Results from the Pierre Auger Observatory
The Pierre Auger Observatory is the largest observatory of high-energy cosmic rays. It is located in Argentina and has been taking data since January 2004. Extensive air showers initiated by cosmic rays are measured by the hybrid detector, which combines the sampling of particle density at ground by...
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| Veröffentlicht in: | Advances in Astronomy and Space Physics |
|---|---|
| Datum: | 2012 |
| 1. Verfasser: | |
| Format: | Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
Головна астрономічна обсерваторія НАН України
2012
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/119176 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Results from the Pierre Auger Observatory / R. Šmída // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 67-72. — Бібліогр.: 22 назв. — англ. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| _version_ | 1862743518357749760 |
|---|---|
| author | Šmída, R. |
| author_facet | Šmída, R. |
| citation_txt | Results from the Pierre Auger Observatory / R. Šmída // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 67-72. — Бібліогр.: 22 назв. — англ. |
| collection | DSpace DC |
| container_title | Advances in Astronomy and Space Physics |
| description | The Pierre Auger Observatory is the largest observatory of high-energy cosmic rays. It is located in Argentina and has been taking data since January 2004. Extensive air showers initiated by cosmic rays are measured by the hybrid detector, which combines the sampling of particle density at ground by water-Cherenkov tanks and the measurement of atmospheric fluorescence light by telescopes. New detection techniques, like radio and microwave measurement, are also being tested. Results regarding the energy spectrum, mass composition and arrival directions of cosmic rays are presented here.
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| first_indexed | 2025-12-07T20:30:39Z |
| format | Article |
| fulltext | |
| id | nasplib_isofts_kiev_ua-123456789-119176 |
| institution | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| issn | 2227-1481 |
| language | English |
| last_indexed | 2025-12-07T20:30:39Z |
| publishDate | 2012 |
| publisher | Головна астрономічна обсерваторія НАН України |
| record_format | dspace |
| spelling | Šmída, R. 2017-06-04T18:39:33Z 2017-06-04T18:39:33Z 2012 Results from the Pierre Auger Observatory / R. Šmída // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 67-72. — Бібліогр.: 22 назв. — англ. 2227-1481 https://nasplib.isofts.kiev.ua/handle/123456789/119176 The Pierre Auger Observatory is the largest observatory of high-energy cosmic rays. It is located in Argentina and has been taking data since January 2004. Extensive air showers initiated by cosmic rays are measured by the hybrid detector, which combines the sampling of particle density at ground by water-Cherenkov tanks and the measurement of atmospheric fluorescence light by telescopes. New detection techniques, like radio and microwave measurement, are also being tested. Results regarding the energy spectrum, mass composition and arrival directions of cosmic rays are presented here. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics Results from the Pierre Auger Observatory Article published earlier |
| spellingShingle | Results from the Pierre Auger Observatory Šmída, R. |
| title | Results from the Pierre Auger Observatory |
| title_full | Results from the Pierre Auger Observatory |
| title_fullStr | Results from the Pierre Auger Observatory |
| title_full_unstemmed | Results from the Pierre Auger Observatory |
| title_short | Results from the Pierre Auger Observatory |
| title_sort | results from the pierre auger observatory |
| url | https://nasplib.isofts.kiev.ua/handle/123456789/119176 |
| work_keys_str_mv | AT smidar resultsfromthepierreaugerobservatory |