AN INVESTIGATION OF THE X-RAY EMISSION OF SOLAR FLARES BY THE RADIO ASTRONOMICAL METHOD,

Abstract

The following conclusions are based on a study of the frequency dependence of the attenuation of cosmic radio noise during sudden ionospheric disturbances: (1) the spectral distribution of the X-ray emission intensity of flares varies for each flare, and (2) some solar flares are characterized by an appreciable intensity increase of X-ray emission in the short-wave region. (Author)

Document Details

Document Type
Technical Report
Publication Date
Jan 01, 1963
Accession Number
AD0428086

Entities

People

  • Alice B. Dunn
  • Y. I. Neshpor

Tags

DTIC Thesaurus Topics

  • Attenuation
  • Emission
  • Frequency
  • Intensity
  • Ionospheric Disturbances
  • Noise
  • Noise (Radio)
  • Solar Flares
  • X Rays

Fields of Study

  • Physics

Readers

  • Astronomy and Astrophysics.
  • Solar Physics
  • Spectroscopy.