Evidence of large scale diverging paths in the solar corona for type III bursts exciters
- 1 November 1975
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 45 (1), 169-179
- https://doi.org/10.1007/bf00152229
Abstract
No abstract availableKeywords
This publication has 6 references indexed in Scilit:
- Type III solar radio bursts observed at 169 MHz: Height and relative positions in pairsSolar Physics, 1974
- Acceleration of electrons in absence of detectable optical flares deduced from type III radio bursts, H? activity and soft X-ray emissionSolar Physics, 1974
- On the role of the magnetic configuration of flares for production of type III solar radio burstsSolar Physics, 1974
- Coronal Magnetic Field Structure Derived from Two-Frequency Radioheliograph ObservationsSymposium - International Astronomical Union, 1974
- Optical and Radio Observations of Large Scale Magnetic Fields on the SunSymposium - International Astronomical Union, 1971
- Scatter in the Positions of Sources of Associated Type III Solar BurstsPublications of the Astronomical Society of Australia, 1969