Unsolved problems of solar wind expansion: Can we learn anything from SOHO?
- 1 October 1994
- journal article
- Published by Springer Nature in Space Science Reviews
- Vol. 70 (1) , 331-340
- https://doi.org/10.1007/bf00777888
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Overestimating the coronal density and its effect on the velocities derived from L? Doppler dimmingSolar Physics, 1993
- How reliable are coronal hole temperatures deduced from observations?The Astrophysical Journal, 1993
- Solar wind from a corona with a large helium abundanceJournal of Geophysical Research, 1992
- The effect of a non-Maxwellian electron distribution on oxygen and iron ionization balances in the solar coronaThe Astrophysical Journal, 1983
- Temperature gradients in the inner coronaSolar Physics, 1978
- A steady three‐fluid coronal expansion for nonspherical geometriesJournal of Geophysical Research, 1978
- The coronal temperature and nonthermal motions in a coronal hole compared with other solar regionsThe Astrophysical Journal, 1977
- High-speed solar wind flow parameters at 1 AUJournal of Geophysical Research, 1976
- ALFVtN Waves in a Two-Fluid Model of the Solar WindThe Astrophysical Journal, 1973
- Dynamical theory of the solar windSpace Science Reviews, 1965