Latitudinal distribution of the solar wind properties in the low- and high-pressure regimes: Wind observations
The solar wind properties depend on λ, the heliomagnetic latitude with respect to the heliospheric current sheet (HCS), more than on the heliographic latitude. We analyse the wind properties observed by Wind at 1 AU during about 2.5 solar rotations in 1995, a period close to the last...
Main Authors: | C. Lacombe, C. Salem, A. Mangeney, J.-L. Steinberg, M. Maksimovic, J. M. Bosqued |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2000-08-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/18/852/2000/angeo-18-852-2000.pdf |
Similar Items
-
Evidence for the interplanetary electric potential? WIND observations of electrostatic fluctuations
by: C. Lacombe, et al.
Published: (2002-05-01) -
WIND observations of coherent electrostatic waves in the solar wind
by: A. Mangeney, et al.
Published: (1999-03-01) -
Cluster observations in the magnetosheath – Part 1: Anisotropies of the wave vector distribution of the turbulence at electron scales
by: A. Mangeney, et al.
Published: (2006-12-01) -
Cluster observations in the magnetosheath – Part 2: Intensity of the turbulence at electron scales
by: C. Lacombe, et al.
Published: (2006-12-01) -
Quantifying the latitudinal representivity of in situ solar wind observations
by: Owens Mathew J., et al.
Published: (2020-01-01)