oth@@ Sokolsky, P. @@oth@@ Springer, R.W. @@oth@@ Stokes, B.T. @@oth@@ Stratton, S.R. @@oth@@ Stroman, T.A. @@oth@@ Suzawa, T. @@oth@@ Takamura, M. @@oth@@ Takeda, M. @@oth@@ Takeishi, R. @@oth@@ Taketa, A. @@oth@@ Takita, M. @@oth@@ Tameda, Y. @@oth@@ Tanaka, H. @@oth@@ Tanaka, K. @@oth@@ Tanaka, M. @@oth@@ Thomas, S.B. @@oth@@ Thomson, G.B. @@oth@@ Tinyakov, P. @@oth@@ Tkachev, I. @@oth@@ Tokuno, H. @@oth@@ Tomida, T. @@oth@@ Troitsky, S. @@oth@@ Tsunesada, Y. @@oth@@ Tsutsumi, K. @@oth@@ Uchihori, Y. @@oth@@ Udo, S. @@oth@@ Urban, F. @@oth@@ Vasiloff, G. @@oth@@ Wong, T. @@oth@@ Yamane, R. @@oth@@ Yamaoka, H. @@oth@@ Yamazaki, K. @@oth@@ Yang, J. @@oth@@ Yashiro, K. @@oth@@ Yoneda, Y. @@oth@@ Yoshida, S. @@oth@@ Yoshii, H. @@oth@@ Zollinger, R. @@oth@@ Zundel, Z. @@oth@@ |
| publishDateDaySort_date |
2015-01-01T00:00:00Z |
| hierarchy_top_id |
ELV016257995 |
| dewey-sort |
3540 |
| id |
ELV029098270 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV029098270</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230625165840.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">180603s2015 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.astropartphys.2015.02.008</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">GBVA2015015000015.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV029098270</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0927-6505(15)00034-1</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">540</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">540</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">690</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">50.92</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Abbasi, R.U.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015transfer abstract</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">18</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Energy spectrum</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Ultra high energy</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Hybrid</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Telescope Array</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Cosmic rays</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Abe, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Abu-Zayyad, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Allen, M.G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anderson, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Azuma, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Barcikowski, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Belz, J.W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bergman, D.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Blake, S.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cady, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chae, M.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cheon, B.G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chiba, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chikawa, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cho, W.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fujii, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fukushima, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Goto, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hanlon, W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayashi, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayashida, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hibino, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Honda, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ikeda, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Inoue, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ishii, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ishimori, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ito, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ivanov, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jui, C.C.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kadota, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kakimoto, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kalashev, O.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kasahara, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawai, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawakami, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawana, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawata, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kido, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, H.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, J.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, J.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kitamura, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kitamura, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kuzmin, V.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kwon, Y.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lan, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lim, S.I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lundquist, J.P.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Machida, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Martens, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Matsuda, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Matsuyama, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Matthews, J.N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Minamino, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mukai, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Myers, I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nagasawa, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nagataki, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nakamura, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nonaka, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nozato, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ogio, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ogura, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ohnishi, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ohoka, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oki, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Okuda, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ono, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oshima, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ozawa, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Park, I.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pshirkov, M.S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rodriguez, D.C.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rubtsov, G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ryu, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sagawa, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sakurai, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sampson, A.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Scott, L.M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shah, P.D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shibata, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shibata, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shimodaira, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shin, B.K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shin, H.S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Smith, J.D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sokolsky, P.