The X-Ray Telescope (XRT) for the Hinode Mission
Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability w...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Golub, L. [verfasserIn] DeLuca, E. [verfasserIn] Austin, G. [verfasserIn] Bookbinder, J. [verfasserIn] Caldwell, D. [verfasserIn] Cheimets, P. [verfasserIn] Cirtain, J. [verfasserIn] Cosmo, M. [verfasserIn] Reid, P. [verfasserIn] Sette, A. [verfasserIn] Weber, M. [verfasserIn] Sakao, T. [verfasserIn] Kano, R. [verfasserIn] Shibasaki, K. [verfasserIn] Hara, H. [verfasserIn] Tsuneta, S. [verfasserIn] Kumagai, K. [verfasserIn] Tamura, T. [verfasserIn] Shimojo, M. [verfasserIn] McCracken, J. [verfasserIn] Carpenter, J. [verfasserIn] Haight, H. [verfasserIn] Siler, R. [verfasserIn] Wright, E. [verfasserIn] Tucker, J. [verfasserIn] Rutledge, H. [verfasserIn] Barbera, M. [verfasserIn] Peres, G. [verfasserIn] Varisco, S. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2007 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Dordrecht [u.a.] : Springer Science + Business Media B.V, 1967, 243(2007), 1 vom: Juni, Seite 63-86 |
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| Übergeordnetes Werk: |
volume:243 ; year:2007 ; number:1 ; month:06 ; pages:63-86 |
| Links: |
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| DOI / URN: |
10.1007/s11207-007-0182-1 |
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| Katalog-ID: |
SPR017749069 |
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| 024 | 7 | |a 10.1007/s11207-007-0182-1 |2 doi | |
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| 100 | 1 | |a Golub, L. |e verfasserin |4 aut | |
| 245 | 1 | 4 | |a The X-Ray Telescope (XRT) for the Hinode Mission |
| 264 | 1 | |c 2007 | |
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| 520 | |a Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. | ||
| 650 | 4 | |a Polyimide |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Focal Plane |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Focus Mechanism |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Point Spread Function |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Focus Position |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a DeLuca, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Austin, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Bookbinder, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Caldwell, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Cheimets, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Cirtain, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Cosmo, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Reid, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Sette, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Weber, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Sakao, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Kano, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Shibasaki, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Hara, H. |e verfasserin |4 aut | |
| 700 | 1 | |a Tsuneta, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Kumagai, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Tamura, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Shimojo, M. |e verfasserin |4 aut | |
| 700 | 1 | |a McCracken, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Carpenter, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Haight, H. |e verfasserin |4 aut | |
| 700 | 1 | |a Siler, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Wright, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Tucker, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Rutledge, H. |e verfasserin |4 aut | |
| 700 | 1 | |a Barbera, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Peres, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Varisco, S. |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Solar physics |d Dordrecht [u.a.] : Springer Science + Business Media B.V, 1967 |g 243(2007), 1 vom: Juni, Seite 63-86 |w (DE-627)269019162 |w (DE-600)1473830-2 |x 1573-093X |7 nnns |
