Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances

By using treatment results of world net neutron monitor data by the global survey method, the behaviour of cosmic ray current (anisotropy) during Forbush-effects for the 1965 to 1999 period is analyzed. Peculiarities of the current be-haviour before the shock wave arrival are investigated depending...

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Other Authors: The Pennsylvania State University CiteSeerX Archives
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Language:English
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Yakutsk
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.554.8725
http://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/PROCEEDINGS/PDF/890.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.554.8725 2023-05-15T18:45:25+02:00 Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.554.8725 http://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/PROCEEDINGS/PDF/890.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.554.8725 http://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/PROCEEDINGS/PDF/890.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/PROCEEDINGS/PDF/890.pdf text ftciteseerx 2016-01-08T11:43:52Z By using treatment results of world net neutron monitor data by the global survey method, the behaviour of cosmic ray current (anisotropy) during Forbush-effects for the 1965 to 1999 period is analyzed. Peculiarities of the current be-haviour before the shock wave arrival are investigated depending on the value of intensity decrease effect and heliocoordinates of disturbance sources on the Sun. Data of the Yakutsk underground complex of muon telescopes are also used in the analysis. Possibilities to predict the arrival of large-scale disturbances of in-terplanetary medium at the Earth by the behaviour of the observed cosmic ray anisotropy are discussed. 1. Text Yakutsk Unknown Yakutsk
institution Open Polar
collection Unknown
op_collection_id ftciteseerx
language English
description By using treatment results of world net neutron monitor data by the global survey method, the behaviour of cosmic ray current (anisotropy) during Forbush-effects for the 1965 to 1999 period is analyzed. Peculiarities of the current be-haviour before the shock wave arrival are investigated depending on the value of intensity decrease effect and heliocoordinates of disturbance sources on the Sun. Data of the Yakutsk underground complex of muon telescopes are also used in the analysis. Possibilities to predict the arrival of large-scale disturbances of in-terplanetary medium at the Earth by the behaviour of the observed cosmic ray anisotropy are discussed. 1.
author2 The Pennsylvania State University CiteSeerX Archives
format Text
title Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances
spellingShingle Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances
title_short Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances
title_full Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances
title_fullStr Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances
title_full_unstemmed Dynamics of the Cosmic Ray Current Behaviour During Large-Scale Solar Wind Disturbances
title_sort dynamics of the cosmic ray current behaviour during large-scale solar wind disturbances
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.554.8725
http://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/PROCEEDINGS/PDF/890.pdf
geographic Yakutsk
geographic_facet Yakutsk
genre Yakutsk
genre_facet Yakutsk
op_source http://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/PROCEEDINGS/PDF/890.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.554.8725
http://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/PROCEEDINGS/PDF/890.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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