TA anisotropy summary
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.
Keywords
cosmic rays;ultra-high energy cosmic rays;energy spectrum;anisotropy;Telescope Array;
Data
| Language: | English |
|---|---|
| Year of publishing: | 2019 |
| Typology: | 1.08 - Published Scientific Conference Contribution |
| Organization: | UNG - University of Nova Gorica |
| UDC: | 52 |
| COBISS: |
12877059
|
| ISSN: | 2100-014X |
| Views: | 2159 |
| Downloads: | 73 |
| Average score: | 0 (0 votes) |
| Metadata: |
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Other data
| URN: | URN:SI:UNG |
|---|---|
| Type (COBISS): | Not categorized |
| Pages: | Str. 1-7 |
| DOI: | 10.1051/epjconf/201921001004 |
| ID: | 11596566 |
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