Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf
The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the sig...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Barwick, S.W. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017transfer abstract |
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| Umfang: |
19 |
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| Übergeordnetes Werk: |
Enthalten in: Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells - 2012transfer abstract, Amsterdam [u.a.] |
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| Übergeordnetes Werk: |
volume:90 ; year:2017 ; pages:50-68 ; extent:19 |
| Links: |
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| DOI / URN: |
10.1016/j.astropartphys.2017.02.003 |
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| 520 | |a The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. | ||
| 520 | |a The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. | ||
| 700 | 1 | |a Besson, D.Z. |4 oth | |
| 700 | 1 | |a Burgman, A. |4 oth | |
| 700 | 1 | |a Chiem, E. |4 oth | |
| 700 | 1 | |a Hallgren, A. |4 oth | |
| 700 | 1 | |a Hanson, J.C. |4 oth | |
| 700 | 1 | |a Klein, S.R. |4 oth | |
| 700 | 1 | |a Kleinfelder, S.A. |4 oth | |
| 700 | 1 | |a Nelles, A. |4 oth | |
| 700 | 1 | |a Persichilli, C. |4 oth | |
| 700 | 1 | |a Phillips, S. |4 oth | |
| 700 | 1 | |a Prakash, T. |4 oth | |
| 700 | 1 | |a Reed, C. |4 oth | |
| 700 | 1 | |a Shively, S.R. |4 oth | |
| 700 | 1 | |a Tatar, J. |4 oth | |
| 700 | 1 | |a Unger, E. |4 oth | |
| 700 | 1 | |a Walker, J. |4 oth | |
| 700 | 1 | |a Yodh, G. |4 oth | |
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10.1016/j.astropartphys.2017.02.003 doi GBVA2017015000002.pica (DE-627)ELV036004251 (ELSEVIER)S0927-6505(16)30213-4 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Barwick, S.W. verfasserin aut Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf 2017transfer abstract 19 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. Besson, D.Z. oth Burgman, A. oth Chiem, E. oth Hallgren, A. oth Hanson, J.C. oth Klein, S.R. oth Kleinfelder, S.A. oth Nelles, A. oth Persichilli, C. oth Phillips, S. oth Prakash, T. oth Reed, C. oth Shively, S.R. oth Tatar, J. oth Unger, E. oth Walker, J. oth Yodh, G. 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:90 year:2017 pages:50-68 extent:19 https://doi.org/10.1016/j.astropartphys.2017.02.003 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 90 2017 50-68 19 045F 540 |
| spelling |
10.1016/j.astropartphys.2017.02.003 doi GBVA2017015000002.pica (DE-627)ELV036004251 (ELSEVIER)S0927-6505(16)30213-4 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Barwick, S.W. verfasserin aut Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf 2017transfer abstract 19 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. Besson, D.Z. oth Burgman, A. oth Chiem, E. oth Hallgren, A. oth Hanson, J.C. oth Klein, S.R. oth Kleinfelder, S.A. oth Nelles, A. oth Persichilli, C. oth Phillips, S. oth Prakash, T. oth Reed, C. oth Shively, S.R. oth Tatar, J. oth Unger, E. oth Walker, J. oth Yodh, G. 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:90 year:2017 pages:50-68 extent:19 https://doi.org/10.1016/j.astropartphys.2017.02.003 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 90 2017 50-68 19 045F 540 |
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10.1016/j.astropartphys.2017.02.003 doi GBVA2017015000002.pica (DE-627)ELV036004251 (ELSEVIER)S0927-6505(16)30213-4 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Barwick, S.W. verfasserin aut Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf 2017transfer abstract 19 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. Besson, D.Z. oth Burgman, A. oth Chiem, E. oth Hallgren, A. oth Hanson, J.C. oth Klein, S.R. oth Kleinfelder, S.A. oth Nelles, A. oth Persichilli, C. oth Phillips, S. oth Prakash, T. oth Reed, C. oth Shively, S.R. oth Tatar, J. oth Unger, E. oth Walker, J. oth Yodh, G. 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:90 year:2017 pages:50-68 extent:19 https://doi.org/10.1016/j.astropartphys.2017.02.003 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 90 2017 50-68 19 045F 540 |
