Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow with the IceCube Detector
Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow with the IceCube Detector
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DOI：
10.3847/1538-4357/aaffd1
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发表时间：
2018-11
期刊：
影响因子：
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通讯作者：
I. C. M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;D. Altmann;K. Andeen;T. Anderson;I. Ansseau;G. Anton;C. Arguelles;J. Auffenberg;S. Axani;P. Backes;H. Bagherpour;X. Bai;A. Barbano;J. P. Barron;S. Barwick;V. Baum;R. Bay;J. Beatty;J. Tjus;K. Becker;S. BenZvi;D. Berley;E. Bernardini;D. Besson;G. Binder;D. Bindig;E. Blaufuss;S. Blot;C. Bohm;M. Borner;F. Bos;S. Boser;O. Botner;E. Bourbeau;J. Bourbeau;F. Bradascio;J. Braun;H. Bretz;S. Bron;J. Brostean-Kaiser;A. Burgman;R. Busse;T. Carver;C. Chen;E. Cheung;D. Chirkin;K. Clark;L. Classen;G. Collin;J. Conrad;P. Coppin;P. Correa;D. Cowen;R. Cross;P. Dave;M. Day;J. Andr'e;C. Clercq;J. DeLaunay;H. Dembinski;K. Deoskar;S. Ridder;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;J. C. D'iaz-V'elez;H. Dujmovic;M. Dunkman;E. Dvorak;B. Eberhardt;T. Ehrhardt;B. Eichmann;P. Eller;P. Evenson;S. Fahey;A. Fazely;J. Felde;K. Filimonov;C. Finley;A. Franckowiak;E. Friedman;A. Fritz;T. Gaisser;J. Gallagher;E. Ganster;S. Garrappa;L. Gerhardt;K. Ghorbani;W. Giang;T. Glauch;T. Glusenkamp;A. Goldschmidt;J. G. Gonzalez;D. Grant;Z. Griffith;C. Haack;A. Hallgren;L. Halve;F. Halzen;K. Hanson;D. Hebecker;D. Heereman;K. Helbing;R. Hellauer;S. Hickford;J. Hignight;G. Hill;K. Hoffman;R. Hoffmann;T. Hoinka;B. Hokanson-Fasig;K. Hoshina;F. Huang;M. Huber;K. Hultqvist;Mirco Hünnefeld;R. Hussain;S. In;N. Iovine;A. Ishihara;E. Jacobi;G. Japaridze;M. Jeong;K. Jero;B. Jones;P. Kalaczyński;W. Kang;A. Kappes;D. Kappesser;T. Karg;A. Karle;U. Katz;M. Kauer;A. Keivani;J. Kelley;A. Kheirandish;J. Kim;T. Kintscher;J. Kiryluk;T. Kittler;S. Klein;R. Koirala;H. Kolanoski;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;K. Krings;M. Kroll;G. Kruckl;S. Kunwar;N. Kurahashi;A. Kyriacou;M. Labare;J. Lanfranchi;M. Larson;F. Lauber;K. Leonard;M. Leuermann;Q. Liu;E. Lohfink;C. J. L. Mariscal;L. Lu;J. Lunemann;W. Luszczak;J. Madsen;G. Maggi;K. Mahn;Y. Makino;S. Mancina;I. Marics;R. Maruyama;K. Mase;R. Maunu;K. Meagher;M. Medici;M. Meier;T. Menne;G. Merino;T. Meures;S. Miarecki;J. Micallef;G. Moment'e;T. Montaruli;R. Moore;M. Moulai;R. Nagai;R. Nahnhauer;P. Nakarmi;U. Naumann;G. Neer;H. Niederhausen;S. Nowicki;D. Nygren;A. Pollmann;A. Olivas;A. O'Murchadha;E. O’Sullivan;T. Palczewski;H. Pandya;D. Pankova;P. Peiffer;J. Pepper;C. Heros;D. Pieloth;E. Pinat;A. Pizzuto;M. Plum;P. Price;G. Przybylski;C. Raab;M. Rameez;L. Rauch;K. Rawlins;I. C. Rea;R. Reimann;B. Relethford;G. Renzi;E. Resconi;W. Rhode;M. Richman;S. Robertson;M. Rongen;C. Rott;T. Ruhe;D. Ryckbosch;D. Rysewyk;I. Safa;S. Herrera;A. Sandrock;J. Sandroos;M. Santander;S. Sarkar;K. Satalecka;M. Schaufel;P. Schlunder;T. Schmidt;A. Schneider;J. Schneider;S. Schoneberg;L. Schumacher;S. Sclafani;D. Seckel;S. Seunarine;J. Soedingrekso;D. Soldin;M. Song;G. Spiczak;C. Spiering;J. Stachurska;M. Stamatikos;T. Stanev;Alexander