Polarization Spectra of Centimeter Wavelength Solar Bursts Using Whole-Sun Observations.

Abstract

The physics of microwave-burst emission is briefly examined to give the rationale for investigating polarization spectra. The instruments used to carry out the 9.4 GHz and 7 GHz circular-polarization measurements and the 5 GHz Stokes-parameter measurements are described. A survey of the August 1972 to December 1973 period produced a table of 45 bursts, from which some limited results were obtained. About 75 to 80 percent of all bursts are circularly polarized, with varying polarization over the 5 to 9.4 GHz range. For most bursts where the circular polarization pc increases toward the upper or lower end of the 5 to 9.4 GHz range, the total intensity I also increases in that direction. The few bursts having a pc sense reversal in the 5 to 9.4 GHz range also have a spectral maximum of I at roughly the same frequency. Some simplified explanations of the results are presented.

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Document Details

Document Type
Technical Report
Publication Date
Dec 08, 1976
Accession Number
ADA038782

Entities

People

  • Donald A. Guidice

Organizations

  • Air Force Research Laboratory

Tags

Communities of Interest

  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Air Force
  • Audio Frequency
  • Bandwidth
  • C Band
  • Circular Polarization
  • Detectors
  • Drops
  • Flux Density
  • Frequency
  • Instrumentation
  • Linear Polarization
  • Measurement
  • Microwave Frequency
  • Noise
  • Observatories
  • Polarization
  • Radiation

Fields of Study

  • Physics

Readers

  • Electromagnetic Wave Scattering and Antenna Radiation Engineering
  • Electronics Engineering
  • Space/Atmospheric Physics.