CLUSTER MISSION AND DATA ANALYSIS FOR THE MARCH 2001 MAGNETIC STORM

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dc.contributor.authorFrutos Alfaro F.
dc.contributor.authorKorth A.
dc.contributor.authorFränz M.
dc.contributor.authorMouikis C.G.
dc.contributor.authorKistler L.M.
dc.contributor.authorMöbius E.
dc.contributor.authorKucharek H.
dc.contributor.authorKlecker B.
dc.contributor.authorRème H.
dc.contributor.authorDandouras I.
dc.contributor.authorBosqued J.M.
dc.contributor.authorSauvaud J.A.
dc.contributor.authorMcFadden J.P.
dc.contributor.authorCarlson C.W.
dc.contributor.authorAmata E.
dc.contributor.authorLundin R.
dc.date.accessioned2022-10-20T08:59:35Z
dc.date.available2022-10-20T08:59:35Z
dc.date.issued2004
dc.description.abstractThe CLUSTER mission is intended for the study of the Earth’s magnetosphere and Sun-Earth relationships. Four satellites fly in a tetrahedral formation sending data that can separate spatial from temporal effects for the first time. This formation will provide a better understanding of microscopic and macroscopic features in the magnetosphere and the solar wind. As an illustration we discuss the CIS data during a large magnetic storm.
dc.identifierhttps://elibrary.ru/item.asp?id=14367732
dc.identifier.citationGeofisica International, 2004, 43, 2, 217-223
dc.identifier.issn0016-7169
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/38970
dc.subjectCLUSTER mission
dc.subjectmagnetic storm
dc.subjection spectrometry
dc.titleCLUSTER MISSION AND DATA ANALYSIS FOR THE MARCH 2001 MAGNETIC STORM
dc.typeСтатья

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