A new classification of geomagnetic storms and their source flares
dc.contributor.author | Yoshida, Sekiko | |
dc.date.accessioned | 2024-10-25T21:07:05Z | |
dc.date.available | 2024-10-25T21:07:05Z | |
dc.date.issued | 1965-08 | |
dc.identifier.uri | http://hdl.handle.net/11122/15547 | |
dc.description | UAG R-167; Scientific Report | en_US |
dc.description.abstract | Geomagnetic storms which occurred between 1956 and 1963 are classified in terms of different combinations of the three basic storm fields, the DCF, DR and DP fields. For each storm, a new attempt is made to identify the source solar flare, based on several new important findings on characteristics of geomagnetic storms. | en_US |
dc.description.sponsorship | This research was supported in part by a grant from the National Aeronautics and Space Administration under contract NsG 201-62. | en_US |
dc.description.tableofcontents | Introduction – Bases for the identification – Description of the table – New classification of geomagnetic storms -- Table. | en_US |
dc.language.iso | en_US | en_US |
dc.publisher | Geophysical Institute at the University of Alaska Fairbanks | en_US |
dc.subject | Geomagnetism | en_US |
dc.subject | Magnetic storms | en_US |
dc.subject | Solar flares | en_US |
dc.title | A new classification of geomagnetic storms and their source flares | en_US |
dc.type | Report | en_US |
refterms.dateFOA | 2024-10-25T21:07:06Z |
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