Prediction of Solar-Terrestrial Disturbances: Decay Phase of Energetic Proton Events.

Abstract

The decay phase of solar proton events, as observed at Earth, depends strongly on the proton injection history, the distribution of the proton population in solar longitude, and the state of the interplanetary medium. In an attempt to gain an additional diagnostic of these complex conditions, the evolution of the flux anisotropy is examined, both theoretically and observationally. In relatively simple events, the component of the flux anisotorpy parallel to the interplanetary magnetic field proves to be a useful indicator. In more complicated events additional information from solar wind, magnetic field, and lower energy (< 1 MeV) ions would appear to be necessary. Research papers on these related quantities are also cited. (Author)

Open PDF

Document Details

Document Type
Technical Report
Publication Date
Oct 01, 1982
Accession Number
ADA130103

Entities

People

  • Edmond C. Roelof

Organizations

  • Johns Hopkins University

Tags

Communities of Interest

  • Space

DTIC Thesaurus Topics

  • Bow Shock
  • Charged Particles
  • Contracts
  • Convection
  • Cosmic Rays
  • Electric Fields
  • Electromagnetic Spectra
  • Jet Propulsion
  • Magnetic Fields
  • Magnetic Storms
  • Physics
  • Physics Laboratories
  • Shock
  • Solar Activity
  • Solar Cycle
  • Solar Flares
  • United States

Fields of Study

  • Physics

Readers

  • Plasma Physics / Magnetohydrodynamics
  • Solar Physics
  • Systems Analysis and Design