30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy

Abstract: Based on data of world network neutron monitors and muon telescopes at Yakutsk and Nagoya stations an anisotropy component of galactic cosmic rays directed across a mean field line (in the direction of 15 LT) has been revealed. This component undergoes the 11-year variation. Its value rise...

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Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.9136
http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc0131.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.541.9136 2023-05-15T18:45:25+02:00 30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.9136 http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc0131.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.9136 http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc0131.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc0131.pdf text ftciteseerx 2016-01-08T11:06:33Z Abstract: Based on data of world network neutron monitors and muon telescopes at Yakutsk and Nagoya stations an anisotropy component of galactic cosmic rays directed across a mean field line (in the direction of 15 LT) has been revealed. This component undergoes the 11-year variation. Its value rises with increasing the interplanetary magnetic field intensity, solar activity level and neutral sheet deformation. Such a property of this component is explained by the action of the vortex electric field in the heliosphere. The 22-year variation of an anisotropy component directed along the magnetic field is of drift origin. Text Yakutsk Unknown Yakutsk
institution Open Polar
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description Abstract: Based on data of world network neutron monitors and muon telescopes at Yakutsk and Nagoya stations an anisotropy component of galactic cosmic rays directed across a mean field line (in the direction of 15 LT) has been revealed. This component undergoes the 11-year variation. Its value rises with increasing the interplanetary magnetic field intensity, solar activity level and neutral sheet deformation. Such a property of this component is explained by the action of the vortex electric field in the heliosphere. The 22-year variation of an anisotropy component directed along the magnetic field is of drift origin.
author2 The Pennsylvania State University CiteSeerX Archives
format Text
title 30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy
spellingShingle 30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy
title_short 30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy
title_full 30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy
title_fullStr 30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy
title_full_unstemmed 30TH INTERNATIONAL COSMIC RAY CONFERENCE Vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy
title_sort 30th international cosmic ray conference vortex electric field in interplanetary medium and the 11-year modulation of galactic cosmic ray anisotropy
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.9136
http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc0131.pdf
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http://galprop.stanford.edu/elibrary/icrc/2007/preliminary/pdf/icrc0131.pdf
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