Microwave Radio Emission from Loop Structures in the Solar Chromosphere and Corona.

Abstract

The overall objective of this research is to revisit the slowly varying or S component of solar microwave emission having in hand a much more detailed knowledge of active region structure than was available when the S component was studied extensively in the 1950s and 1960s. In particular we want to consider the radio emission from the active region loop structures so evident in Skylab X-ray and UV images. (Author)

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Document Details

Document Type
Technical Report
Publication Date
Oct 01, 1980
Accession Number
ADA097139

Entities

People

  • John F. Vesecky

Organizations

  • Stanford University

Tags

Communities of Interest

  • Air Platforms

DTIC Thesaurus Topics

  • Absorption
  • Absorption Coefficients
  • Analytic Geometry
  • Brightness
  • Contracts
  • Frequency
  • Geometric Forms
  • Geometry
  • Magnetic Fields
  • Magnetic Flux
  • Magnetic Flux Density
  • Military Research
  • Observation
  • Radar Astronomy
  • Radio Astronomy
  • Temperature Gradients
  • X Rays

Readers

  • Solar Physics
  • Strategic Security Studies