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10.1016/j.astropartphys.2017.02.003 doi GBVA2017015000002.pica (DE-627)ELV036004251 (ELSEVIER)S0927-6505(16)30213-4 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Barwick, S.W. verfasserin aut Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf 2017transfer abstract 19 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. Besson, D.Z. oth Burgman, A. oth Chiem, E. oth Hallgren, A. oth Hanson, J.C. oth Klein, S.R. oth Kleinfelder, S.A. oth Nelles, A. oth Persichilli, C. oth Phillips, S. oth Prakash, T. oth Reed, C. oth Shively, S.R. oth Tatar, J. oth Unger, E. oth Walker, J. oth Yodh, G. 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:90 year:2017 pages:50-68 extent:19 https://doi.org/10.1016/j.astropartphys.2017.02.003 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 90 2017 50-68 19 045F 540 |
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10.1016/j.astropartphys.2017.02.003 doi GBVA2017015000002.pica (DE-627)ELV036004251 (ELSEVIER)S0927-6505(16)30213-4 DE-627 ger DE-627 rakwb eng 540 540 DE-600 620 VZ 690 VZ 50.92 bkl Barwick, S.W. verfasserin aut Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf 2017transfer abstract 19 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. Besson, D.Z. oth Burgman, A. oth Chiem, E. oth Hallgren, A. oth Hanson, J.C. oth Klein, S.R. oth Kleinfelder, S.A. oth Nelles, A. oth Persichilli, C. oth Phillips, S. oth Prakash, T. oth Reed, C. oth Shively, S.R. oth Tatar, J. oth Unger, E. oth Walker, J. oth Yodh, G. 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:90 year:2017 pages:50-68 extent:19 https://doi.org/10.1016/j.astropartphys.2017.02.003 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_252 50.92 Meerestechnik VZ AR 90 2017 50-68 19 045F 540 |
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Enthalten in Flexible, metal-free composite counter electrodes for efficient fiber-shaped dye-sensitized solar cells Amsterdam [u.a.] volume:90 year:2017 pages:50-68 extent:19 |
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Barwick, S.W. @@aut@@ Besson, D.Z. @@oth@@ Burgman, A. @@oth@@ Chiem, E. @@oth@@ Hallgren, A. @@oth@@ Hanson, J.C. @@oth@@ Klein, S.R. @@oth@@ Kleinfelder, S.A. @@oth@@ Nelles, A. @@oth@@ Persichilli, C. @@oth@@ Phillips, S. @@oth@@ Prakash, T. @@oth@@ Reed, C. @@oth@@ Shively, S.R. @@oth@@ Tatar, J. @@oth@@ Unger, E. @@oth@@ Walker, J. @@oth@@ Yodh, G. @@oth@@ |
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Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf |
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The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. |
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The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. |
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The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 1016 eV. The most neutrino-like background stems from the radio emission of air showers. This article reports on dedicated efforts of simulating and detecting the signals of cosmic rays. A description of the fully radio self-triggered data-set, the properties of the detected air shower signals in the frequency range of 100–500 MHz and the consequences for neutrino detection are given. 38 air shower signals are identified by their distinct waveform characteristics, are in good agreement with simulations and their signals provide evidence that neutrino-induced radio signals will be distinguishable with high efficiency in ARIANNA. The cosmic ray flux at a mean energy of 6 . 5 − 1.0 + 1.2 × 10 17 eV is measured to be 1 . 1 − 0.7 + 1.0 × 10 − 16 eV − 1 km − 2 sr − 1 yr − 1 and one five-fold coincident event is used to illustrate the capabilities of the ARIANNA detector to reconstruct arrival direction and energy of air showers. |
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