Testing for uniformity of ultra-high energy cosmic ray arrival directions
Author:
Affiliation:
1. Shafer Institute for Cosmophysical Research and Aeronomy, Lenin Avenue 31, Yakutsk 677980, Russia
Abstract
Publisher
World Scientific Pub Co Pte Lt
Subject
Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics
Link
https://www.worldscientific.com/doi/pdf/10.1142/S0218271816500656
Reference12 articles.
1. Galactic cosmic-ray anisotropy and its modulation in the heliomagnetosphere, inferred from air shower observation at Mt. Norikura
2. THE EAST-WEST METHOD: AN EXPOSURE-INDEPENDENT METHOD TO SEARCH FOR LARGE-SCALE ANISOTROPIES OF COSMIC RAYS
3. Determining the primary cosmic ray energy from the total flux of Cherenkov light measured at the Yakutsk EAS array
4. Main results of the study of ultrahigh-energy cosmic rays in the Yakutsk Extensive Air Shower Array
5. Analysis of anisotropy of cosmic rays with the energy of about 1017 eV by Yakutsk EAS array data
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Upper limit on the fraction of the cosmic ray flux from a separable source in the energy interval (1017 -1019 eV), estimated using data from the Yakutsk array;EPJ Web of Conferences;2019
2. Zenith angle distribution of cosmic ray showers measured with the Yakutsk array and its application to the analysis of arrival directions in equatorial coordinates;Physical Review D;2018-04-10
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