Accession Number:

AD0637813

Title:

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

Descriptive Note:

Corporate Author:

SACRAMENTO PEAK OBSERVATORY SUNSPOT N MEX

Personal Author(s):

Report Date:

1966-01-01

Pagination or Media Count:

11.0

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 2 some solar flares are characterized by an appreciable intensity increase of X-ray emission in the short-wave region 0.1-1 A. Author

Subject Categories:

  • Astrophysics
  • Nuclear Physics and Elementary Particle Physics

Distribution Statement:

APPROVED FOR PUBLIC RELEASE