A comparison of coronal rotation and interplanetary recurrence during 1964–1976
- 1 January 1987
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 92 (A7), 7235
- https://doi.org/10.1029/ja092ia07p07235
Abstract
No abstract availableKeywords
This publication has 28 references indexed in Scilit:
- Prediction of geomagnetic activity on time scales of one to ten yearsReviews of Geophysics, 1986
- Rotational characteristics of the white-light solar corona 1965-1983The Astrophysical Journal, 1984
- Variations in solar rotation with the sunspot cycleThe Astrophysical Journal, 1984
- The power spectrum of the solar wind speed for periods greater than 10 daysJournal of Geophysical Research, 1978
- Solar wind speed variations: 1962-1974Journal of Geophysical Research, 1976
- Spectral analysis of the geomagnetic activity indexaaover a 103-year intervalJournal of Geophysical Research, 1975
- The heliographic latitude dependence and sector structure of the interplanetary magnetic field 1969?1974: Results from the HEOS satellitesSolar Physics, 1975
- Spectrum of the geomagnetic activity indexApJournal of Geophysical Research, 1972
- Differential rotation of the solar electron coronaSolar Physics, 1969
- Brightness variations of the white light corona during the years 1964?67Solar Physics, 1969