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2021
article
Measurements of the time-dependent cosmic-ray Sun shadow with seven years of IceCube data: Comparison with the Solar cycle and magnetic field models
M. G. Aartsen, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, Cyril Martin Alispach, N. M. Amin, K. Andeen, T. Anderson, I. Ansseau, G. Anton, C. Argüelles, J. Auffenberg, Spencer Axani, H. Bagherpour, X. Bai, A. V. Balagopal, Anastasia Maria Barbano, S. W. Barwick, Benjamin Bastian, Vedant Basu, V. Baum, S. Baur, R. Bay, J. J. Beatty, K.-H. Becker, J. Becker Tjus, S. BenZvi, D. Berley, E. Bernardini, D. Besson, G. Binder, D. Bindig, E. Blaufuss, Summer Blot, C. Böhm, S. Böser, O. Botner, J. Böttcher, Etienne Bourbeau, J. Bourbeau, Federica Bradascio, J. Braun, S. Bron, Jannes Brostean-Kaiser, A. Burgman, J. Büscher, Raffaela Busse, T. Carver, C. Chen, E. Cheung, D. Chirkin, S. Choi, Brian Clark, K. Clark, Lew Classen, Alan Coleman, G. H. Collin, J. M. Conrad, Paul Coppin, Pablo Correa, D. F. Cowen, R. Cross, Pranav Dave, C. De Clercq, James DeLaunay, H.-P. Dembinski, Kunal Deoskar, S. De Ridder, Abhishek Desai, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, Sukeerthi Dharani, A. Diaz, J. C. Díaz–Vélez, Hrvoje Dujmović, M. Dunkman, M. A. DuVernois, Emily Dvorak, Thomas Ehrhardt, P. Eller, R. Engel, P. A. Evenson, S. Fahey, A. R. Fazely, J. Felde, H. Fichtner, Aaron Fienberg, K. Filimonov, C. Finley, D. B. Fox, A. Franckowiak, Edward Friedman, Alexander Fritz, T. K. Gaisser, J. S. Gallagher, Erik Ganster, S. Garrappa, L. Gerhardt, Theo Glauch, T. Glüsenkamp, A. Goldschmidt, J. G. González, Sreetama Goswami, D. Grant, T. Grégoire, Z. Griffith, Spencer Griswold, M. Günder, Mehmet Gündüz, Christian Haack, A. Hallgren, R. Halliday, L. Halve, F. Halzen, K. Hanson, John Hardin, A. Haungs, Simon Hauser, D. Hebecker, D. Heereman, P. Heix, K. Helbing, R. Hellauer, Felix Henningsen, S. Hickford, J. Hignight, Colton Hill, G. C. Hill, K. D. Hoffman, R. Hoffmann, Tobias Hoinka, Benjamin Hokanson-Fasig, K. Hoshina, F. Huang, M. E. Huber, Thomas Huber, K. Hultqvist, Mirco Hünnefeld, Raamis Hussain, S. In, N. Iovine, A. Ishihara, Matti Jansson, G. S. Japaridze, Minjin Jeong, B. J. P. Jones, F. Jonske, R. Joppe, Donghwa Kang, Woosik Kang, A. Kappes, David Kappesser, T. Karg, Martina Karl, A. Karle, U. Katz, M. Kauer, Moritz Kellermann, J. L. Kelley, Ali Kheirandish, J. Kim, Ken'ichi Kin, T. Kintscher, J. Kiryluk, T. Kittler, J. Kleimann, Ramesh Koirala, H. Kolanoski, L. Köpke, Claudio Kopper, S. Kopper, D. J. Koskinen, Paras Koundal, M. Kowalski, K. Krings, G. Krückl, N. Kulacz, N. Kurahashi, A. Kyriacou, J. L. Lanfranchi, M. J. Larson, Frederik Hermann Lauber, Jeffrey Lazar, Agnieszka Leszczyńska, Y. Li, Qinrui Liu, Elisa Lohfink, L. Lu, Francesco Lucarelli, Andrew Ludwig, J. Lünemann, William Luszczak, W. Y., J. Madsen, G. Maggi, K. B. M. Mahn, Yuya Makino, P. Mallik, Sarah Mancina, Ioana Codrina Mariş, R. Maruyama, K. Mase, R. Maunu, Frank McNally, K. Meagher, M. Medici, Andrés Medina, Maximilian Meier, S. Meighen-Berger, J. Merz, T. Meures, Jessie Micallef, D. Mockler, G. Momenté, T. Montaruli, R. W. Moore, R. Morse, Marjon Moulai, P. Muth, R. Nagai, Uwe Naumann, G. Neer, Le Viet Nguyen, Hans Niederhausen, M. U. Nisa, Sarah Nowicki, D. R. Nygren, A. Obertacke Pollmann, M. Oehler, A. Olivas, A. O’Murchadha, Erin O’Sullivan, Hershal Pandya, D. V. Pankova, N. Park, Grant Parker, Ek Narayan Paudel, P. Peiffer, C. Pérez de los Heros, Saskia Philippen, D. Pieloth, Sarah Pieper, E. Pinat, A. Pizzuto, M. Plum, Yuriy Popovych, Alessio Porcelli, Maria Prado Rodriguez, P. B. Price, G. T. Przybylski, Christoph Raab, Amirreza Raissi, M. Rameez, L. Rauch, K. Rawlins, I. C. Rea, Abdul Rehman, R. Reimann, B. Relethford, M. Renschler, Giovanni Renzi, E. Resconi, W. Rhode, M. Richman, Benedikt Riedel, S. Robertson, Gerrit Roellinghoff, Martin Rongen, C. Rott, T. Ruhe, D. Ryckbosch, Devyn Rysewyk