Are coronal holes the only source of fast solar wind at solar minimum?
- 28 October 2003
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 108 (A10)
- https://doi.org/10.1029/2002ja009776
Abstract
No abstract availableKeywords
This publication has 59 references indexed in Scilit:
- Effect of Flow-Tube Geometry on Solar Wind PropertiesAstrophysics and Space Science, 2002
- A Two-Dimensional Alfvén-Wave-Driven Solar Wind ModelSolar Physics, 2001
- Model of solar wind flow near an equatorial coronal streamerPublished by AIP Publishing ,1999
- Sources of magnetic fields in recurrent interplanetary streamsJournal of Geophysical Research, 1978
- Coronal holes and high‐speed wind streamsReviews of Geophysics, 1977
- Flux-corrected transport. III. Minimal-error FCT algorithmsJournal of Computational Physics, 1976
- Flux-corrected transport II: Generalizations of the methodJournal of Computational Physics, 1975
- Flux-corrected transport. I. SHASTA, a fluid transport algorithm that worksJournal of Computational Physics, 1973
- Physics of Fully Ionized GasesAmerican Journal of Physics, 1963
- Difference Methods for Initial-Value ProblemsPhysics Today, 1959