Coronal holes as sources of large‐scale solar wind disturbances and geomagnetic perturbations
- 1 April 1991
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 96 (A4) , 5387-5396
- https://doi.org/10.1029/90ja02562
Abstract
No abstract availableKeywords
This publication has 43 references indexed in Scilit:
- A discussion about the geometry of the SKYLAB north polar coronal holeThe Astrophysical Journal, 1989
- Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation methodPlanetary and Space Science, 1989
- Radioheliograph and white-light coronagraph studies of a coronal mass ejection eventSolar Physics, 1989
- Origin of strong interplanetary shocksNature, 1985
- Tracking a high-latitude corotating stream for more than half a solar rotationPlanetary and Space Science, 1984
- Type II solar radio bursts, interplanetary shocks, and energetic particle eventsThe Astrophysical Journal, 1984
- Tracking a major interplanetary disturbancePlanetary and Space Science, 1983
- Open magnetic structures on the sunThe Astrophysical Journal, 1977
- Physical properties of a polar coronal hole from 2 to 5 solar radiiThe Astrophysical Journal, 1977
- Long-lived sectors of enhanced density irregularities in the solar windPlanetary and Space Science, 1972