Solar wind density model from km-wave type III bursts
- 1 March 1973
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 29 (1), 197-209
- https://doi.org/10.1007/bf00153449
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- The Electron Temperature in the Two-Component Solar WindThe Astrophysical Journal, 1971
- Dynamic Spectra of Type III Solar Bursts from 4 TO 2 MHz Observed by Ogo-IiiThe Astrophysical Journal, 1970
- Type III radio bursts in the outer coronaSolar Physics, 1969
- Brightness variations of the white light corona during the years 1964?67Solar Physics, 1969
- Type III solar radio noise bursts at hectometer wavelengthsPlanetary and Space Science, 1969
- Observations of the 1963 July 20 Solar Eclipse: II. The Electron Density in the Solar Corona in the Region 5 < R/R0 < 16 obtained from Measurements of Fraunhofer Line Depth, and the Polarization of the F CoronaMonthly Notices of the Royal Astronomical Society, 1966
- Spectral Observations of Solar Radio Bursts.IV. The Exciters of Fast-Drift Bursts.The Astrophysical Journal, 1963
- A Comparison of the Dynamic Spectra of Solar Radio Bursts in the Decimeterand Meter-Wave Ranges.The Astrophysical Journal, 1961
- A Study of the Outer Corona from a High Altitude Aircraft at the Eclipse of 1954 June 30: II. Electron Densities in the Outer Corona and Zodiacal Light RegionsMonthly Notices of the Royal Astronomical Society, 1956
- Strahlung, Ergiebigkeit und Elektronendichte der SonnenkoronaAstronomische Nachrichten, 1937