| Title: | TA Anisotropy Summary |
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| Authors: | ID Kawata, K. (Author)
ID Lundquist, Jon Paul (Author), et al. |
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| Files: |  epjconf_uhecr18_01004.pdf (1,88 MB)
MD5: 789D9CFCFAA055CB82AE0BEB60FFA1A2
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| Language: | English |
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| Work type: | Not categorized |
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| Typology: | 1.08 - Published Scientific Conference Contribution |
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| Organization: | UNG - University of Nova Gorica
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| Abstract: | The Telescope Array (TA) is the largest ultra-high-energy cosmic-ray (UHECR) detector in the northern hemisphere. It consists of an array of 507 surface detectors (SD) covering a total 700 km^2 and three fluorescence detector stations overlooking the SD array. In this proceedings, we summarize recent results on the search for directional anisotropy of UHECRs using the latest dataset collected by the TA SD array. We obtained hints of the anisotropy of the UHECRs in the northern sky from the various analyses. |
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| Keywords: | cosmic radiation, UHE detector, fluorescence detector, surface, Telescope Array Experiment, anisotropy, experimental results |
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| Publication version: | Version of Record |
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| Year of publishing: | 2019 |
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| Number of pages: | 7 |
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| Numbering: | UHEC2018, 210 |
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| PID: | 20.500.12556/RUNG-5167-f5f46695-527f-05b6-52ff-e603f0fa6618  |
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| COBISS.SI-ID: | 12877059 |
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| DOI: | 10.1051/epjconf/201921001004 |
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| NUK URN: | URN:SI:UNG:REP:0PGHPGPK |
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| Publication date in RUNG: | 28.04.2020 |
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| Views: | 3890 |
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| Downloads: | 82 |
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