Two Classes of Gamma-Ray/Proton Flares: Impulsive and Gradual. Revision,

Abstract

We have studied various properties of gamma ray/proton flares, which produce nuclear gamma rays and/or interplanetary energetic protons. We have found that there exist two classes of gamma ray/proton (GR/P) flares, with each class having many distinct characteristics in common. Gradual GR/P flares (so named because of gradual variations of hard X-ray fluxes with duration of spike bursts longer than 90 s) have the following characteristics: long duration (> 10 min) hard / X-ray and microwave emission, gradual variation of microwave flux, relatively large ratios of microwave to hard X-ray fluxes, large H-alpha areas, long-duration soft X-ray emission (> 1 hr), hard X-ray emission from extended coronal loops, interplanetary type II emission, coronal mass ejections, and production of large numbers of interplanetary energetic protons. Impulsive GR/P flares display directly opposing behavior in the above respects. However, the two classes of GR/P flares have a few characteristics common to both of them.

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Document Details

Document Type
Technical Report
Publication Date
Nov 01, 1985
Accession Number
ADA163105

Entities

People

  • Taeil Bai

Organizations

  • Stanford University

Tags

Communities of Interest

  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Classification
  • Coronal Mass Ejections
  • Cosmic Rays
  • Detectors
  • Ejection
  • Energy Bands
  • Flux Density
  • Gamma Rays
  • Hard X Rays
  • High Energy
  • Human Behavior
  • Microwaves
  • Observation
  • Soft X Rays
  • Solar Flares
  • X Ray Spectra
  • X Rays

Fields of Study

  • Physics

Readers

  • Solar Physics