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Springer, R.W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stokes, B.T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stratton, S.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stroman, T.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Suzawa, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takamura, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takeda, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takeishi, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Taketa, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takita, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tameda, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tanaka, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tanaka, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tanaka, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Thomas, S.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Thomson, G.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tinyakov, P.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tkachev, I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tokuno, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tomida, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Troitsky, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tsunesada, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tsutsumi, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Uchihori, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Udo, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Urban, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Vasiloff, G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wong, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yamane, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yamaoka, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yamazaki, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yang, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yashiro, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yoneda, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yoshida, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yoshii, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zollinger, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zundel, Z.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="n">Elsevier Science</subfield><subfield code="t">Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells</subfield><subfield code="d">2012transfer abstract</subfield><subfield code="g">Amsterdam [u.a.]</subfield><subfield code="w">(DE-627)ELV016257995</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:68</subfield><subfield code="g">year:2015</subfield><subfield code="g">pages:27-44</subfield><subfield code="g">extent:18</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1016/j.astropartphys.2015.02.008</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ELV</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_252</subfield></datafield><datafield tag="936" ind1="b" ind2="k"><subfield code="a">50.92</subfield><subfield code="j">Meerestechnik</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">68</subfield><subfield code="j">2015</subfield><subfield code="h">27-44</subfield><subfield code="g">18</subfield></datafield><datafield tag="953" ind1=" " ind2=" "><subfield code="2">045F</subfield><subfield code="a">540</subfield></datafield></record></collection>
|
| author |
Abbasi, R.U. |
| spellingShingle |
Abbasi, R.U. ddc 540 ddc 620 ddc 690 bkl 50.92 Elsevier Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array |
| authorStr |
Abbasi, R.U. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)ELV016257995 |
| format |
electronic Article |
| dewey-ones |
540 - Chemistry & allied sciences 620 - Engineering & allied operations 690 - Buildings |
| delete_txt_mv |
keep |
| author_role |
aut |
| collection |
elsevier |
| remote_str |
true |
| illustrated |
Not Illustrated |
| topic_title |
540 540 DE-600 620 VZ 690 VZ 50.92 bkl The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays Elsevier |
| topic |
ddc 540 ddc 620 ddc 690 bkl 50.92 Elsevier Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays |
| topic_unstemmed |
ddc 540 ddc 620 ddc 690 bkl 50.92 Elsevier Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays |
| topic_browse |
ddc 540 ddc 620 ddc 690 bkl 50.92 Elsevier Energy spectrum Elsevier Ultra high energy Elsevier Hybrid Elsevier Telescope Array Elsevier Cosmic rays |
| format_facet |
Elektronische Aufsätze Aufsätze Elektronische Ressource |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
zu |
| author2_variant |
m a ma t a z taz m a ma r a ra r a ra e b eb j b jb d b db s b sb r c rc m c mc b c bc j c jc m c mc w c wc t f tf m f mf t g tg w h wh y h yh n h nh k h kh k h kh d i di n i ni t i ti r i ri h i hi d i di c j cj k k kk f k fk o k ok k k kk h k hk s k sk s k sk k k kk e k ek h k hk j k jk j k jk s k sk y k yk v k vk y k yk j l jl s l sl j l jl k m km k m km t m tm t m tm j m jm m m mm k m km i m im k n kn s n sn t n tn t n tn a n an s o so j o jo m o mo h o ho k o ko t o to m o mo a o ao s o so i p ip m p mp d r dr g r gr d r dr h s hs n s ns a s as l s ls p s ps f s fs t s ts h s hs b s bs h s hs j s js p s ps r s rs b s bs s s ss t s ts t s ts m t mt m t mt r t rt a t at m t mt y t yt h t ht k t kt m t mt s t st g t gt p t pt i t it h t ht t t tt s t st y t yt k t kt y u yu s u su f u fu g v gv t w tw r y ry h y hy k y ky j y jy k y ky y y yy s y sy h y hy r z rz z z zz |
| hierarchy_parent_title |
Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
| hierarchy_parent_id |
ELV016257995 |
| dewey-tens |
540 - Chemistry 620 - Engineering 690 - Building & construction |
| hierarchy_top_title |
Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)ELV016257995 |
| title |
The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array |
| ctrlnum |
(DE-627)ELV029098270 (ELSEVIER)S0927-6505(15)00034-1 |
| title_full |
The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array |
| author_sort |
Abbasi, R.U. |
| journal |
Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
| journalStr |
Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science 600 - Technology |
| recordtype |
marc |
| publishDateSort |
2015 |
| contenttype_str_mv |
zzz |
| container_start_page |
27 |
| author_browse |
Abbasi, R.U. |
| container_volume |
68 |
| physical |
18 |
| class |
540 540 DE-600 620 VZ 690 VZ 50.92 bkl |
| format_se |
Elektronische Aufsätze |
| author-letter |
Abbasi, R.U. |
| doi_str_mv |
10.1016/j.astropartphys.2015.02.008 |
| dewey-full |
540 620 690 |
| title_sort |
hybrid energy spectrum of telescope array’s middle drum detector and surface array |
| title_auth |
The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array |
| abstract |
The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. |
| abstractGer |
The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. |
| abstract_unstemmed |
The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown. |
| collection_details |
GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 |
| title_short |
The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array |
| url |
