All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field
We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular p...
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creator | Arteaga-Velázquez, J. C. BenZvi, S. Y. Brisbois, C. Casanova, S. Cotti, U. Cotzomi, J. Fiorino, D. W. Hampel-Arias, Z. Hueyotl-Zahuantitla, F. Malone, K. Miranda-Romagnoli, P. Pretz, J. Schneider, M. Surajbali, P. Tollefson, K. Wood, J. Adams, J. Aguilar, J. A. Anton, G. Argüelles, C. Auffenberg, J. Axani, S. Barron, J. P. Berley, D. Bernardini, Elisa Binder, G. Blaufuss, E. Blot, S. Bourbeau, E. Bradascio, F. Brostean-Kaiser, J. Cheung, E. Classen, L. Coppin, P. Dave, P. Day, M. Desiati, P. DeYoung, T. Dujmovic, H. Eberhardt, B. Ehrhardt, T. Filimonov, K. Friedman, E. Ghorbani, K. Gonzalez, J. G. Heereman, D. Helbing, K. Hickford, S. Huang, F. Huber, M. Kang, W. Karg, T. Katz, U. Kelley, J. L. Kintscher, T. Kittler, T. Köpke, L. Kowalski, Marek Kurahashi, N. Labare, M. Larson, M. J. Leuermann, M. Liu, Q. R. Maggi, G. Mariş, I. C. Maunu, R. Meagher, K. Miarecki, S. Momenté, G. Moulai, M. Nahnhauer, R. Pérez De Los Heros, C. Pinat, E. Plum, M. Rameez, M. Reimann, R. Robertson, S. Rysewyk, D. Santander, M. Schneider, A. Sclafani, S. Seckel, D. Seunarine, S. Soldin, D. Song, M. Stasik, A. Sullivan, G. W. Tenholt, F. Ter-Antonyan, S. Tilav, S. Vandenbroucke, J. Van Eijk, D. Van Eijndhoven, N. Watson, T. B. Weaver, C. Whitehorn, N. Wood, T. R. Woschnagg, K. Xu, Y. Yanez, J. P. |
description | We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and present a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map, we determine the horizontal dipole components of the anisotropy δ 0h = 9.16 × 10−4 and δ 6h = 7.25 × 10−4 (±0.04 × 10−4). In addition, we infer the direction (2292 ± 35 R.A., 114 ± 30 decl.) of the interstellar magnetic field from the boundary between large-scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large-scale anisotropy to be . |
doi_str_mv | 10.3204/pubdb-2020-00512 |
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Y. ; Brisbois, C. ; Casanova, S. ; Cotti, U. ; Cotzomi, J. ; Fiorino, D. W. ; Hampel-Arias, Z. ; Hueyotl-Zahuantitla, F. ; Malone, K. ; Miranda-Romagnoli, P. ; Pretz, J. ; Schneider, M. ; Surajbali, P. ; Tollefson, K. ; Wood, J. ; Adams, J. ; Aguilar, J. A. ; Anton, G. ; Argüelles, C. ; Auffenberg, J. ; Axani, S. ; Barron, J. P. ; Berley, D. ; Bernardini, Elisa ; Binder, G. ; Blaufuss, E. ; Blot, S. ; Bourbeau, E. ; Bradascio, F. ; Brostean-Kaiser, J. ; Cheung, E. ; Classen, L. ; Coppin, P. ; Dave, P. ; Day, M. ; Desiati, P. ; DeYoung, T. ; Dujmovic, H. ; Eberhardt, B. ; Ehrhardt, T. ; Filimonov, K. ; Friedman, E. ; Ghorbani, K. ; Gonzalez, J. G. ; Heereman, D. ; Helbing, K. ; Hickford, S. ; Huang, F. ; Huber, M. ; Kang, W. ; Karg, T. ; Katz, U. ; Kelley, J. L. ; Kintscher, T. ; Kittler, T. ; Köpke, L. ; Kowalski, Marek ; Kurahashi, N. ; Labare, M. ; Larson, M. J. ; Leuermann, M. ; Liu, Q. R. ; Maggi, G. ; Mariş, I. C. ; Maunu, R. ; Meagher, K. ; Miarecki, S. ; Momenté, G. ; Moulai, M. ; Nahnhauer, R. ; Pérez De Los Heros, C. ; Pinat, E. ; Plum, M. ; Rameez, M. ; Reimann, R. ; Robertson, S. ; Rysewyk, D. ; Santander, M. ; Schneider, A. ; Sclafani, S. ; Seckel, D. ; Seunarine, S. ; Soldin, D. ; Song, M. ; Stasik, A. ; Sullivan, G. W. ; Tenholt, F. ; Ter-Antonyan, S. ; Tilav, S. ; Vandenbroucke, J. ; Van Eijk, D. ; Van Eijndhoven, N. ; Watson, T. B. ; Weaver, C. ; Whitehorn, N. ; Wood, T. R. ; Woschnagg, K. ; Xu, Y. ; Yanez, J. P.