Detection of the temporal variation of the Sun's cosmic ray shadow with
  the IceCube detector

IceCube Collaboration; Aartsen, MG; Ackermann, M; Adams, J; Aguilar, JA; Ahlers, M; Ahrens, M; Altmann, D; Andeen, K; Anderson, T; Ansseau, I; Anton, G; Argüelles, C; Auffenberg, J; Axani, S; Backes, P; Bagherpour, H; Bai, X; Barbano, A; Barron, JP; Barwick, SW; Baum, V; Bay, R; Beatty, JJ; Tjus, JB; Becker, K-H; Benzvi, S; Berley, D; Bernardini, E; Besson, DZ; Binder, G; Bindig, D; Blaufuss, E; Blot, S; Bohm, C; Börner, M; Bos, F; Böser, S; Botner, O; Bourbeau, E; Bourbeau, J; Bradascio, F; Braun, J; Bretz, H-P; Bron, S; Brostean-Kaiser, J; Burgman, A; Busse, RS; Carver, T; Chen, C; Cheung, E; Chirkin, D; Clark, K; Classen, L; Collin, GH; Conrad, JM; Coppin, P; Correa, P; Cowen, DF; Cross, R; Dave, P; Day, M; André, JPAMD; Clercq, CD; Delaunay, JJ; Dembinski, H; Deoskar, K; Ridder, SD; Desiati, P; Vries, KDD; Wasseige, GD; With, MD; Deyoung, T; Díaz-Vélez, JC; Dujmovic, H; Dunkman, M; Dvorak, E; Eberhardt, B; Ehrhardt, T; Eichmann, B; Eller, P; Evenson, PA; Fahey, S; Fazely, AR; Felde, J; Filimonov, K; Finley, C; Franckowiak, A; Friedman, E; Fritz, A; Gaisser, TK; Gallagher, J; Ganster, E; Garrappa, S; Gerhardt, L; Ghorbani, K; Giang, W; Glauch, T; Glüsenkamp, T; Goldschmidt, A; Gonzalez, JG; Grant, D; Griffith, Z; Haack, C; Hallgren, A; Halve, L; Halzen, F; Hanson, K; Hebecker, D; Heereman, D; Helbing, K; Hellauer, R; Hickford, S; Hignight, J; Hill, GC; Hoffman, KD; Hoffmann, R; Hoinka, T; Hokanson-Fasig, B; Hoshina, K; Huang, F; Huber, M; Hultqvist, K; Hünnefeld, M; Hussain, R; In, S; Iovine, N; Ishihara, A; Jacobi, E; Japaridze, GS; Jeong, M; Jero, K; Jones, BJP; Kalaczynski, P; Kang, W; Kappes, A; Kappesser, D; Karg, T; Karle, A; Katz, U; Kauer, M; Keivani, A; Kelley, JL; Kheirandish, A; Kim, J; Kintscher, T; Kiryluk, J; Kittler, T; Klein, SR; Koirala, R; Kolanoski, H; Köpke, L; Kopper, C; Kopper, S; Koskinen, DJ; Kowalski, M; Krings, K; Kroll, M; Krückl, G; Kunwar, S; Kurahashi, N; Kyriacou, A; Labare, M; Lanfranchi, JL; Larson, MJ; Lauber, F; Leonard, K; Leuermann, M; Liu, QR; Lohfink, E; Mariscal, CJL; Lu, L; Lünemann, J; Luszczak, W; Madsen, J; Maggi, G; Mahn, KBM; Makino, Y; Mancina, S; Mariş, IC; Maruyama, R; Mase, K; Maunu, R; Meagher, K; Medici, M; Meier, M; Menne, T; Merino, G; Meures, T; Miarecki, S; Micallef, J; Momenté, G; Montaruli, T; Moore, RW; Moulai, M; Nagai, R; Nahnhauer, R; Nakarmi, P; Naumann, U; Neer, G; Niederhausen, H; Nowicki, SC; Nygren, DR; Pollmann, AO; Olivas, A; O'Murchadha, A; O'Sullivan, E; Palczewski, T; Pandya, H; Pankova, DV; Peiffer, P; Pepper, JA; Heros, CPDL; Pieloth, D; Pinat, E; Pizzuto, A; Plum, M; Price, PB; Przybylski, GT; Raab, C; Rameez, M; Rauch, L; Rawlins, K; Rea, IC; Reimann, R; Relethford, B; Renzi, G; Resconi, E; Rhode, W; Richman, M; Robertson, S; Rongen, M; Rott, C; Ruhe, T; Ryckbosch, D; Rysewyk, D; Safa, I; Herrera, SES; Sandrock, A; Sandroos, J; Santander, M; Sarkar, S; Sarkar, S; Satalecka, K; Schaufel, M; Schlunder, P; Schmidt, T; Schneider, A; Schneider, J; Schöneberg, S; Schumacher, L; Sclafani, S; Seckel, D; Seunarine, S; Soedingrekso, J; Soldin, D; Song, M; Spiczak, GM; Spiering, C; Stachurska, J; Stamatikos, M; Stanev, T; Stasik, A; Stein, R; Stettner, J; Steuer, A; Stezelberger, T; Stokstad, RG; Stößl, A; Strotjohann, NL; Stuttard, T; Sullivan, GW; Sutherland, M; Taboada, I; Tenholt, F; Ter-Antonyan, S; Terliuk, A; Tilav, S; Toale, PA; Tobin, MN; Tönnis, C; Toscano, S; Tosi, D; Tselengidou, M; Tung, CF; Turcati, A; Turcotte, R; Turley, CF; Ty, B; Unger, E; Elorrieta, MAU; Usner, M; Vandenbroucke, J; Driessche, WV; Eijk, DV; Eijndhoven, NV; Vanheule, S; Santen, JV; Vraeghe, M; Walck, C; Wallace, A; Wallraff, M; Wandler, FD; Wandkowsky, N; Watson, TB; Weaver, C; Weiss, MJ; Wendt, C; Werthebach, J; Westerhoff, S; Whelan, BJ; Whitehorn, N; Wiebe, K; Wiebusch, CH; Wille, L; Williams, DR; Wills, L; Wolf, M; Wood, J; Wood, TR; Woolsey, E; Woschnagg, K; Wrede, G; Xu, DL; Xu, XW; Xu, Y; Yanez, JP; Yodh, G; Yoshida, S; Yuan, T

