Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field
The Earth's magnetic field effect on the azimuthal distribution of extensive air showers (EAS) of cosmic rays has been evaluated using a bulk of the Yakutsk array data. The uniform azimuthal distribution of the EAS event rate is rejected at the significance level 10^(-14). Amplitude of the firs...
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ftcern:oai:cds.cern.ch:382691 2023-05-15T18:45:25+02:00 Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field Ivanov, A A Egorova, V P Kolosov, V A Krasilnikov, A D Pravdin, M I Sleptsov, I Ye 1999 http://cds.cern.ch/record/382691 eng eng http://cds.cern.ch/record/382691 astro-ph/9903337 oai:cds.cern.ch:382691 Astrophysics and Astronomy 1999 ftcern 2018-07-28T03:57:40Z The Earth's magnetic field effect on the azimuthal distribution of extensive air showers (EAS) of cosmic rays has been evaluated using a bulk of the Yakutsk array data. The uniform azimuthal distribution of the EAS event rate is rejected at the significance level 10^(-14). Amplitude of the first harmonics of observed distribution depends on zenith angle as A1=0.2*sin^2(theta) and is almost independent of the primary energy; the phase coincides with the magnetic meridian. Basing upon the value of measured effect, the correction factor has been derived for the particle density depending on a geomagnetic parameter of a shower. Other/Unknown Material Yakutsk CERN Document Server (CDS) Yakutsk |
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CERN Document Server (CDS) |
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English |
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Astrophysics and Astronomy |
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Astrophysics and Astronomy Ivanov, A A Egorova, V P Kolosov, V A Krasilnikov, A D Pravdin, M I Sleptsov, I Ye Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field |
topic_facet |
Astrophysics and Astronomy |
description |
The Earth's magnetic field effect on the azimuthal distribution of extensive air showers (EAS) of cosmic rays has been evaluated using a bulk of the Yakutsk array data. The uniform azimuthal distribution of the EAS event rate is rejected at the significance level 10^(-14). Amplitude of the first harmonics of observed distribution depends on zenith angle as A1=0.2*sin^2(theta) and is almost independent of the primary energy; the phase coincides with the magnetic meridian. Basing upon the value of measured effect, the correction factor has been derived for the particle density depending on a geomagnetic parameter of a shower. |
author |
Ivanov, A A Egorova, V P Kolosov, V A Krasilnikov, A D Pravdin, M I Sleptsov, I Ye |
author_facet |
Ivanov, A A Egorova, V P Kolosov, V A Krasilnikov, A D Pravdin, M I Sleptsov, I Ye |
author_sort |
Ivanov, A A |
title |
Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field |
title_short |
Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field |
title_full |
Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field |
title_fullStr |
Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field |
title_full_unstemmed |
Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field |
title_sort |
azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field |
publishDate |
1999 |
url |
http://cds.cern.ch/record/382691 |
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Yakutsk |
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Yakutsk |
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Yakutsk |
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Yakutsk |
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http://cds.cern.ch/record/382691 astro-ph/9903337 oai:cds.cern.ch:382691 |
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1766236477998497792 |