</creator><creatorcontrib>Arteaga-Velázquez, J. C. ; BenZvi, S. Y. ; Brisbois, C. ; Casanova, S. ; Cotti, U. ; Cotzomi, J. ; Fiorino, D. W. ; Hampel-Arias, Z. ; Hueyotl-Zahuantitla, F. ; Malone, K. ; Miranda-Romagnoli, P. ; Pretz, J. ; Schneider, M. ; Surajbali, P. ; Tollefson, K. ; Wood, J. ; Adams, J. ; Aguilar, J. A. ; Anton, G. ; Argüelles, C. ; Auffenberg, J. ; Axani, S. ; Barron, J. P. ; Berley, D. ; Bernardini, Elisa ; Binder, G. ; Blaufuss, E. ; Blot, S. ; Bourbeau, E. ; Bradascio, F. ; Brostean-Kaiser, J. ; Cheung, E. ; Classen, L. ; Coppin, P. ; Dave, P. ; Day, M. ; Desiati, P. ; DeYoung, T. ; Dujmovic, H. ; Eberhardt, B. ; Ehrhardt, T. ; Filimonov, K. ; Friedman, E. ; Ghorbani, K. ; Gonzalez, J. G. ; Heereman, D. ; Helbing, K. ; Hickford, S. ; Huang, F. ; Huber, M. ; Kang, W. ; Karg, T. ; Katz, U. ; Kelley, J. L. ; Kintscher, T. ; Kittler, T. ; Köpke, L. ; Kowalski, Marek ; Kurahashi, N. ; Labare, M. ; Larson, M. J. ; Leuermann, M. ; Liu, Q. R. ; Maggi, G. ; Mariş, I. C. ; Maunu, R. ; Meagher, K. ; Miarecki, S. ; Momenté, G. ; Moulai, M. ; Nahnhauer, R. ; Pérez De Los Heros, C. ; Pinat, E. ; Plum, M. ; Rameez, M. ; Reimann, R. ; Robertson, S. ; Rysewyk, D. ; Santander, M. ; Schneider, A. ; Sclafani, S. ; Seckel, D. ; Seunarine, S. ; Soldin, D. ; Song, M. ; Stasik, A. ; Sullivan, G. W. ; Tenholt, F. ; Ter-Antonyan, S. ; Tilav, S. ; Vandenbroucke, J. ; Van Eijk, D. ; Van Eijndhoven, N. ; Watson, T. B. ; Weaver, C. ; Whitehorn, N. ; Wood, T. R. ; Woschnagg, K. ; Xu, Y. ; Yanez, J. P.</creatorcontrib><description>We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and present a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map, we determine the horizontal dipole components of the anisotropy δ 0h = 9.16 × 10−4 and δ 6h = 7.25 × 10−4 (±0.04 × 10−4). In addition, we infer the direction (2292 ± 35 R.A., 114 ± 30 decl.) of the interstellar magnetic field from the boundary between large-scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large-scale anisotropy to be .</description><identifier>ISSN: 0004-637X</identifier><identifier>ISSN: 1538-4357</identifier><identifier>DOI: 10.3204/pubdb-2020-00512</identifier><language>eng</language><publisher>Deutsches Elektronen-Synchrotron, DESY, Hamburg</publisher><subject>cosmic radiation: anisotropy ; cosmic radiation: TeV ; dipole ; HAWC ; IceCube ; magnetic field ; observatory ; particle: energy ; power spectrum: angular dependence ; propagation</subject><creationdate>2019</creationdate><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0001-8594-8666 ; 0000-0003-3251-2126 ; 0000-0003-3108-1141 ; 0000-0002-7669-266X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>776,780,1888,4476,27902</link.rule.ids><linktorsrc>$$Uhttps://commons.datacite.org/doi.org/10.3204/pubdb-2020-00512$$EView_record_in_DataCite.org$$FView_record_in_$$GDataCite.org</linktorsrc></links><search><creatorcontrib>Arteaga-Velázquez, J. 