Cantu, I. Safa, S. E. Sanchez Herrera, Alexander Sandrock, J. Sandroos, M. Santander, S. Sarkar, K. Satalecka, Maximilian Karl Scharf, Merlin Schaufel, H. Schieler, P. Schlunder, T. Schmidt, A. Schneider, Judith Schneider, Frank Schröder, L. Schumacher, S. Sclafani, D. Seckel, S. Seunarine, S. Shefali, M. Silva, B. Smithers, R. Snihur, Jan Soedingrekso, Dennis Soldin, M. Song, G. M. Spiczak, C. Spiering, Juliana Stachurska, M. Stamatikos, Todor Stanev, Robert Stein, J. Stettner, A. Steuer, T. Stezelberger, R. G. Stokstad, N. L. Strotjohann, T. Stürwald, Thomas Stuttard, G. W. Sullivan, I. Taboada, F. Tenholt, S. Ter–Antonyan, A. Terliuk, S. Tilav, Kirsten Tollefson, Lenka Tomankova, Christoph Tönnis, S. Toscano, D. Tosi, Alexander Trettin, M. Tselengidou, C. F. Tung, A. Turcati, Roxanne Turcotte, Colin Turley, B. Ty, E. Unger, Martin Unland Elorrieta, M. Usner, J. Vandenbroucke, W. Van Driessche, D. van Eijk, N. van Eijndhoven, D. Vannerom, J. V. Santen, Stef Verpoest, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, Timothyblake Watson, C. Weaver, A. Weindl, Matthew J. Weiss, Jan Weldert, Chris Wendt, Johannes Werthebach, B. J. Whelan, N. Whitehorn, K. Wiebe, C. H. Wiebusch, D. R. Williams, L. Wills, Martin Wolf, T. R. Wood, K. Woschnagg, Gerrit Wrede, Johan Wilfried Wulff, Xiaolin Xu, Yunlin Xu, S. Yoshida, Tianlu Yuan, Z. Zhang, M. Zöcklein
19Citations signalées — pas une note de qualité
50Institutions déclarées
12Pays d’affiliation déclarés
Résumé fourni par la source
Observations of the time-dependent cosmic-ray Sun shadow have been proven as a valuable diagnostic for the assessment of solar magnetic field models. In this paper, seven years of IceCube data are compared to solar activity and solar magnetic field models. A quantitative comparison of solar magnetic field models with IceCube data on the event rate level is performed for the first time. Additionally, a first energy-dependent analysis is presented and compared to recent predictions. We use seven years of IceCube data for the moon and the Sun and compare them to simulations on data rate level. The simulations are performed for the geometrical shadow hypothesis for the moon and the Sun and for a cosmic-ray propagation model governed by the solar magnetic field for the case of the Sun. We find that a linearly decreasing relationship between Sun shadow strength and solar activity is preferred over a constant relationship at the $6.4\ensuremath{\sigma}$ level. We test two commonly used models of the coronal magnetic field, both combined with a Parker spiral, by modeling cosmic-ray propagation in the solar magnetic field. Both models predict a weakening of the shadow in times of high solar activity as it is also visible in the data. We find tensions with the data on the order of $3\ensuremath{\sigma}$ for both models, assuming only statistical uncertainties. The magnetic field model CSSS fits the data slightly better than the PFSS model. This is generally consistent with what is found previously by the Tibet $\mathrm{AS}\text{\ensuremath{-}}\ensuremath{\gamma}$ Experiment; a deviation of the data from the two models is, however, not significant at this point. Regarding the energy dependence of the Sun shadow, we find indications that the shadowing effect increases with energy during times of high solar activity, in agreement with theoretical predictions.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Measurements of the time-dependent cosmic-ray Sun shadow with seven years of IceCube data: Comparison with the Solar cycle and magnetic field models
- Date Crossref
- 08/02/2021
- Éditeur
- American Physical Society (APS)
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude et ne compte pas comme une seconde source scientifique indépendante.
Institutions déclarées
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Sujets associés
Solar and Space Plasma DynamicsIonosphere and magnetosphere dynamicsAstrophysics and Cosmic Phenomena