THE TIME DEPENDENCE OF THE LOW ENERGY PROTON BELTS.

Abstract

The time dependence of the low energy proton space distributions and differential energy distributions at 8 energies from 0.17-3.4 MeV are presented for the period of August 15, 1964 to February 8, 1965. The data were obtained from the directional proton spectrometer on the satellite 1964-45A which was launched on August 14, 1964 into a near polar orbit with a 3765 km apogee and a 270 km perigee. The proton flux decay constant can be expressed as 1/tau 1/(DAY) = (-.0007 + or - .0007) + (.0033 + or - .0009) 1n sub e E(MeV). Protons of 0.2 MeV decreased with an apparent lifetime of 150 days, those of 1 MeV were constant and protons of 2.5 MeV increased with an apparent lifetime of 500 days. PHE MAXIMUM PEAK HEIGHTS OF THE ENERGY DIStributions decreased by less than a factor of 2 and the energy spectra hardened slightly with time. The positions of the maxima remained almost constant. Therefore, the low energy proton radiation belts were rather stable from August 15, 1964 to February 8, 1965. (Author)

Document Details

Document Type
Technical Report
Publication Date
Nov 01, 1966
Accession Number
AD0805729

Entities

People

  • R. Stephen White

Organizations

  • The Aerospace Corporation

Tags

Communities of Interest

  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Apogees
  • Apsides
  • Artificial Satellites
  • Direction Finding
  • Directional
  • Navigation
  • Orbits
  • Polar Orbits
  • Position Finding
  • Radiation
  • Spectra
  • Spectrometers
  • Time Dependence

Fields of Study

  • Physics

Readers

  • Mathematics or Statistics
  • Solar Physics
  • Space Exploration and Orbital Mechanics.

Technology Areas

  • Space
  • Space - Orbital Debris