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P.</creatorcontrib><title>All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field</title><addtitle>The astrophysical journal / 1 Part 1 871(1)</addtitle><description>We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and present a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map, we determine the horizontal dipole components of the anisotropy δ 0h = 9.16 × 10−4 and δ 6h = 7.25 × 10−4 (±0.04 × 10−4). In addition, we infer the direction (2292 ± 35 R.A., 114 ± 30 decl.) of the interstellar magnetic field from the boundary between large-scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large-scale anisotropy to be .</description><subject>cosmic radiation: anisotropy</subject><subject>cosmic radiation: TeV</subject><subject>dipole</subject><subject>HAWC</subject><subject>IceCube</subject><subject>magnetic field</subject><subject>observatory</subject><subject>particle: energy</subject><subject>power spectrum: angular dependence</subject><subject>propagation</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>report</rsrctype><creationdate>2019</creationdate><recordtype>report</recordtype><sourceid>PQ8</sourceid><recordid>eNqdj71OAzEQhF0EifDTU-4LGPZ8AZQyiohAShqIEJ21udsEB59t2Zvi3p5cFF6AajSj-YpPqbsK72uDk4d02LQbbdCgRnyszEiNEXGin-rnr0t1Vcp-qGY6Hasy815__PSwYiqHzB0HgbgF-WaYBVei5Jj6YZnH0rkG3qkvQAIVwpo_gUILK0rJhd0ftowNeXgLwrkIe0_5-NgFliO9cOzbG3WxJV_49pzXChcv6_mrbkmoccI2ZddR7m2FdhCyJyE7CNmTUP0P5Bc9LlbP</recordid><startdate>2019</startdate><enddate>2019</enddate><creator>Arteaga-Velázquez, J. 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P.</creator><creator>Berley, D.</creator><creator>Bernardini, Elisa</creator><creator>Binder, G.</creator><creator>Blaufuss, E.</creator><creator>Blot, S.</creator><creator>Bourbeau, E.</creator><creator>Bradascio, F.</creator><creator>Brostean-Kaiser, J.</creator><creator>Cheung, E.</creator><creator>Classen, L.</creator><creator>Coppin, P.</creator><creator>Dave, P.</creator><creator>Day, M.</creator><creator>Desiati, P.</creator><creator>DeYoung, T.</creator><creator>Dujmovic, H.</creator><creator>Eberhardt, B.</creator><creator>Ehrhardt, T.</creator><creator>Filimonov, K.</creator><creator>Friedman, E.</creator><creator>Ghorbani, K.</creator><creator>Gonzalez, J. G.</creator><creator>Heereman, D.</creator><creator>Helbing, K.</creator><creator>Hickford, S.</creator><creator>Huang, F.</creator><creator>Huber, M.</creator><creator>Kang, W.</creator><creator>Karg, T.</creator><creator>Katz, U.</creator><creator>Kelley, J. 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R.</creator><creator>Woschnagg, K.</creator><creator>Xu, Y.</creator><creator>Yanez, J. P.