Latitude-time distribution of 3 types of magnetic field activity in the global solar cycle
- 1 October 1992
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 141 (2) , 381-390
- https://doi.org/10.1007/bf00155187
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- HeI dark points and 11-year solar cycleSolar Physics, 1991
- A two-component solar cycleSolar Physics, 1991
- Do polar faculae on the sun predict a sunspot cycle?Solar Physics, 1989
- Evolution of latitude zonal structure of the large-scale magnetic field in solar cyclesSolar Physics, 1989
- The extended solar activity cycleNature, 1988
- Weak solar fields and their connection to the solar cycleSolar Physics, 1987
- Torsional oscillations and the solar cycleSolar Physics, 1987
- Poleward migration of the magnetic neutral line and the reversal of the polar fields on the SunSolar Physics, 1983
- The sun is observed to be a torsional oscillator with a period of 11 yearsThe Astrophysical Journal, 1980
- Solar magnetic fields derived from hydrogen alpha filtergramsReviews of Geophysics, 1972