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Interplanetary and Solar Electrons 2 keV to > 1 MeV

NSSDCA ID: 1978-079A-09

Mission Name: ISEE 3
Principal Investigator:Prof. Kinsey A. Anderson

Description

This experiment was designed to study spectra and anisotropies of interplanetary and solar electrons (2 to 1000 keV) in the transition energy range between solar wind and low-energy cosmic rays. The electrons were measured by a pair of passively cooled, surface-barrier, semiconductor-detector telescopes (approximately 15 keV to approximately 1 MeV) and by a hemispherical plate electrostatic analyzer with channel-multiplier detectors (2-18 keV). Counting rates were sectored into angular sectors about either the magnetic field or the sun direction. The telescope yielded 8 or 16 sectors and the analyzer yielded 16 sectors.

Alternate Names

  • ISEE3/InterplanetaryandSolarElectrons
  • X-Ray and Electrons

Facts in Brief

Mass: 11.6 kg
Power (avg): 5 W

Funding Agency

  • NASA-Office of Space Science United States

Discipline

  • Space Physics: Heliospheric Studies

Additional Information

Questions and comments about this experiment can be directed to: Dr. H. Kent Hills

 

Personnel

NameRoleOriginal AffiliationE-mail
Dr. Sharad R. KaneOther InvestigatorUniversity of California, Berkeleysharadk@ssl.berkeley.edu
Prof. Robert P. LinOther InvestigatorUniversity of California, Berkeley
Dr. Dean F. SmithOther InvestigatorHigh Altitude Observatorydean.f.smith@noaa.gov
Prof. Kinsey A. AndersonPrincipal InvestigatorUniversity of California, Berkeleyanderson@ssl.berkeley.edu

Selected References

  • Anderson, K. A., et al., Experiment to measure interplanetary and solar electrons, IEEE Trans. Geosci. Electron., GE-16, No. 3, 153-156, July 1978.
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