Longitude-Time Pattern for Quiet-Time Midlatitude Electron Precipitation

Abstract

During geomagnetically quiet times, particle precipitation at midlatitudes (2 < or = L < or = 4) results from a combination of pitch angle diffusion into the bounce loss cone and the opening of the bounce loss cone in the direction of drift to a maximum value which defines the drift loss cone. The geographical distribution of precipitation can thus be determined from geomagnetic field models which give the rate of change of the bounce loss cone size provided that an assumption is made about the spatial distribution of the source region where particles are scattered in the drift loss cone. Some observations indicate that the pitch angle scattering of kilovolt electrons occurs preferentially in the 0600-1200 LT quadrant of the magnetosphere. If the source of drift loss cone electrons is localized, precipitation into the midlatitude atmosphere will depend on both longitude and time of day. A simple model, in which the morning source is represented by a delta function at 0800 LT, leads to a qualitative picture of the morphology of precipitation in both Northern and Southern Hemispheres. The predictions of this model are consistent with some observations of 29 and 59 keV electrons from the low altitude satellite 1972-76B.

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Document Details

Document Type
Technical Report
Publication Date
May 10, 1977
Accession Number
ADA040470

Entities

People

  • Alfred L. Vampola
  • Janet G. Luhmann

Organizations

  • The Aerospace Corporation

Tags

Communities of Interest

  • Space

DTIC Thesaurus Topics

  • Acquisition
  • Altitude
  • Artificial Satellites
  • Atmospheres
  • Data Acquisition
  • Delta Functions
  • Electrons
  • Hemispheres
  • Longitude
  • Low Altitude
  • Observation
  • Particles
  • Precipitation
  • Scattering
  • Southern Hemisphere
  • Windshield Wipers
  • Windshields

Readers

  • Solar Physics
  • Space/Atmospheric Physics.

Technology Areas

  • Microelectronics
  • Space