Stasik;R. Stein;J. Stettner;A. Steuer;T. Stezelberger;R. Stokstad;A. Stossl;N. Strotjohann;T. Stuttard;G. Sullivan;M. Sutherland;I. Taboada;F. Tenholt;S. Ter-Antonyan;A. Terliuk;S. Tilav;P. Toale;M. Tobin;C. Tonnis;S. Toscano;D. Tosi;M. Tselengidou;C. Tung;A. Turcati;R. Turcotte;C. Turley;B. Ty;E. Unger;M. U. Elorrieta;M. Usner;J. Vandenbroucke;W. Driessche;D. Eijk;N. Eijndhoven;S. Vanheule;J. Santen;M. Vraeghe;C. Walck;A. Wallace;M. Wallraff;F. Wandler;N. Wandkowsky;T. B. Watson;C. Weaver;M. Weiss;C. Wendt;J. Werthebach;S. Westerhoff;B. Whelan;N. Whitehorn;K. Wiebe;C. Wiebusch;L. Wille;D. Williams;L. Wills;M. Wolf;J. Wood;T. R. Wood;E. Woolsey;K. Woschnagg;G. Wrede;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;T. Yuan
中科院分区：
文献类型：
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作者：
I. C. M. Aartsen;M. Ackermann;J. Adams;J. Aguilar;M. Ahlers;M. Ahrens;D. Altmann;K. Andeen;T. Anderson;I. Ansseau;G. Anton;C. Arguelles;J. Auffenberg;S. Axani;P. Backes;H. Bagherpour;X. Bai;A. Barbano;J. P. Barron;S. Barwick;V. Baum;R. Bay;J. Beatty;J. Tjus;K. Becker;S. BenZvi;D. Berley;E. Bernardini;D. Besson;G. Binder;D. Bindig;E. Blaufuss;S. Blot;C. Bohm;M. Borner;F. Bos;S. Boser;O. Botner;E. Bourbeau;J. Bourbeau;F. Bradascio;J. Braun;H. Bretz;S. Bron;J. Brostean-Kaiser;A. Burgman;R. Busse;T. Carver;C. Chen;E. Cheung;D. Chirkin;K. Clark;L. Classen;G. Collin;J. Conrad;P. Coppin;P. Correa;D. Cowen;R. Cross;P. Dave;M. Day;J. Andr'e;C. Clercq;J. DeLaunay;H. Dembinski;K. Deoskar;S. Ridder;P. Desiati;K. D. Vries;G. Wasseige;M. With;T. DeYoung;J. C. D'iaz-V'elez;H. Dujmovic;M. Dunkman;E. Dvorak;B. Eberhardt;T. Ehrhardt;B. Eichmann;P. Eller;P. Evenson;S. Fahey;A. Fazely;J. Felde;K. Filimonov;C. Finley;A. Franckowiak;E. Friedman;A. Fritz;T. Gaisser;J. Gallagher;E. Ganster;S. Garrappa;L. Gerhardt;K. Ghorbani;W. Giang;T. Glauch;T. Glusenkamp;A. Goldschmidt;J. G. Gonzalez;D. Grant;Z. Griffith;C. Haack;A. Hallgren;L. Halve;F. Halzen;K. Hanson;D. Hebecker;D. Heereman;K. Helbing;R. Hellauer;S. Hickford;J. Hignight;G. Hill;K. Hoffman;R. Hoffmann;T. Hoinka;B. Hokanson-Fasig;K. Hoshina;F. Huang;M. Huber;K. Hultqvist;Mirco