https://doi.org/10.1016/j.astropartphys.2015.02.008 |
| remote_bool |
true |
| author2 |
Abe, M. Abu-Zayyad, T. Allen, M.G. Anderson, R. Azuma, R. Barcikowski, E. Belz, J.W. Bergman, D.R. Blake, S.A. Cady, R. Chae, M.J. Cheon, B.G. Chiba, J. Chikawa, M. Cho, W.R. Fujii, T. Fukushima, M. Goto, T. Hanlon, W. Hayashi, Y. Hayashida, N. Hibino, K. Honda, K. Ikeda, D. Inoue, N. Ishii, T. Ishimori, R. Ito, H. Ivanov, D. Jui, C.C.H. Kadota, K. Kakimoto, F. Kalashev, O. Kasahara, K. Kawai, H. Kawakami, S. Kawana, S. Kawata, K. Kido, E. Kim, H.B. Kim, J.H. Kitamura, S. Kitamura, Y. Kuzmin, V. Kwon, Y.J. Lan, J. Lim, S.I. Lundquist, J.P. Machida, K. Martens, K. Matsuda, T. Matsuyama, T. Matthews, J.N. Minamino, M. Mukai, K. Myers, I. Nagasawa, K. Nagataki, S. Nakamura, T. Nonaka, T. Nozato, A. Ogio, S. Ogura, J. Ohnishi, M. Ohoka, H. Oki, K. Okuda, T. Ono, M. Oshima, A. Ozawa, S. Park, I.H. Pshirkov, M.S. Rodriguez, D.C. Rubtsov, G. Ryu, D. Sagawa, H. Sakurai, N. Sampson, A.L. Scott, L.M. Shah, P.D. Shibata, F. Shibata, T. Shimodaira, H. Shin, B.K. Shin, H.S. Smith, J.D. Sokolsky, P. Springer, R.W. Stokes, B.T. Stratton, S.R. Stroman, T.A. Suzawa, T. Takamura, M. Takeda, M. Takeishi, R. Taketa, A. Takita, M. Tameda, Y. Tanaka, H. Tanaka, K. Tanaka, M. Thomas, S.B. Thomson, G.B. Tinyakov, P. Tkachev, I. Tokuno, H. Tomida, T. Troitsky, S. Tsunesada, Y. Tsutsumi, K. Uchihori, Y. Udo, S. Urban, F. Vasiloff, G. Wong, T. Yamane, R. Yamaoka, H. Yamazaki, K. Yang, J. Yashiro, K. Yoneda, Y. Yoshida, S. Yoshii, H. Zollinger, R. Zundel, Z. |
| author2Str |
Abe, M. Abu-Zayyad, T. Allen, M.G. Anderson, R. Azuma, R. Barcikowski, E. Belz, J.W. Bergman, D.R. Blake, S.A. Cady, R. Chae, M.J. Cheon, B.G. Chiba, J. Chikawa, M. Cho, W.R. Fujii, T. Fukushima, M. Goto, T. Hanlon, W. Hayashi, Y. Hayashida, N. Hibino, K. Honda, K. Ikeda, D. Inoue, N. Ishii, T. Ishimori, R. Ito, H. Ivanov, D. Jui, C.C.H. Kadota, K. Kakimoto, F. Kalashev, O. Kasahara, K. Kawai, H. Kawakami, S. Kawana, S. Kawata, K. Kido, E. Kim, H.B. Kim, J.H. Kitamura, S. Kitamura, Y. Kuzmin, V. Kwon, Y.J. Lan, J. Lim, S.I. Lundquist, J.P. Machida, K. Martens, K. Matsuda, T. Matsuyama, T. Matthews, J.N. Minamino, M. Mukai, K. Myers, I. Nagasawa, K. Nagataki, S. Nakamura, T. Nonaka, T. Nozato, A. Ogio, S. Ogura, J. Ohnishi, M. Ohoka, H. Oki, K. Okuda, T. Ono, M. Oshima, A. Ozawa, S. Park, I.H. Pshirkov, M.S. Rodriguez, D.C. Rubtsov, G. Ryu, D. Sagawa, H. Sakurai, N. Sampson, A.L. Scott, L.M. Shah, P.D. Shibata, F. Shibata, T. Shimodaira, H. Shin, B.K. Shin, H.S. Smith, J.D. Sokolsky, P. Springer, R.W. Stokes, B.T. Stratton, S.R. Stroman, T.A. Suzawa, T. Takamura, M. Takeda, M. Takeishi, R. Taketa, A. Takita, M. Tameda, Y. Tanaka, H. Tanaka, K. Tanaka, M. Thomas, S.B. Thomson, G.B. Tinyakov, P. Tkachev, I. Tokuno, H. Tomida, T. Troitsky, S. Tsunesada, Y. Tsutsumi, K. Uchihori, Y. Udo, S. Urban, F. Vasiloff, G. Wong, T. Yamane, R. Yamaoka, H. Yamazaki, K. Yang, J. Yashiro, K. Yoneda, Y. Yoshida, S. Yoshii, H. Zollinger, R. Zundel, Z. |
| ppnlink |
ELV016257995 |
| mediatype_str_mv |
z |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| author2_role |
oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth oth |
| doi_str |
10.1016/j.astropartphys.2015.02.008 |
| up_date |
2024-07-06T20:32:39.060Z |
| _version_ |
1803863152722444288 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV029098270</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230625165840.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">180603s2015 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.astropartphys.2015.02.008</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">GBVA2015015000015.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV029098270</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0927-6505(15)00034-1</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">540</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">540</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">690</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">50.92</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Abbasi, R.U.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The hybrid energy spectrum of Telescope Array’s Middle Drum Detector and surface array</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015transfer abstract</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">18</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Telescope Array experiment studies ultra high energy cosmic rays using a hybrid detector. Fluorescence telescopes measure the longitudinal development of the extensive air shower generated when a primary cosmic ray particle interacts with the atmosphere. Meanwhile, scintillator detectors measure the lateral distribution of secondary shower particles that hit the ground. The Middle Drum (MD) fluorescence telescope station consists of 14 telescopes from the High Resolution Fly’s Eye (HiRes) experiment, providing a direct link back to the HiRes measurements. Using the scintillator detector data in conjunction with the telescope data improves the geometrical reconstruction of the showers significantly, and hence, provides a more accurate reconstruction of the energy of the primary particle. The Middle Drum hybrid spectrum is presented and compared to that measured by the Middle Drum station in monocular mode. Further, the hybrid data establishes a link between the Middle Drum data and the surface array. A comparison between the Middle Drum hybrid energy spectrum and scintillator Surface Detector (SD) spectrum is also shown.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Energy spectrum</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Ultra high energy</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Hybrid</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Telescope Array</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Cosmic rays</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Abe, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Abu-Zayyad, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Allen, M.G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Anderson, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Azuma, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Barcikowski, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Belz, J.W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bergman, D.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Blake, S.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cady, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chae, M.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cheon, B.G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chiba, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chikawa, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Cho, W.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fujii, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Fukushima, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Goto, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hanlon, W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayashi, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hayashida, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hibino, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Honda, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ikeda, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Inoue, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ishii, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ishimori, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ito, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ivanov, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jui, C.C.