Solar Energetic Particle Spectrum on 2006 December 13 Determined by IceTop

On 2006 December 13 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick Cerenkov detectors with multiple thresholds deployed at high altitude with no geomagnetic cutoff, we determined the par...

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Published inThe Astrophysical journal Vol. 689; no. 1; pp. L65 - L68
Main Authors Adams, J, Ahrens, J, Andeen, K, Bai, X, Bay, R, Bazo Alba, J. L, Becker, J. K, Becker, K. H, Berghaus, P, Bertrand, D, Bieber, J. W, Blaufuss, E, Bohm, C, Böser, S, Chirkin, D, Clem, J, Cowen, D. F, Danninger, M, Dreyer, J, Dumm, J. P, Duvoort, M. R, Ehrlich, R, Eisch, J, Evenson, P. A, Fox, B. D, Gaisser, T. K, Ganugapati, R, Grant, D, Grullon, S, Gurtner, M, Halzen, F, Hanson, K, Helbing, K, Hill, G. C, Hülss, J. P, Hultqvist, K, Hundertmark, S, Jacobsen, J, Japaridze, G. S, Joseph, J. M, Kampert, K. H, Karg, T, Klein, S. R, Kohnen, G, Kolanoski, H, Kowalski, M, Kowarik, T, Krasberg, M, Kuehn, K, Labare, M, Lauer, R, Leich, H, Madsen, J, Matis, H. S, Messarius, T, Mészáros, P, Montaruli, T, Morse, R, Movit, S. M, Nahnhauer, R, Nam, J. W, Niessen, P, Nygren, D. R, Olivas, A, Patton, S, Pérez de los Heros, C, Petrovic, J, Piegsa, A, Pieloth, D, Pohl, A. C, Potthoff, N, Przybylski, G. T, Rizzo, A, Rothmaier, F, Roucelle, C, Rutledge, D, Schlenstedt, S, Schneider, D, Schultz, O, Seckel, D, Seo, S. H, Seunarine, S, Silvestri, A, Smith, A. J, Spiering, C, Stanev, T, Stezelberger, T, Stokstad, R. G, Strahler, E. A, Sulanke, K. H, Swillens, Q, Taboada, I, Tarasova, O, Ter-Antonyan, S, Tilav, S, Tluczykont, M, Waldenmaier, T, Williams, D. R, Wischnewski, R, Yodh, G
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 2008
IOP
Subjects
Online AccessGet full text
ISSN1538-4357
0004-637X
1538-4357
DOI10.1086/595679

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Abstract On 2006 December 13 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick Cerenkov detectors with multiple thresholds deployed at high altitude with no geomagnetic cutoff, we determined the particle energy spectrum in the energy range 0.6-7.6 GeV. This is the first such spectral measurement using a single instrument with a well- defined viewing direction. We compare the IceTop spectrum and its time evolution with previously published results and outline plans for improved resolution of future solar particle spectra.
AbstractList On 2006 December 13 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop tanks, which are thick Cerenkov detectors with multiple thresholds deployed at high altitude with no geomagnetic cutoff, we determined the particle energy spectrum in the energy range 0.6-7.6 GeV. This is the first such spectral measurement using a single instrument with a well-defined viewing direction. We compare the IceTop spectrum and its time evolution with previously published results and outline plans for improved resolution of future solar particle spectra.
Author Wiedemann, C
Christy, B
Kowarik, T
Semburg, B
Tosi, D
Mészáros, P
Schultz, O
Fox, B. D
Olivo, M
Becka, T
Kampert, K. H
Filimonov, K
Smith, A. J
Swillens, Q
Blaufuss, E
Voigt, B
Gurtner, M
Ono, M
Westerhoff, S
Hulth, P. O
Bieber, J. W
Movit, S. M
Karle, A
Depaepe, O
Strahler, E. A
Hanson, K
Pyle, R
Krasberg, M
Pieloth, D
Karg, T
Razzaque, S
Hardtke, D
Meli, A
Seckel, D
Berley, D
Stoyanov, S
Evenson, P. A
Schneider, D
Przybylski, G. T
Kappes, A
Hardtke, R
Sullivan, G. W
Botner, O
Beattie, K
Whitehorn, N
van Eijndhoven, N
Engdegaard, O
de Vries-Uiterweerd, G
Schlenstedt, S
Toale, P. A
Braun, J
Waldmann, H
Sander, H. G
Nygren, D. R
Seunarine, S
Becker, K. H
Price, P. B
Boersma, D. J
Berghaus, P
Köpke, L
Madsen, J
Baker, M
Spiering, C
Ribordy, M
Clem, J
Matis, H. S
Kolanoski, H
Halzen, F
Leich, H
Han, K
Johansson, H
Tluczykont, M
Straszheim, T
De Clercq, C
Redl, P
Vogt, C
Duvoort, M. R
Walter, M
Joseph, J. M
Wendt, C
Rawlins, K
Ackermann, M
Foerster, M. M
Goodman, J. A
Meagher, K
Abbasi, R
Auffenberg, J
Rhode, W
Gerhardt, L
Van Overloop, A
Walck, C
Tilav, S
Viscomi, V
Wischnewski,
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10.1093/rpd/nch175
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Bombardieri (3) 2006; 644
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Snippet On 2006 December 13 the IceTop air shower array at the South Pole detected a major solar particle event. By numerically simulating the response of the IceTop...
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Earth, ocean, space
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Physics
Sun: flares
Sun: particle emission
Title Solar Energetic Particle Spectrum on 2006 December 13 Determined by IceTop
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