Vacuum Ultraviolet Backgrounds from Space - Ten Years After

Abstract

The past ten years has seen progress in the understanding of the ultraviolet background of the earth's atmosphere. These airglow, auroral, and scattering emission sources set limits on the usefulness of UV for space observations. They also, however, enable several types of passive remote sensing; such as, electron density profiles, neutral density and composition, and auroral location and strength. The paper describes our measurements and data analysis in the these areas. UV imaging the aurora has been achieved by four experiments, and these are briefly reviewed. UV imaging of the aurora has been achieved by four experiments, and these are briefly reviewed. UV imaging has opened up a new way to study solar-terrestrial relationships.

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Document Details

Document Type
Technical Report
Publication Date
Aug 01, 1989
Accession Number
ADA211353

Entities

People

  • F. J. Leblanc
  • J. C. Larrabee
  • R. E. Huffman

Organizations

  • Air Force Research Laboratory

Tags

Communities of Interest

  • Space

DTIC Thesaurus Topics

  • Altitude
  • Analyzers
  • Artificial Satellites
  • Databases
  • Detectors
  • Electron Density
  • Electron Energy
  • Electrons
  • Emission
  • Environment
  • Geophysics
  • Measurement
  • Remote Detectors
  • Remote Sensing
  • Scattering
  • Spacecraft
  • Spectrometers

Readers

  • Pulsed Power and Plasma Physics.
  • Space/Atmospheric Physics.
  • Systems Analysis and Design

Technology Areas

  • Microelectronics
  • Space