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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Hauptverfasser: 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.
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container_end_page (2019). doi:10.3847/1538
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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. 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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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C.</creator><creator>Maunu, R.</creator><creator>Meagher, K.</creator><creator>Miarecki, S.</creator><creator>Momenté, G.</creator><creator>Moulai, M.</creator><creator>Nahnhauer, R.</creator><creator>Pérez De Los Heros, C.</creator><creator>Pinat, E.</creator><creator>Plum, M.</creator><creator>Rameez, M.</creator><creator>Reimann, R.</creator><creator>Robertson, S.</creator><creator>Rysewyk, D.</creator><creator>Santander, M.</creator><creator>Schneider, A.</creator><creator>Sclafani, S.</creator><creator>Seckel, D.</creator><creator>Seunarine, S.</creator><creator>Soldin, D.</creator><creator>Song, M.</creator><creator>Stasik, A.</creator><creator>Sullivan, G. W.</creator><creator>Tenholt, F.</creator><creator>Ter-Antonyan, S.</creator><creator>Tilav, S.</creator><creator>Vandenbroucke, J.</creator><creator>Van Eijk, D.</creator><creator>Van Eijndhoven, N.</creator><creator>Watson, T. B.</creator><creator>Weaver, C.</creator><creator>Whitehorn, N.</creator><creator>Wood, T. 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. P.</creatorcontrib><creatorcontrib>Berley, D.</creatorcontrib><creatorcontrib>Bernardini, Elisa</creatorcontrib><creatorcontrib>Binder, G.</creatorcontrib><creatorcontrib>Blaufuss, E.</creatorcontrib><creatorcontrib>Blot, S.</creatorcontrib><creatorcontrib>Bourbeau, E.</creatorcontrib><creatorcontrib>Bradascio, F.</creatorcontrib><creatorcontrib>Brostean-Kaiser, J.</creatorcontrib><creatorcontrib>Cheung, E.</creatorcontrib><creatorcontrib>Classen, L.</creatorcontrib><creatorcontrib>Coppin, P.</creatorcontrib><creatorcontrib>Dave, P.</creatorcontrib><creatorcontrib>Day, M.</creatorcontrib><creatorcontrib>Desiati, P.</creatorcontrib><creatorcontrib>DeYoung, T.</creatorcontrib><creatorcontrib>Dujmovic, H.</creatorcontrib><creatorcontrib>Eberhardt, B.</creatorcontrib><creatorcontrib>Ehrhardt, T.</creatorcontrib><creatorcontrib>Filimonov, K.</creatorcontrib><creatorcontrib>Friedman, E.</creatorcontrib><creatorcontrib>Ghorbani, K.</creatorcontrib><creatorcontrib>Gonzalez, J. G.</creatorcontrib><creatorcontrib>Heereman, D.</creatorcontrib><creatorcontrib>Helbing, K.</creatorcontrib><creatorcontrib>Hickford, S.</creatorcontrib><creatorcontrib>Huang, F.</creatorcontrib><creatorcontrib>Huber, M.</creatorcontrib><creatorcontrib>Kang, W.</creatorcontrib><creatorcontrib>Karg, T.</creatorcontrib><creatorcontrib>Katz, U.</creatorcontrib><creatorcontrib>Kelley, J. L.</creatorcontrib><creatorcontrib>Kintscher, T.</creatorcontrib><creatorcontrib>Kittler, T.</creatorcontrib><creatorcontrib>Köpke, L.</creatorcontrib><creatorcontrib>Kowalski, Marek</creatorcontrib><creatorcontrib>Kurahashi, N.</creatorcontrib><creatorcontrib>Labare, M.</creatorcontrib><creatorcontrib>Larson, M. J.</creatorcontrib><creatorcontrib>Leuermann, M.</creatorcontrib><creatorcontrib>Liu, Q. R.</creatorcontrib><creatorcontrib>Maggi, G.</creatorcontrib><creatorcontrib>Mariş, I. 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
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