Ulysses at 50° south: constant immersion in the high‐speed solar wind
Open Access
- 15 June 1994
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 21 (12) , 1105-1108
- https://doi.org/10.1029/94gl01065
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- A forward‐reverse shock pair in the solar wind driven by over‐expansion of a coronal mass ejection: Ulysses observationsGeophysical Research Letters, 1994
- Latitudinal variation of solar wind corotating stream interaction regions: UlyssesGeophysical Research Letters, 1993
- Disappearance of the heliospheric sector structure at UlyssesGeophysical Research Letters, 1993
- Ulysses observations of a recurrent high speed solar wind stream and the heliomagnetic streamer beltGeophysical Research Letters, 1993
- The evolution of the interplanetary sector structure in 1992Geophysical Research Letters, 1993
- Prediction of the heliospheric current sheet tilt: 1992 – 1996Geophysical Research Letters, 1993
- Evolution of the solar wind structure over a solar cycle: Interplanetary scintillation velocity measurements compared with coronal observationsJournal of Geophysical Research, 1991
- In-situ observations of the latitudinal gradients of the solar wind parameters during 1976 and 1977Solar Physics, 1986
- The structure of the heliospheric current sheet: 1978–1982Journal of Geophysical Research, 1983
- Compressions and rarefactions in the solar wind: Vela 3Journal of Geophysical Research, 1972