The Effect of Solar Activity on the Cosmic Ray Intensity at Solar Minimum

Abstract

In examining the cosmic ray intensity between successive solar minima, it has been noted that the intensity at 1 AU was slightly higher between the 19th and 20th solar cycles (i.e. 1965) and between the 21st and 22nd solar cycles (i.e. 1987) than between the 20th and 21st solar cycles (i.e. 1976). The fact that the galactic cosmic ray intensity in the mid 70's did not return to the levels observed at the other two solar minima is attributed to increased solar activity throughout the 1976 solar minimum period.

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Document Details

Document Type
Technical Report
Publication Date
Apr 29, 1991
Accession Number
ADA235342

Entities

People

  • Don F. Smart
  • Margaret Shea

Organizations

  • Phillips Laboratory

Tags

Communities of Interest

  • Air Platforms

DTIC Thesaurus Topics

  • Availability
  • Classification
  • Cosmic Rays
  • Cycles
  • Detectors
  • Galactic Cosmic Rays
  • Geophysics
  • High Latitudes
  • Intensity
  • Magnetic Fields
  • Radiation
  • Radio Frequency
  • Security
  • Solar Activity
  • Solar Cycle
  • Solar Flares
  • Sunspots

Fields of Study

  • Physics

Readers

  • Mathematics or Statistics
  • Space/Atmospheric Physics.