On the possibility of inferring the solar and interplanetary sector structure from statistics of geomagnetic storms and solar activity
- 30 November 1973
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 21 (11) , 2003-2011
- https://doi.org/10.1016/0032-0633(73)90129-3
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- Relation between coronal λ 5303 intensity, recurrent geomagnetic storms, and solar sector structureJournal of Geophysical Research, 1973
- Active solar radio regions at metric frequencies and the interplanetary sector structuresSolar Physics, 1971
- Solar radio centers and interplanetary sector structures in connection with recurrent geomagnetic stormsJournal of Geophysical Research, 1970
- Some features of the solar microwave emission and their connection with geomagnetic activitySolar Physics, 1969
- ?Bartels' active longitudes?, sector boundaries and flare activitySolar Physics, 1969
- Quasi-stationary emission of gases from the sunSpace Science Reviews, 1964
- M-RegionsPlanetary and Space Science, 1964
- Recurrent geomagnetic storms, solar M-regions and the solar windPlanetary and Space Science, 1964
- Statistics of Geomagnetic Storms and Solar ActivityMonthly Notices of the Royal Astronomical Society, 1961
- Geomagnetism and the emission-line corona, 1950-1953Smithsonian Contributions to Astrophysics, 1957