A moving Type IV burst, observed with the Culgoora radioheliograph on 1970 April 29, moved out to about 3 R o and attained high circular polarization before fading. The appearance of the moving Type IV source suggests an isolated, self-contained, synchrotron emitting plasmoid. Magnetic field maps of
Determination of the coronal magnetic field and the radio-emitting electron energy from a Type IV solar radio burst
โ Scribed by Reuven Ramaty; Richard E. Lingenfelter
- Publisher
- Springer
- Year
- 1968
- Tongue
- English
- Weight
- 731 KB
- Volume
- 5
- Category
- Article
- ISSN
- 0038-0938
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