Observations of Solar X-ray Emission in the Band 44-60 Å from U.S. Naval Research Laboratory Satellite 1963-21-C

Details Observations of Solar X-ray Emission in the Band 44-60 Å from U.S. Naval Research Laboratory Satellite 1963-21-C Observations of Solar X-ray Emission in the Band 44-60 Å from U.S. Naval Research Laboratory Satellite 1963-21-C

Aug 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964natur.203..962t&link_type=abstract

Nature, Volume 203, Issue 4948, pp. 962-963 (1964).

Physics

2

Scientific paper

THE U.S. Naval Research Laboratory has instrumented a series of satellites for the investigation of solar X-ray and ultra-violet emissions1,2. It has generously allowed the Radio Research Station, Slough, to participate in these experiments and has provided the necessary information for reducing telemetry data. This communication presents some results for X-rays in the band 44-60 Å derived from telemetry recorded from satellite 1963-21-C at the D.S.I.R. Radio Research Minitrack Station at Winkfield during June-July 1963. The principle of the experiment has been used on previous satellites and has been described by Acton et al.2.

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