THE SPECTRUM OF A LOCAL SOURCE OF RADIO EMISSION ON THE SUN,

Abstract

The spectrum of local radio emission sources is most directly determined by simultaneous observations of several waves at a high angular resolution. Such observations of the emission of a source associated with the group of spots No. 188 (the numeration of the bulletin ''Solar Data'' (S sub p = 1076)) in the range from 0.8 cm to 30 cm were carried out during the solar eclipse on 19 April 1959. The results are shown as a graph for the ratio of the source flux F sub u, to the flux of the undisturbed sun, F sub o. Data are from the observations of the joint expedition of the AN SSSR and the AN KNR and from observations in Japan. (Author)

Document Details

Document Type
Technical Report
Publication Date
Aug 15, 1962
Accession Number
AD0284129

Entities

People

  • A.p. Molchanov

Organizations

  • National Air and Space Intelligence Center

Tags

DTIC Thesaurus Topics

  • Eclipses
  • Emission
  • Observation
  • Solar Eclipses
  • Spectra

Fields of Study

  • Environmental science
  • Physics

Readers

  • Astronomy/Astrophysics
  • Information Retrieval
  • Seismology