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kadota, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kakimoto, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kalashev, O.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kasahara, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawai, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawakami, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawana, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kawata, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kido, E.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, H.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, J.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, J.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kitamura, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kitamura, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kuzmin, V.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kwon, Y.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lan, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lim, S.I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lundquist, J.P.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Machida, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Martens, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Matsuda, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Matsuyama, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Matthews, J.N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Minamino, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mukai, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Myers, I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nagasawa, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nagataki, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nakamura, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nonaka, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Nozato, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ogio, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ogura, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ohnishi, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ohoka, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oki, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Okuda, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ono, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Oshima, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ozawa, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Park, I.H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pshirkov, M.S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rodriguez, D.C.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rubtsov, G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ryu, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sagawa, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sakurai, N.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sampson, A.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Scott, L.M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shah, P.D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shibata, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shibata, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shimodaira, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shin, B.K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Shin, H.S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Smith, J.D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Sokolsky, P.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Springer, R.W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stokes, B.T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stratton, S.R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Stroman, T.A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Suzawa, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takamura, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takeda, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takeishi, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Taketa, A.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Takita, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tameda, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tanaka, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tanaka, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tanaka, M.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Thomas, S.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Thomson, G.B.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tinyakov, P.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tkachev, I.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tokuno, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tomida, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Troitsky, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tsunesada, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tsutsumi, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Uchihori, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Udo, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Urban, F.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Vasiloff, G.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wong, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yamane, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yamaoka, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yamazaki, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yang, J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yashiro, K.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yoneda, Y.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yoshida, S.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yoshii, H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zollinger, R.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zundel, Z.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="n">Elsevier Science</subfield><subfield code="t">Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells</subfield><subfield code="d">2012transfer abstract</subfield><subfield code="g">Amsterdam [u.a.]</subfield><subfield code="w">(DE-627)ELV016257995</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:68</subfield><subfield code="g">year:2015</subfield><subfield code="g">pages:27-44</subfield><subfield code="g">extent:18</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1016/j.astropartphys.2015.02.008</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ELV</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_252</subfield></datafield><datafield tag="936" ind1="b" ind2="k"><subfield code="a">50.92</subfield><subfield code="j">Meerestechnik</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">68</subfield><subfield code="j">2015</subfield><subfield code="h">27-44</subfield><subfield code="g">18</subfield></datafield><datafield tag="953" ind1=" " ind2=" "><subfield code="2">045F</subfield><subfield code="a">540</subfield></datafield></record></collection>
|
| score |
7.400714 |