Influence of stream‐stream interaction on the winding angle of the IMF spiral
Open Access
- 15 July 1998
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 25 (14) , 2617-2620
- https://doi.org/10.1029/98gl01974
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- On the winding of the IMF spiral for slow and fast wind within the inner heliosphereGeophysical Research Letters, 1997
- Comment on “The underlying magnetic field direction in Ulysses observations of the southern polar heliosphere” by Forsyth et al.Geophysical Research Letters, 1996
- The underlying Parker spiral structure in the Ulysses magnetic field observations, 1990–1994Journal of Geophysical Research, 1996
- The underlying magnetic field direction in Ulysses observations of the southern polar heliosphereGeophysical Research Letters, 1995
- MHD structures, waves and turbulence in the solar wind: Observations and theoriesSpace Science Reviews, 1995
- Origin of low cross‐helicity regions in the inner solar windJournal of Geophysical Research, 1991
- Solar cycle variation of the interplanetary magnetic field spiralThe Astrophysical Journal, 1991
- north‐south asymmetry of the interplanetary magnetic field spiralJournal of Geophysical Research, 1988
- Determination of the solar wind angular momentum flux from the HELIOS data - an observational test of the Weber and Davis theoryThe Astrophysical Journal, 1983
- Dynamics of the Interplanetary Gas and Magnetic Fields.The Astrophysical Journal, 1958