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- W2074912500 abstract "Neutron detectors on the Vela satellites have been operating in space at 16–20 RE since October 17, 1963. An attempt to measure the near-earth intensity of a steady-state solar neutron emission has been made by inspection of the neutron detector counting rate records before, during, and after the satellites are eclipsed by the moon or by the earth. The solar flux was too low to be measured; an upper limit of 0.01 neutron cm−2 sec−1 was determined, assuming a spectrum similar to the terrestrial neutron albedo spectrum. Counting rate records also have been inspected for measurable intensities of solar neutron bursts following solar flares, including two importance 3 flares and a number of flares with associated type IV solar radio noise bursts. No detectable events have been found to date. Neutron bursts with integrated intensities at the earth of 1.5×103 neutrons cm−2 could have been detected. The search is continuing as the solar activity rises from solar minimum." @default.
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- W2074912500 date "1966-10-01" @default.
- W2074912500 modified "2023-09-26" @default.
- W2074912500 title "A search for solar neutrons near solar minimum" @default.
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- W2074912500 doi "https://doi.org/10.1029/jz071i019p04605" @default.
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