Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-26T17:33:42.464Z Has data issue: false hasContentIssue false
  • English
  • Français

52. Brightness distribution of the sun at 1·45 metres

Published online by Cambridge University Press:  14 August 2015

J. Firor
J. Firor*
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, D.C., U.S.A.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The brightness distribution of the quiet sun at radio frequencies is of importance in determining the electron density and temperature in the chromosphere and the corona. Calculations made by Smerd, based on parameters derived from optical observations of the sun, indicate that the brightness distributions for wave-lengths near 1·5 metres are sensitive to the assumed coronal conditions and hence are well suited to checking these parameters.

Type
Part IV: The Quiet Sun
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 294 - 297
Copyright
Copyright © Cambridge University Press 1957