</creator><general>Deutsches Elektronen-Synchrotron, DESY, Hamburg</general><scope>PQ8</scope><orcidid>https://orcid.org/0000-0001-8594-8666</orcidid><orcidid>https://orcid.org/0000-0003-3251-2126</orcidid><orcidid>https://orcid.org/0000-0003-3108-1141</orcidid><orcidid>https://orcid.org/0000-0002-7669-266X</orcidid></search><sort><creationdate>2019</creationdate><title>All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field</title><author>Arteaga-Velázquez, J. C. ; BenZvi, S. Y. ; Brisbois, C. ; Casanova, S. ; Cotti, U. ; Cotzomi, J. ; Fiorino, D. W. ; Hampel-Arias, Z. ; Hueyotl-Zahuantitla, F. ; Malone, K. ; Miranda-Romagnoli, P. ; Pretz, J. ; Schneider, M. ; Surajbali, P. ; Tollefson, K. ; Wood, J. ; Adams, J. ; Aguilar, J. A. ; Anton, G. ; Argüelles, C. ; Auffenberg, J. ; Axani, S. ; Barron, J. P. ; Berley, D. ; Bernardini, Elisa ; Binder, G. ; Blaufuss, E. ; Blot, S. ; Bourbeau, E. ; Bradascio, F. ; Brostean-Kaiser, J. ; Cheung, E. ; Classen, L. ; Coppin, P. ; Dave, P. ; Day, M. ; Desiati, P. ; DeYoung, T. ; Dujmovic, H. ; Eberhardt, B. ; Ehrhardt, T. ; Filimonov, K. ; Friedman, E. ; Ghorbani, K. ; Gonzalez, J. G. ; Heereman, D. ; Helbing, K. ; Hickford, S. ; Huang, F. ; Huber, M. ; Kang, W. ; Karg, T. ; Katz, U. ; Kelley, J. L. ; Kintscher, T. ; Kittler, T. ; Köpke, L. ; Kowalski, Marek ; Kurahashi, N. ; Labare, M. ; Larson, M. J. ; Leuermann, M. ; Liu, Q. R. ; Maggi, G. ; Mariş, I. C. ; Maunu, R. ; Meagher, K. ; Miarecki, S. ; Momenté, G. ; Moulai, M. ; Nahnhauer, R. ; Pérez De Los Heros, C. ; Pinat, E. ; Plum, M. ; Rameez, M. ; Reimann, R. ; Robertson, S. ; Rysewyk, D. ; Santander, M. ; Schneider, A. ; Sclafani, S. ; Seckel, D. ; Seunarine, S. ; Soldin, D. ; Song, M. ; Stasik, A. ; Sullivan, G. W. ; Tenholt, F. ; Ter-Antonyan, S. ; Tilav, S. ; Vandenbroucke, J. ; Van Eijk, D. ; Van Eijndhoven, N. ; Watson, T. B. ; Weaver, C. ; Whitehorn, N. ; Wood, T. R. ; Woschnagg, K. ; Xu, Y. ; Yanez, J. P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-datacite_primary_10_3204_pubdb_2020_005123</frbrgroupid><rsrctype>reports</rsrctype><prefilter>reports</prefilter><language>eng</language><creationdate>2019</creationdate><topic>cosmic radiation: anisotropy</topic><topic>cosmic radiation: TeV</topic><topic>dipole</topic><topic>HAWC</topic><topic>IceCube</topic><topic>magnetic field</topic><topic>observatory</topic><topic>particle: energy</topic><topic>power spectrum: angular dependence</topic><topic>propagation</topic><toplevel>online_resources</toplevel><creatorcontrib>Arteaga-Velázquez, J. C.</creatorcontrib><creatorcontrib>BenZvi, S. Y.</creatorcontrib><creatorcontrib>Brisbois, C.</creatorcontrib><creatorcontrib>Casanova, S.</creatorcontrib><creatorcontrib>Cotti, U.</creatorcontrib><creatorcontrib>Cotzomi, J.</creatorcontrib><creatorcontrib>Fiorino, D. W.</creatorcontrib><creatorcontrib>Hampel-Arias, Z.</creatorcontrib><creatorcontrib>Hueyotl-Zahuantitla, F.</creatorcontrib><creatorcontrib>Malone, K.</creatorcontrib><creatorcontrib>Miranda-Romagnoli, P.</creatorcontrib><creatorcontrib>Pretz, J.</creatorcontrib><creatorcontrib>Schneider, M.</creatorcontrib><creatorcontrib>Surajbali, P.</creatorcontrib><creatorcontrib>Tollefson, K.</creatorcontrib><creatorcontrib>Wood, J.</creatorcontrib><creatorcontrib>Adams, J.</creatorcontrib><creatorcontrib>Aguilar, J. A.</creatorcontrib><creatorcontrib>Anton, G.