The diurnal variation of cosmic ray electrons

Details The diurnal variation of cosmic ray electrons The diurnal variation of cosmic ray electrons

Oct 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969p%26ss...17.1781s&link_type=abstract

Planetary and Space Science, Volume 17, Issue 10, p. 1781-1793.

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Scientific paper

The cosmic ray electron intensity between 30 MeV and 1500 MeV has been measured with a system composed of a Cerenkov telescope and a lead-scintillator sandwich detector. Results are presented from a balloon flight made at Kiruna, Northern Sweden, in 1967. The electron measurements were made between 3.7 and 4.5g cm-2 residual atmosphere from local midnight until after local noon. The results show that at energies between 30 MeV and 900 MeV the durnal variation is 0 +/- 25 per cent. This is compared with other results from Fort Churchill, Canada and with satellite observations. Present address: NASA, Goddard Space Flight Center, Greenbelt, Md. 20771, U.S.A.

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