| 773 | 1 | 8 | |g volume:243 |g year:2007 |g number:1 |g month:06 |g pages:63-86 |
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10.1007/s11207-007-0182-1 doi (DE-627)SPR017749069 (SPR)s11207-007-0182-1-e DE-627 ger DE-627 rakwb eng 530 ASE 39.51 bkl Golub, L. verfasserin aut The X-Ray Telescope (XRT) for the Hinode Mission 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. Polyimide (dpeaa)DE-He213 Focal Plane (dpeaa)DE-He213 Focus Mechanism (dpeaa)DE-He213 Point Spread Function (dpeaa)DE-He213 Focus Position (dpeaa)DE-He213 DeLuca, E. verfasserin aut Austin, G. verfasserin aut Bookbinder, J. verfasserin aut Caldwell, D. verfasserin aut Cheimets, P. verfasserin aut Cirtain, J. verfasserin aut Cosmo, M. verfasserin aut Reid, P. verfasserin aut Sette, A. verfasserin aut Weber, M. verfasserin aut Sakao, T. verfasserin aut Kano, R. verfasserin aut Shibasaki, K. verfasserin aut Hara, H. verfasserin aut Tsuneta, S. verfasserin aut Kumagai, K. verfasserin aut Tamura, T. verfasserin aut Shimojo, M. verfasserin aut McCracken, J. verfasserin aut Carpenter, J. verfasserin aut Haight, H. verfasserin aut Siler, R. verfasserin aut Wright, E. verfasserin aut Tucker, J. verfasserin aut Rutledge, H. verfasserin aut Barbera, M. verfasserin aut Peres, G. verfasserin aut Varisco, S. verfasserin aut Enthalten in Solar physics Dordrecht [u.a.] : Springer Science + Business Media B.V, 1967 243(2007), 1 vom: Juni, Seite 63-86 (DE-627)269019162 (DE-600)1473830-2 1573-093X nnns volume:243 year:2007 number:1 month:06 pages:63-86 https://dx.doi.org/10.1007/s11207-007-0182-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.51 ASE AR 243 2007 1 06 63-86 |
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10.1007/s11207-007-0182-1 doi (DE-627)SPR017749069 (SPR)s11207-007-0182-1-e DE-627 ger DE-627 rakwb eng 530 ASE 39.51 bkl Golub, L. verfasserin aut The X-Ray Telescope (XRT) for the Hinode Mission 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. Polyimide (dpeaa)DE-He213 Focal Plane (dpeaa)DE-He213 Focus Mechanism (dpeaa)DE-He213 Point Spread Function (dpeaa)DE-He213 Focus Position (dpeaa)DE-He213 DeLuca, E. verfasserin aut Austin, G. verfasserin aut Bookbinder, J. verfasserin aut Caldwell, D. verfasserin aut Cheimets, P. verfasserin aut Cirtain, J. verfasserin aut Cosmo, M. verfasserin aut Reid, P. verfasserin aut Sette, A. verfasserin aut Weber, M. verfasserin aut Sakao, T. verfasserin aut Kano, R. verfasserin aut Shibasaki, K. verfasserin aut Hara, H. verfasserin aut Tsuneta, S. verfasserin aut Kumagai, K. verfasserin aut Tamura, T. verfasserin aut Shimojo, M. verfasserin aut McCracken, J. verfasserin aut Carpenter, J. verfasserin aut Haight, H. verfasserin aut Siler, R. verfasserin aut Wright, E. verfasserin aut Tucker, J. verfasserin aut Rutledge, H. verfasserin aut Barbera, M. verfasserin aut Peres, G. verfasserin aut Varisco, S. verfasserin aut Enthalten in Solar physics Dordrecht [u.a.] : Springer Science + Business Media B.V, 1967 243(2007), 1 vom: Juni, Seite 63-86 (DE-627)269019162 (DE-600)1473830-2 1573-093X nnns volume:243 year:2007 number:1 month:06 pages:63-86 https://dx.doi.org/10.1007/s11207-007-0182-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.51 ASE AR 243 2007 1 06 63-86 |
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10.1007/s11207-007-0182-1 doi (DE-627)SPR017749069 (SPR)s11207-007-0182-1-e DE-627 ger DE-627 rakwb eng 530 ASE 39.51 bkl Golub, L. verfasserin aut The X-Ray Telescope (XRT) for the Hinode Mission 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. Polyimide (dpeaa)DE-He213 Focal Plane (dpeaa)DE-He213 Focus Mechanism (dpeaa)DE-He213 Point Spread Function (dpeaa)DE-He213 Focus Position (dpeaa)DE-He213 DeLuca, E. verfasserin aut Austin, G. verfasserin aut Bookbinder, J. verfasserin aut Caldwell, D. verfasserin aut Cheimets, P. verfasserin aut Cirtain, J. verfasserin aut Cosmo, M. verfasserin aut Reid, P. verfasserin aut Sette, A. verfasserin aut Weber, M. verfasserin aut Sakao, T. verfasserin