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,...
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 |
Similar Items
-
EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation
by: R. A. Fallows, et al.
Published: (2002-09-01) -
Estimating random transverse velocities in the fast solar wind from EISCAT Interplanetary Scintillation measurements
by: A. Canals, et al.
Published: (2002-09-01) -
EISCAT measurements of the solar wind
by: A. R. Breen, et al.
Published: (1996-12-01) -
Developments in the use of EISCAT for interplanetary scintillation
by: R. A. Fallows, et al.
Published: (2008-08-01) -
Simultaneous interplanetary scintillation and optical measurements of the acceleration of the slow solar wind
by: A. R. Breen, et al.
Published: (2000-09-01)