Source heights of metre wavelength bursts of spectral types I and III

Details Source heights of metre wavelength bursts of spectral types I and III Source heights of metre wavelength bursts of spectral types I and III

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...50..437s&link_type=abstract

Solar Physics, vol. 50, Nov.-Dec. 1976, p. 437-445.

Astronomy and Astrophysics

Astronomy

26

Electron Density (Concentration), Radio Astronomy, Solar Corona, Solar Limb, Type 3 Bursts, Error Analysis, Optical Density, Plasma Frequencies, Radial Distribution, Solar Spectra

Scientific paper

Direct measurements by the Culgoora radioheliograph of the apparent source heights of type I and type III bursts at the solar limb are described. The average observed height is approximately the same for type I and type III sources. The heights are somewhat larger than previous estimates. After refraction effects are removed, the present results give an electron-density model for the source region below 3 solar radii with densities on the average between 8 and 10 times the values for corresponding heights in the quiet K-corona.

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