Relation between coronal λ 5303 intensity, recurrent geomagnetic storms, and solar sector structure
- 1 August 1973
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 78 (22) , 4787-4791
- https://doi.org/10.1029/ja078i022p04787
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- On the variation of the coronal λ5303 intensity relative to the interplanetary and solar magnetic sector structure, and to geomagnetic activityPlanetary and Space Science, 1973
- Properties of a Coronal "hole" Derived from Extreme-Ultraviolet ObservationsThe Astrophysical Journal, 1972
- Interplanetary sector structure at solar maximumJournal of Geophysical Research, 1972
- Coronal Expansion and Solar WindPublished by Springer Nature ,1972
- Solar Magnetic Fields - ExtendedPublications of the Astronomical Society of the Pacific, 1971
- Sector Structure of the Solar Magnetic FieldPublished by Springer Nature ,1971
- Some features of the solar microwave emission and their connection with geomagnetic activitySolar Physics, 1969
- Variations in the polarity distribution of the interplanetary magnetic fieldJournal of Geophysical Research, 1966
- Green coronal line intensity and geomagnetismJournal of Geophysical Research, 1959
- Geomagnetism and the emission-line corona, 1950-1953Smithsonian Contributions to Astrophysics, 1957