Coronal densities and magnetic fields from K-coronameter and type IV radio burst data
- 1 September 1969
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 9 (1) , 183-193
- https://doi.org/10.1007/bf00145739
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Brightness variations of the white light corona during the years 1964?67Solar Physics, 1969
- Asymptotic Form for Synchrotron Spectra Below Razin CutoffThe Astrophysical Journal, 1969
- Determination of the coronal magnetic field and the radio-emitting electron energy from a Type IV solar radio burstSolar Physics, 1968
- Relativistic electrons from solar flaresSolar Physics, 1968
- Influence of the ionized medium on synchrotron emission of intermediate energy electronsJournal of Geophysical Research, 1968
- Structure of the Solar CoronaAnnual Review of Astronomy and Astrophysics, 1967
- The influence of the ionized medium on synchrotron emission spectra in the solar coronaJournal of Geophysical Research, 1967
- An Example of Meteorological Considerations in Selecting an Observatory Site in HawaiiPublications of the Astronomical Society of the Pacific, 1966
- The Solar Corona in Active Regions and the Thermal Origin of the Slowly Varying Component of Solar Radio Radiation.The Astrophysical Journal, 1961
- A New Instrument for Observing the Electron Corona.The Astrophysical Journal, 1957