The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations

The solar maximum solar wind is highly structured in latitude, longitude and in time. Coronal measurements show a very high degree of variability, with large variations that are less apparent within in situ spacecraft measurements. Interplanetary scintillation (IPS) observations from EISCAT,...

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Bibliographic Details
Main Authors: A. R. Breen, P. Riley, A. J. Lazarus, A. Canals, R. A. Fallows, J. Linker, Z. Mikic
Format: Article
Language:English
Published: Copernicus Publications 2002-09-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/20/1291/2002/angeo-20-1291-2002.pdf