Alfven Waves in the Solar Wind in Association with Solar Energetic Particles: Sunspot Umbral Origin.

Abstract

We report on a search for Alfven waves in the solar wind during solar particle events. During the period June 6-8, 1979, we find clear signatures of outgoing Alfven waves which could have been released from the sun simultaneously with the initial release of energetic particles. The waves are soliton-like, with durations of 200-900 seconds. An isolated square Alfven solution is also seen when the first particles (with E approximately 57 MeV) are detected: the width of this solution is approximately 950 seconds. A series of five small amplitude spikes in the magnetic field are also seen, preceding the arrival of the first particles by a few hours. The spikes are separated by intervals of 854 + or - 20 seconds. We suggest that these periodicities are determined by conditions at the sun. The features which we have detected are consistent with Alfven waves released from the umbra of a sunspot during a flare. (Author)

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Document Details

Document Type
Technical Report
Publication Date
Feb 04, 1983
Accession Number
ADA128046

Entities

People

  • A. J. Owens
  • D. J. Mullan

Tags

Communities of Interest

  • Energy and Power Technologies
  • Space

DTIC Thesaurus Topics

  • Air Force
  • Atmospheres
  • Convection
  • Coordinate Systems
  • Cosmic Rays
  • Cross Correlation
  • Detectors
  • Interplanetary Space
  • Magnetic Fields
  • Magnetometers
  • Measurement
  • Particle Flux
  • Solar Atmosphere
  • Solar Wind
  • Square Waves
  • Sun
  • Wave Propagation

Fields of Study

  • Physics

Readers

  • Atmospheric Science / Meteorology, specifically Wind Wave Turbulence.
  • Solar Physics