The solar origins of solar wind interstream flows: Near‐equatorial coronal streamers
- 1 July 1981
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 86 (A7) , 5408-5416
- https://doi.org/10.1029/ja086ia07p05408
Abstract
No abstract availableKeywords
This publication has 50 references indexed in Scilit:
- Measurements of coronal kinetic temperatures from 1.5 to 3 solar radiiThe Astrophysical Journal, 1980
- Variation of the average ‘freezing‐in’ temperature of oxygen ions with solar wind speedGeophysical Research Letters, 1980
- Singly‐ionized helium in the driver gas of an interplanetary shock waveGeophysical Research Letters, 1980
- Plasma instabilities in the solar wind: A theoretical reviewReviews of Geophysics, 1980
- Solar wind flows associated with hot heavy ionsThe Astrophysical Journal, 1980
- Observation of sectored structure in the outer solar corona: Correlation with interplanetary magnetic fieldSolar Physics, 1974
- K corona and magnetic sector boundariesGeophysical Research Letters, 1974
- Properties of a Coronal "hole" Derived from Extreme-Ultraviolet ObservationsThe Astrophysical Journal, 1972
- Solar Wind Ion CompositionPhysical Review Letters, 1968
- A Photometric Study of the Solar Corona.The Astrophysical Journal, 1955