Solar‐cycle variation of low density solar wind during more than three solar cycles
- 1 December 2000
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 27 (23) , 3761-3764
- https://doi.org/10.1029/2000gl000077
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Sources of geomagnetic activity over the solar cycle: Relative importance of coronal mass ejections, high‐speed streams, and slow solar windJournal of Geophysical Research, 2000
- Solar wind measurements with SOHO: The CELIAS/MTOF proton monitorJournal of Geophysical Research, 1998
- Variability of the tail lobe field strengthJournal of Geophysical Research, 1996
- Regions of abnormally low proton temperature in the solar wind (1965–1991) and their association with ejectaJournal of Geophysical Research, 1995
- On the low correlation between long‐term averages of solar wind speed and geomagnetic activity after 1976Journal of Geophysical Research, 1993
- Coronal mass ejections and magnetic flux ropes in interplanetary spacePublished by Wiley ,1990
- A Sub‐Alfvénic solar wind: Interplanetary and magnetosheath observationsJournal of Geophysical Research, 1982
- New aspects of the cosmic-ray modulation in 1974-1975 near solar minimumThe Astrophysical Journal, 1977