Search for Solar Recombination Lines in the Frequency Range 110-115 GHz.

Abstract

A search for solar recombination lines in active regions was made in the frequency range 110-115 GHz. The results, which were negative, are presented. An upper limit of T(l)/T(chr) approximately 10 to the minus 3rd power is given for the intensity ratio of the line to the continuum chromospheric emission. (Author)

Document Details

Document Type
Technical Report
Publication Date
Apr 15, 1973
Accession Number
AD0763719

Entities

People

  • Fred I. Shimabukuro
  • William J. Wilson

Organizations

  • The Aerospace Corporation

Tags

DTIC Thesaurus Topics

  • Emission
  • Frequency

Fields of Study

  • Physics

Readers

  • Microwave Engineering.
  • Plasma Physics / Magnetohydrodynamics
  • Solar Physics