NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Positron annihilation radiation from solar flaresPositron-annihilation radiation has been observed from the June 21, 1980 and June 3, 1982 flares by the gamma-ray spectrometer on the Solar Maximum Mission satellite. The observed 0.511-MeV line fluences from the flares were 14.6 + or - 3.3 gamma/sq cm and 103 + or - 8 gamma/sq cm, respectively. Measurement of the line width establishes an upper limit to the temperature in the annihilation region of 3 x 10 to the 6th K. The time dependence of the 0.511-MeV line during the 1980 flare is consistent with the calculations of Ramaty et al. (1983) for positrons created in the decay of radioactive nuclei. The time dependence of the 0.511-MeV line for the 1982 flare is more complex and requires more detailed study.
Document ID
19850049127
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Share, G. H.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington DC, United States)
Chupp, E. L.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Forrest, D. J.
(New Hampshire, University Durham, NH, United States)
Rieger, E.
(Max-Planck-Institut fuer Physik und Astrophysik Garching, Germany)
Date Acquired
August 12, 2013
Publication Date
January 1, 1983
Subject Category
Solar Physics
Meeting Information
Meeting: Positron-electron pairs in astrophysics
Location: Greenbelt, MD
Start Date: January 6, 1983
End Date: January 8, 1983
Accession Number
85A31278
Funding Number(s)
CONTRACT_GRANT: NASA ORDER S-70926-A
CONTRACT_GRANT: NAS5-23761
CONTRACT_GRANT: BMFT-01-OK-017-ZA/WS/WRK-2754
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available