Comparison of Hα synoptic charts with the large-scale solar magnetic field as observed at Stanford
- 1 November 1977
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 55 (1), 63-68
- https://doi.org/10.1007/bf00150874
Abstract
No abstract availableKeywords
This publication has 9 references indexed in Scilit:
- The sun's magnetic sector structureSolar Physics, 1975
- Solar cycle variation of large-scale coronal structuresSolar Physics, 1974
- Observation of sectored structure in the outer solar corona: Correlation with interplanetary magnetic fieldSolar Physics, 1974
- A model combining the polar and the sector structured solar magnetic fieldsSolar Physics, 1974
- K corona and magnetic sector boundariesGeophysical Research Letters, 1974
- Influence of Solar Magnetic Sector Structure on Terrestrial Atmospheric VorticityJournal of the Atmospheric Sciences, 1974
- Analysis and synthesis of coronal and interplanetary energetic particle, plasma, and magnetic field observations over three solar rotationsJournal of Geophysical Research, 1973
- Solar magnetic fields derived from hydrogen alpha filtergramsReviews of Geophysics, 1972
- The interplanetary magnetic field. Solar origin and terrestrial effectsSpace Science Reviews, 1968