Hünnefeld;R. Hussain;S. In;N. Iovine;A. Ishihara;E. Jacobi;G. Japaridze;M. Jeong;K. Jero;B. Jones;P. Kalaczyński;W. Kang;A. Kappes;D. Kappesser;T. Karg;A. Karle;U. Katz;M. Kauer;A. Keivani;J. Kelley;A. Kheirandish;J. Kim;T. Kintscher;J. Kiryluk;T. Kittler;S. Klein;R. Koirala;H. Kolanoski;L. Kopke;C. Kopper;S. Kopper;D. Koskinen;M. Kowalski;K. Krings;M. Kroll;G. Kruckl;S. Kunwar;N. Kurahashi;A. Kyriacou;M. Labare;J. Lanfranchi;M. Larson;F. Lauber;K. Leonard;M. Leuermann;Q. Liu;E. Lohfink;C. J. L. Mariscal;L. Lu;J. Lunemann;W. Luszczak;J. Madsen;G. Maggi;K. Mahn;Y. Makino;S. Mancina;I. Marics;R. Maruyama;K. Mase;R. Maunu;K. Meagher;M. Medici;M. Meier;T. Menne;G. Merino;T. Meures;S. Miarecki;J. Micallef;G. Moment'e;T. Montaruli;R. Moore;M. Moulai;R. Nagai;R. Nahnhauer;P. Nakarmi;U. Naumann;G. Neer;H. Niederhausen;S. Nowicki;D. Nygren;A. Pollmann;A. Olivas;A. O'Murchadha;E. O’Sullivan;T. Palczewski;H. Pandya;D. Pankova;P. Peiffer;J. Pepper;C. Heros;D. Pieloth;E. Pinat;A. Pizzuto;M. Plum;P. Price;G. Przybylski;C. Raab;M. Rameez;L. Rauch;K. Rawlins;I. C. Rea;R. Reimann;B. Relethford;G. Renzi;E. Resconi;W. Rhode;M. Richman;S. Robertson;M. Rongen;C. Rott;T. Ruhe;D. Ryckbosch;D. Rysewyk;I. Safa;S. Herrera;A. Sandrock;J. Sandroos;M. Santander;S. Sarkar;K. Satalecka;M. Schaufel;P. Schlunder;T. Schmidt;A. Schneider;J. Schneider;S. Schoneberg;L. Schumacher;S. Sclafani;D. Seckel;S. Seunarine;J. Soedingrekso;D. Soldin;M. Song;G. Spiczak;C. Spiering;J. Stachurska;M. Stamatikos;T. Stanev;Alexander Stasik;R. Stein;J. Stettner;A. Steuer;T. Stezelberger;R. Stokstad;A. Stossl;N. Strotjohann;T. Stuttard;G. Sullivan;M. Sutherland;I. Taboada;F. Tenholt;S. Ter-Antonyan;A. Terliuk;S. Tilav;P. Toale;M. Tobin;C. Tonnis;S. Toscano;D. Tosi;M. Tselengidou;C. Tung;A. Turcati;R. Turcotte;C. Turley;B. Ty;E. Unger;M. U. Elorrieta;M. Usner;J. Vandenbroucke;W. Driessche;D. Eijk;N. Eijndhoven;S. Vanheule;J. Santen;M. Vraeghe;C. Walck;A. Wallace;M. Wallraff;F. Wandler;N. Wandkowsky;T. B. Watson;C. Weaver;M. Weiss;C. Wendt;J. Werthebach;S. Westerhoff;B. Whelan;N. Whitehorn;K. Wiebe;C. Wiebusch;L. Wille;D. Williams;L. Wills;M. Wolf;J. Wood;T. R. Wood;E. Woolsey;K. Woschnagg;G. Wrede;D. Xu;X. Xu;Y. Xu;J. Yáñez;G. Yodh;S. Yoshida;T. Yuan
我们报告的观测赤字的宇宙射线通量从月球和太阳的方向与五年的数据所采取的冰立方中微子天文台。在2010年5月至2011年5月期间，冰立方探测器在南极的冰川冰中部署了79根弦，在2011年5月至2015年5月期间使用了86根弦。分箱分析用于测量宇宙射线阴影的相对缺陷和重要性。每年检测到的宇宙射线月影和日影都具有很高的统计显著性（>10σ）。月球阴影的结果与之前的分析一致，并验证了IceCube探测器随时间的稳定性。这项工作代表了IceCube探测器对太阳阴影的首次观测。我们证明了太阳的宇宙线阴影随时间而变化。这些结果使得利用IceCube未来的数据研究太阳附近的宇宙射线传输成为可能。
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 detected with high statistical significance (>10σ) for each year. The results for the Moon shadow are consistent with previous analyses and verify the stability of the IceCube detector over time. This work represents the first observation of the Sun shadow with the IceCube detector. We show that the cosmic ray shadow of the Sun varies with time. These results make it possible to study cosmic ray transport near the Sun with future data from IceCube.