Low frequency turbulence in the solar corona and fundamental radiation of type III solar radio burst
- 1 June 1979
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 62 (2) , 375-382
- https://doi.org/10.1007/bf00155365
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- Numerical simulation of type III solar radio bursts caused by high-density electron beamSolar Physics, 1979
- Dynamics of a cloud of fast electrons travelling through the plasmaSolar Physics, 1979
- Electrostatically unstable heat flow during solar flares and its consequencesSolar Physics, 1977
- An unstable arch model of a solar flareSolar Physics, 1977
- Generation of intermediate drift bursts in solar type IV radio continua through coupling of whistlers and Langmuir wavesSolar Physics, 1975
- Coronal electric currents produced by photospheric motionsSolar Physics, 1974
- Acceleration of electrons and solar flares due to quasi-static electric fieldSolar Physics, 1971
- Theory of solar radio pulsationSolar Physics, 1970
- Currents in the solar atmosphere and a theory of solar flaresSolar Physics, 1967
- Frequency Splitting of Solar Radio BurstsAustralian Journal of Physics, 1967