Interplanetary Cosmic Ray Intensity: 1972-1984 and Out to 32 AU.

Abstract

Using a number of Geiger-Mueller tubes in the University of Iowa instruments on Pioneer 10 and Pioneer 11, we have measured the interplanetary intensity of cosmic rays E sub P > 80 meV) over a complete solar activity cycle and out to a helicocentric distance of over 32 AU. Free space values of the background corrections due to the radioisotope thermal generators were determined during passage of Pioneer 11 under the dense rings of Saturn during the 1 September 1979 encounter. These improved corrections and ones inferred therefrom for Pioneer 10 have supplanted earlier estimates and have been applied to all data.

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Document Details

Document Type
Technical Report
Publication Date
Aug 01, 1984
Accession Number
ADA145130

Entities

People

  • B. A. Randall
  • James A. van Allen

Organizations

  • University of Iowa

Tags

Communities of Interest

  • Advanced Electronics
  • Energy and Power Technologies
  • Space

DTIC Thesaurus Topics

  • Accuracy
  • Cosmic Rays
  • Detectors
  • Energy
  • Galactic Cosmic Rays
  • Intensity
  • Isotopes
  • Kinetic Energy
  • Latitude
  • Orbits
  • Radiation
  • Radioactive Decay
  • Solar Activity
  • Solar System
  • Spacecraft
  • Sun
  • Trajectories

Fields of Study

  • Physics

Readers

  • Solar Physics

Technology Areas

  • AI & ML
  • AI & ML - Bayesian Inference
  • Space
  • Space - Hall-Effect Thruster