The band of solar wind variability at low heliographic latitudes near solar activity minimum: Plasma results from the Ulysses rapid latitude scan
- 7 December 1995
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 22 (23) , 3329-3332
- https://doi.org/10.1029/95gl02163
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Structures in the polar solar wind: Plasma and field observations from UlyssesJournal of Geophysical Research, 1995
- Interplanetary scintillation observations of the high-latitude solar windSpace Science Reviews, 1995
- The large-scale structure of the heliospheric current sheet during the Ulysses epochSpace Science Reviews, 1995
- Variation of fractional electron density fluctuations inside 40 Ro observed by Ulysses ranging measurementsGeophysical Research Letters, 1995
- A new class of forward‐reverse shock pairs in the solar windGeophysical Research Letters, 1994
- Ulysses at 50° south: constant immersion in the high‐speed solar windGeophysical Research Letters, 1994
- Ulysses observations of a recurrent high speed solar wind stream and the heliomagnetic streamer beltGeophysical Research Letters, 1993
- The structure of the white-light corona and the large-scale solar magnetic fieldSolar Physics, 1990
- Coronal mass ejections and magnetic flux ropes in interplanetary spacePublished by Wiley ,1990
- Solar wind helium and hydrogen structure near the heliospheric current sheet: A signal of coronal streamers at 1 AUJournal of Geophysical Research, 1981