aut Kano, R. verfasserin aut Shibasaki, K. verfasserin aut Hara, H. verfasserin aut Tsuneta, S. verfasserin aut Kumagai, K. verfasserin aut Tamura, T. verfasserin aut Shimojo, M. verfasserin aut McCracken, J. verfasserin aut Carpenter, J. verfasserin aut Haight, H. verfasserin aut Siler, R. verfasserin aut Wright, E. verfasserin aut Tucker, J. verfasserin aut Rutledge, H. verfasserin aut Barbera, M. verfasserin aut Peres, G. verfasserin aut Varisco, S. verfasserin aut Enthalten in Solar physics Dordrecht [u.a.] : Springer Science + Business Media B.V, 1967 243(2007), 1 vom: Juni, Seite 63-86 (DE-627)269019162 (DE-600)1473830-2 1573-093X nnns volume:243 year:2007 number:1 month:06 pages:63-86 https://dx.doi.org/10.1007/s11207-007-0182-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.51 ASE AR 243 2007 1 06 63-86 |
| allfieldsGer |
10.1007/s11207-007-0182-1 doi (DE-627)SPR017749069 (SPR)s11207-007-0182-1-e DE-627 ger DE-627 rakwb eng 530 ASE 39.51 bkl Golub, L. verfasserin aut The X-Ray Telescope (XRT) for the Hinode Mission 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. Polyimide (dpeaa)DE-He213 Focal Plane (dpeaa)DE-He213 Focus Mechanism (dpeaa)DE-He213 Point Spread Function (dpeaa)DE-He213 Focus Position (dpeaa)DE-He213 DeLuca, E. verfasserin aut Austin, G. verfasserin aut Bookbinder, J. verfasserin aut Caldwell, D. verfasserin aut Cheimets, P. verfasserin aut Cirtain, J. verfasserin aut Cosmo, M. verfasserin aut Reid, P. verfasserin aut Sette, A. verfasserin aut Weber, M. verfasserin aut Sakao, T. verfasserin aut Kano, R. verfasserin aut Shibasaki, K. verfasserin aut Hara, H. verfasserin aut Tsuneta, S. verfasserin aut Kumagai, K. verfasserin aut Tamura, T. verfasserin aut Shimojo, M. verfasserin aut McCracken, J. verfasserin aut Carpenter, J. verfasserin aut Haight, H. verfasserin aut Siler, R. verfasserin aut Wright, E. verfasserin aut Tucker, J. verfasserin aut Rutledge, H. verfasserin aut Barbera, M. verfasserin aut Peres, G. verfasserin aut Varisco, S. verfasserin aut Enthalten in Solar physics Dordrecht [u.a.] : Springer Science + Business Media B.V, 1967 243(2007), 1 vom: Juni, Seite 63-86 (DE-627)269019162 (DE-600)1473830-2 1573-093X nnns volume:243 year:2007 number:1 month:06 pages:63-86 https://dx.doi.org/10.1007/s11207-007-0182-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.51 ASE AR 243 2007 1 06 63-86 |
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10.1007/s11207-007-0182-1 doi (DE-627)SPR017749069 (SPR)s11207-007-0182-1-e DE-627 ger DE-627 rakwb eng 530 ASE 39.51 bkl Golub, L. verfasserin aut The X-Ray Telescope (XRT) for the Hinode Mission 2007 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. Polyimide (dpeaa)DE-He213 Focal Plane (dpeaa)DE-He213 Focus Mechanism (dpeaa)DE-He213 Point Spread Function (dpeaa)DE-He213 Focus Position (dpeaa)DE-He213 DeLuca, E. verfasserin aut Austin, G. verfasserin aut Bookbinder, J. verfasserin aut Caldwell, D. verfasserin aut Cheimets, P. verfasserin aut Cirtain, J. verfasserin aut Cosmo, M. verfasserin aut Reid, P. verfasserin aut Sette, A. verfasserin aut Weber, M. verfasserin aut Sakao, T. verfasserin aut Kano, R. verfasserin aut Shibasaki, K. verfasserin aut Hara, H. verfasserin aut Tsuneta, S. verfasserin aut Kumagai, K. verfasserin aut Tamura, T. verfasserin aut Shimojo, M. verfasserin aut McCracken, J. verfasserin aut Carpenter, J. verfasserin aut Haight, H. verfasserin aut Siler, R. verfasserin aut Wright, E. verfasserin aut Tucker, J. verfasserin aut Rutledge, H. verfasserin aut Barbera, M. verfasserin aut Peres, G. verfasserin aut Varisco, S. verfasserin aut Enthalten in Solar physics Dordrecht [u.a.] : Springer Science + Business Media B.V, 1967 243(2007), 1 vom: Juni, Seite 63-86 (DE-627)269019162 (DE-600)1473830-2 1573-093X nnns volume:243 year:2007 number:1 month:06 pages:63-86 https://dx.doi.org/10.1007/s11207-007-0182-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.51 ASE AR 243 2007 1 06 63-86 |