</creatorcontrib><creatorcontrib>Argüelles, C.</creatorcontrib><creatorcontrib>Auffenberg, J.</creatorcontrib><creatorcontrib>Axani, S.</creatorcontrib><creatorcontrib>Barron, J. 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C.</creatorcontrib><creatorcontrib>Maunu, R.</creatorcontrib><creatorcontrib>Meagher, K.</creatorcontrib><creatorcontrib>Miarecki, S.</creatorcontrib><creatorcontrib>Momenté, G.</creatorcontrib><creatorcontrib>Moulai, M.</creatorcontrib><creatorcontrib>Nahnhauer, R.</creatorcontrib><creatorcontrib>Pérez De Los Heros, C.</creatorcontrib><creatorcontrib>Pinat, E.</creatorcontrib><creatorcontrib>Plum, M.</creatorcontrib><creatorcontrib>Rameez, M.</creatorcontrib><creatorcontrib>Reimann, R.</creatorcontrib><creatorcontrib>Robertson, S.</creatorcontrib><creatorcontrib>Rysewyk, D.</creatorcontrib><creatorcontrib>Santander, M.</creatorcontrib><creatorcontrib>Schneider, A.</creatorcontrib><creatorcontrib>Sclafani, S.</creatorcontrib><creatorcontrib>Seckel, D.</creatorcontrib><creatorcontrib>Seunarine, S.</creatorcontrib><creatorcontrib>Soldin, D.</creatorcontrib><creatorcontrib>Song, M.</creatorcontrib><creatorcontrib>Stasik, A.</creatorcontrib><creatorcontrib>Sullivan, G. W.</creatorcontrib><creatorcontrib>Tenholt, F.</creatorcontrib><creatorcontrib>Ter-Antonyan, S.</creatorcontrib><creatorcontrib>Tilav, S.</creatorcontrib><creatorcontrib>Vandenbroucke, J.</creatorcontrib><creatorcontrib>Van Eijk, D.</creatorcontrib><creatorcontrib>Van Eijndhoven, N.</creatorcontrib><creatorcontrib>Watson, T. B.</creatorcontrib><creatorcontrib>Weaver, C.</creatorcontrib><creatorcontrib>Whitehorn, N.</creatorcontrib><creatorcontrib>Wood, T. R.</creatorcontrib><creatorcontrib>Woschnagg, K.</creatorcontrib><creatorcontrib>Xu, Y.</creatorcontrib><creatorcontrib>Yanez, J. P.</creatorcontrib><collection>DataCite</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Arteaga-Velázquez, J. C.</au><au>BenZvi, S. Y.</au><au>Brisbois, C.</au><au>Casanova, S.</au><au>Cotti, U.</au><au>Cotzomi, J.</au><au>Fiorino, D. W.</au><au>Hampel-Arias, Z.</au><au>Hueyotl-Zahuantitla, F.</au><au>Malone, K.</au><au>Miranda-Romagnoli, P.</au><au>Pretz, J.</au><au>Schneider, M.</au><au>Surajbali, P.</au><au>Tollefson, K.</au><au>Wood, J.</au><au>Adams, J.</au><au>Aguilar, J. A.</au><au>Anton, G.</au><au>Argüelles, C.</au><au>Auffenberg, J.</au><au>Axani, S.</au><au>Barron, J. P.</au><au>Berley, D.</au><au>Bernardini, Elisa</au><au>Binder, G.</au><au>Blaufuss, E.</au><au>Blot, S.</au><au>Bourbeau, E.</au><au>Bradascio, F.</au><au>Brostean-Kaiser, J.</au><au>Cheung, E.</au><au>Classen, L.</au><au>Coppin, P.</au><au>Dave, P.</au><au>Day, M.</au><au>Desiati, P.</au><au>DeYoung, T.</au><au>Dujmovic, H.</au><au>Eberhardt, B.</au><au>Ehrhardt, T.</au><au>Filimonov, K.</au><au>Friedman, E.</au><au>Ghorbani, K.</au><au>Gonzalez, J. G.</au><au>Heereman, D.</au><au>Helbing, K.</au><au>Hickford, S.</au><au>Huang, F.</au><au>Huber, M.</au><au>Kang, W.</au><au>Karg, T.</au><au>Katz, U.</au><au>Kelley, J. L.</au><au>Kintscher, T.</au><au>Kittler, T.</au><au>Köpke, L.</au><au>Kowalski, Marek</au><au>Kurahashi, N.