How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation

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Location: Deutsche Nationalbibliothek Frankfurt am Main

Extent: Online-Ressource

Language: Englisch

Bibliographic citation: How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation ; volume:21 ; number:6 ; year:2003 ; pages:1257-1261
Annales geophysicae ; 21, Heft 6 (2003), 1257-1261

Creator: Fujiki, K.
Kojima, M.
Tokumaru, M.
Ohmi, T.
Yokobe, A.
Hayashi, K.
McComas, D. J.
Elliott, H. A.

DOI: 10.5194/angeo-21-1257-2003

URN: urn:nbn:de:101:1-2017122111838

Rights: Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.

Last update: 15.08.2025, 7:33 AM CEST

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Associated

Fujiki, K.
Kojima, M.
Tokumaru, M.
Ohmi, T.
Yokobe, A.
Hayashi, K.
McComas, D. J.
Elliott, H. A.

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How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation

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Other Objects (12)

Interplanetary scintillation observations of interaction regions in the solar wind

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EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation

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