Journal article

Detection of the temporal variation of the Sun's cosmic ray shadow with the IceCube detector

Abstract:: We report on the observation of a deficit in the cosmic ray flux from the directions of the Moon and Sun with five years of data taken by the IceCube Neutrino Observatory. Between 2010 May and 2011 May the IceCube detector operated with 79 strings deployed in the glacial ice at the South Pole, and with 86 strings between 2011 May and 2015 May. A binned analysis is used to measure the relative deficit and significance of the cosmic ray shadows. Both the cosmic ray Moon and Sun shadows are dete...
Expand abstract
Collapse abstract

Publication status:: Published

Peer review status:: Peer reviewed

Actions

Email

Email this record

Send the bibliographic details of this record to your email address.

Your Email
Please enter the email address that the record information will be sent to.

-
Your message (optional)
Please add any additional information to be included within the email.
Cite

Cite this record

APA Style

Collaboration, I. C., Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., Barbano, A., … Yuan, T. (2019). Detection of the temporal variation of the Sun's cosmic ray shadow with the IceCube detector. Astrophysical Journal, 872(2).

MLA Style

Collaboration, IceCube, et al. “Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow With the IceCube Detector.” Astrophysical Journal, vol. 872, no. 2, American Astronomical Society, 2019.

Chicago Style

Collaboration, IceCube, MG Aartsen, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, et al. 2019. “Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow With the IceCube Detector.” Astrophysical Journal 872 (2).
Tweet
Print