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Enthalten in Solar physics 243(2007), 1 vom: Juni, Seite 63-86 volume:243 year:2007 number:1 month:06 pages:63-86 |
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Enthalten in Solar physics 243(2007), 1 vom: Juni, Seite 63-86 volume:243 year:2007 number:1 month:06 pages:63-86 |
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Polyimide Focal Plane Focus Mechanism Point Spread Function Focus Position |
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Solar physics |
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Golub, L. @@aut@@ DeLuca, E. @@aut@@ Austin, G. @@aut@@ Bookbinder, J. @@aut@@ Caldwell, D. @@aut@@ Cheimets, P. @@aut@@ Cirtain, J. @@aut@@ Cosmo, M. @@aut@@ Reid, P. @@aut@@ Sette, A. @@aut@@ Weber, M. @@aut@@ Sakao, T. @@aut@@ Kano, R. @@aut@@ Shibasaki, K. @@aut@@ Hara, H. @@aut@@ Tsuneta, S. @@aut@@ Kumagai, K. @@aut@@ Tamura, T. @@aut@@ Shimojo, M. @@aut@@ McCracken, J. @@aut@@ Carpenter, J. @@aut@@ Haight, H. @@aut@@ Siler, R. @@aut@@ Wright, E. @@aut@@ Tucker, J. @@aut@@ Rutledge, H. @@aut@@ Barbera, M. @@aut@@ Peres, G. @@aut@@ Varisco, S. @@aut@@ |
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2007-06-01T00:00:00Z |
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3530 |
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530 ASE 39.51 bkl The X-Ray Telescope (XRT) for the Hinode Mission Polyimide (dpeaa)DE-He213 Focal Plane (dpeaa)DE-He213 Focus Mechanism (dpeaa)DE-He213 Point Spread Function (dpeaa)DE-He213 Focus Position (dpeaa)DE-He213 |
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Golub, L. DeLuca, E. Austin, G. Bookbinder, J. Caldwell, D. Cheimets, P. Cirtain, J. Cosmo, M. Reid, P. Sette, A. Weber, M. Sakao, T. Kano, R. Shibasaki, K. Hara, H. Tsuneta, S. Kumagai, K. Tamura, T. Shimojo, M. McCracken, J. Carpenter, J. Haight, H. Siler, R. Wright, E. Tucker, J. Rutledge, H. Barbera, M. Peres, G. Varisco, S. |
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x-ray telescope (xrt) for the hinode mission |
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The X-Ray Telescope (XRT) for the Hinode Mission |
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Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. |
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Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. |
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Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. The high sensitivity and broad dynamic range of XRT, coupled with the spacecraft’s onboard memory capacity and the planned downlink capability will permit a broad range of coronal studies over an extended period of time, for targets ranging from quiet Sun to X-flares. This paper discusses in detail the design, calibration, and measured performance of the XRT instrument up to the focal plane. The CCD camera and data handling are discussed separately in a companion paper. |
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The X-Ray Telescope (XRT) for the Hinode Mission |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR017749069</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111053425.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201006s2007 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11207-007-0182-1</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR017749069</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11207-007-0182-1-e</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="4"><subfield code="a">530</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.51</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Golub, L.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The X-Ray Telescope (XRT) for the Hinode Mission</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2007</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The X-ray Telescope (XRT) of the Hinode mission provides an unprecedented combination of spatial and temporal resolution in solar coronal studies. 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| score |
7.401602 |