Home > Publications database > All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field > print

001     418363
005     20211110153256.0
024 7 _ |a arXiv:1812.05682
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2019-00395
|2 datacite_doi
024 7 _ |a inspire:1709221
|2 inspire
037 _ _ |a PUBDB-2019-00395
041 _ _ |a English
088 1 _ |a arXiv:1812.05682
088 _ _ |a arXiv:1812.05682
|2 arXiv
100 1 _ |a HAWC Collaboration
|b 0
245 _ _ |a All-Sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field
260 _ _ |c 2018
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1547204072_24617
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a Report
|0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|m report
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a Accepted by The Astrophysical Journal
520 _ _ |a We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the HAWC 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 holds 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 $\delta_{0h} = 9.16 \times 10^{-4}$ and $\delta_{6h} = 7.25 \times 10^{-4}~(\pm0.04 \times 10^{-4})$. In addition, we infer the direction ($229.2\pm 3.5^\circ$ RA , $11.4\pm 3.0^\circ$ Dec.) 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 $\delta_N \sim -3.97 ^{+1.0}_{-2.0} \times 10^{-4}$.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF3-613)
|0 G:(DE-HGF)POF3-613
|c POF3-613
|f POF III
|x 0
588 _ _ |a Dataset connected to arXivarXiv
693 _ _ |0 EXP:(DE-H253)IceCube-20150101
|5 EXP:(DE-H253)IceCube-20150101
|e IceCube South Pole Neutrino Observatory
|x 0
700 1 _ |a Abeysekara, A. U.
|b 1
700 1 _ |a Alfaro, R.
|b 2
700 1 _ |a Alvarez, C.
|b 3
700 1 _ |a Álvarez, J. D.
|b 4
700 1 _ |a Arceo, R.
|b 5
700 1 _ |a Arteaga-Velázquez, J. C.
|b 6
700 1 _ |a Rojas, D. Avila
|b 7
700 1 _ |a Belmont-Moreno, E.
|b 8
700 1 _ |a BenZvi, S. Y.
|b 9
700 1 _ |a Brisbois, C.
|b 10
700 1 _ |a Capistrán, T.
|b 11
700 1 _ |a Carramiñana, A.
|b 12
700 1 _ |a Casanova, S.
|b 13
700 1 _ |a Cotti, U.
|b 14
700 1 _ |a Cotzomi, J.
|b 15
700 1 _ |a Díaz-Vélez, J. C.
|b 16
700 1 _ |a De León, C.
|b 17
700 1 _ |a De la Fuente, E.
|b 18
700 1 _ |a Dichiara, S.
|b 19
700 1 _ |a DuVernois, M. A.
|b 20
700 1 _ |a Espinoza, C.
|b 21
700 1 _ |a Fiorino, D. W.
|b 22
700 1 _ |a Fleischhack, H.
|b 23
700 1 _ |a Fraija, N.
|b 24
700 1 _ |a Galván-Gámez, A.
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700 1 _ |a García-González, J. A.
|b 26
700 1 _ |a González, M. M.
|b 27
700 1 _ |a Goodman, J. A.
|b 28
700 1 _ |a Hampel-Arias, Z.
|b 29
700 1 _ |a Harding, J. P.
|b 30
700 1 _ |a Hernandez, S.
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700 1 _ |a Hona, B.
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700 1 _ |a Iriarte, A.
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700 1 _ |a Jardin-Blicq, A.
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700 1 _ |a Joshi, V.
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700 1 _ |a Marinelli, S. S.
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700 1 _ |a Martínez-Castro, J.
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700 1 _ |a Matthews, J. A.
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700 1 _ |a Noriega-Papaqui, R.
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700 1 _ |a Pérez-Pérez, E. G.
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700 1 _ |a Weisgarber, T.
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700 1 _ |a Wood, J.
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700 1 _ |a Zepeda, A.
|b 73
700 1 _ |a Zhou, H.
|b 74
700 1 _ |a IceCube Collaboration
|0 P:(DE-HGF)0
|b 75
|e Corresponding author
700 1 _ |a Techn. Koordinator:, J. Spengler
|b 76
700 1 _ |a Aartsen, M. G.
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700 1 _ |a Ackermann, M.
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700 1 _ |a Adams, J.
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700 1 _ |a Baum, V.
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700 1 _ |a Bay, R.
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700 1 _ |a Becker, K. -H.
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700 1 _ |a Tjus, J. Becker
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