Predicting Proton Event Time Characteristics from Radio Burst Data,

Abstract

For events originating on the Western hemisphere, the delay before onset of the solar flare protons is shown to be well correlated (r about 0.80) with the rise time of the associated radio-burst at 2-3 GHz or the rise time of the h sub alpha flare. The peak flux time of the protons is shown to be very well correlated (r about 0.90) with the delay before onset, and fairly well correlated (r about 0.70) with the flare or radio rise time. These results allow a prediction of the proton event time characteristics from real time radio burst data. (Author)

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Document Details

Document Type
Technical Report
Publication Date
Jun 01, 1981
Accession Number
ADA106416

Entities

People

  • Pradip Bakshi
  • Thao D. Nguyen

Organizations

  • Boston College

Tags

Communities of Interest

  • C4I
  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Air Force
  • Databases
  • Flux Density
  • Frequency
  • Frequency Bands
  • Hemispheres
  • Intervals
  • Particles
  • Radio Frequency
  • Solar Atmosphere
  • Solar Flares
  • Spectra
  • Standards
  • Technical Information Centers
  • Time Intervals
  • Uncertainty
  • United States

Fields of Study

  • Physics

Readers

  • Solar Physics