Coronal magnetic field structure derived from two-frequency radioheliograph observations
- 1 March 1974
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 35 (1) , 181-192
- https://doi.org/10.1007/bf00156966
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- The gyro-synchrotron radiation from moving type IV sources in the solar coronaSolar Physics, 1973
- Three-frequency operation of the Culgoora radioheliographProceedings of the IEEE, 1973
- Meter-wavelength observations of the solar radio burst storm of August 17?22, 1968Solar Physics, 1972
- Radio Bursts from the Solar CoronaAnnual Review of Astronomy and Astrophysics, 1972
- Radio evidence of twisted bi-polar magnetic fields in the solar coronaSolar Physics, 1972
- Multiple-frequency Operation of the Culgoora RadioheliographNature Physical Science, 1972
- The structure, polarization, and spatial relationship of solar radio sources of spectral types I and IIISolar Physics, 1970
- Some Investigations of the Solar Corona: The First Two Years of Observation With the Culgoora RadioheliographPublications of the Astronomical Society of Australia, 1969
- Observations of Motions in a Solar Storm CentrePublications of the Astronomical Society of Australia, 1969
- The Culgoora RadiospectrographPublications of the Astronomical Society of Australia, 1967