</au><au>Labare, M.</au><au>Larson, M. J.</au><au>Leuermann, M.</au><au>Liu, Q. R.</au><au>Maggi, G.</au><au>Mariş, I. C.</au><au>Maunu, R.</au><au>Meagher, K.</au><au>Miarecki, S.</au><au>Momenté, G.</au><au>Moulai, M.</au><au>Nahnhauer, R.</au><au>Pérez De Los Heros, C.</au><au>Pinat, E.</au><au>Plum, M.</au><au>Rameez, M.</au><au>Reimann, R.</au><au>Robertson, S.</au><au>Rysewyk, D.</au><au>Santander, M.</au><au>Schneider, A.</au><au>Sclafani, S.</au><au>Seckel, D.</au><au>Seunarine, S.</au><au>Soldin, D.</au><au>Song, M.</au><au>Stasik, A.</au><au>Sullivan, G. W.</au><au>Tenholt, F.</au><au>Ter-Antonyan, S.</au><au>Tilav, S.</au><au>Vandenbroucke, J.</au><au>Van Eijk, D.</au><au>Van Eijndhoven, N.</au><au>Watson, T. B.</au><au>Weaver, C.</au><au>Whitehorn, N.</au><au>Wood, T. R.</au><au>Woschnagg, K.</au><au>Xu, Y.</au><au>Yanez, J. P.</au><format>book</format><genre>unknown</genre><ristype>RPRT</ristype><btitle>All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field</btitle><addtitle>The astrophysical journal / 1 Part 1 871(1)</addtitle><date>2019</date><risdate>2019</risdate><spage>96</spage><epage>(2019). doi:10.3847/1538</epage><pages>96-(2019). doi:10.3847/1538</pages><issn>0004-637X</issn><issn>1538-4357</issn><abstract>We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and present a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map, we determine the horizontal dipole components of the anisotropy δ 0h = 9.16 × 10−4 and δ 6h = 7.25 × 10−4 (±0.04 × 10−4). In addition, we infer the direction (2292 ± 35 R.A., 114 ± 30 decl.) of the interstellar magnetic field from the boundary between large-scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large-scale anisotropy to be .</abstract><pub>Deutsches Elektronen-Synchrotron, DESY, Hamburg</pub><doi>10.3204/pubdb-2020-00512</doi><orcidid>https://orcid.org/0000-0001-8594-8666</orcidid><orcidid>https://orcid.org/0000-0003-3251-2126</orcidid><orcidid>https://orcid.org/0000-0003-3108-1141</orcidid><orcidid>https://orcid.org/0000-0002-7669-266X</orcidid></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 0004-637X |
ispartof | |
issn | 0004-637X 1538-4357 |
language | eng |
recordid | cdi_datacite_primary_10_3204_pubdb_2020_00512 |
source | DataCite |
subjects | cosmic radiation: anisotropy cosmic radiation: TeV dipole HAWC IceCube magnetic field observatory particle: energy power spectrum: angular dependence propagation |
title | All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-11T19%3A59%3A31IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-datacite_PQ8&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=unknown&rft.btitle=All-Sky%20Measurement%20of%20the%20Anisotropy%20of%20Cosmic%20Rays%20at%2010%20TeV%20and%20Mapping%20of%20the%20Local%20Interstellar%20Magnetic%20Field&rft.au=Arteaga-Vel%C3%A1zquez,%20J.%20C.&rft.date=2019&rft.spage=96&rft.epage=(2019).%20doi:10.3847/1538&rft.pages=96-(2019).%20doi:10.3847/1538&rft.issn=0004-637X&rft_id=info:doi/10.3204/pubdb-2020-00512&rft_dat=%3Cdatacite_PQ8%3E10_3204_pubdb_2020_00512%3C/datacite_PQ8%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |