The Altitude at which Solar-Flare-Induced Ionization is Released

Abstract

Observations of instantaneous frequency and angle-of-arrival changes during solar flares suggest that new ionization is introduced initially somewhere just above the E region--very probably in the height region 120 to 140 km, although even higher heights are possible. This initial ionization may or may not be followed by the generation of ionization in the absorbing D region. The time variation of height at which solar-flare-induced ionization is released, suggests that the ionization-producing radiant energy is initially soft, and then hardens as the flare progresses.

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Document Details

Document Type
Technical Report
Publication Date
Dec 04, 1961
Accession Number
AD0269748

Entities

People

  • D. P. Kanellakos
  • O. G. Villard Jr.

Organizations

  • Stanford University

Tags

Communities of Interest

  • Advanced Electronics
  • Energy and Power Technologies
  • Weapons Technologies

DTIC Thesaurus Topics

  • Air Force
  • Angle Of Arrival
  • Charged Particles
  • Cosmic Rays
  • Electromagnetic Wave Propagation
  • Electron Density
  • Electrons
  • Frequency
  • Frequency Shift
  • Ionization
  • Ionosphere
  • Measurement
  • Observation
  • Puerto Rico
  • Solar Activity
  • Solar Flares
  • Transmitters

Readers

  • Astronomy and Astrophysics.
  • Mechanical Engineering/Mechanics of Materials.
  • Solar Physics