Using the Voyager Spacecraft for Solar EUV Spectral Radiometry

Details Using the Voyager Spacecraft for Solar EUV Spectral Radiometry Using the Voyager Spacecraft for Solar EUV Spectral Radiometry

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metro..30..397s&link_type=abstract

Metrologia, Volume 30, Issue 4, pp. 397-401 (1993).

Physics

1

Scientific paper

The ultraviolet spectrometers on the Voyager spacecraft are radiometrically stable and presently capable of making long-term, precise measurements of the solar spectral irradiance between 50 nm and 170 nm. If the detection efficiencies of these spectrometers were confirmed through a dedicated program of underflights, and if a campaign of regular Voyager observations of the Sun was instituted, some of the needs for timely, long-term solar EUV flux data could be efficiently met in this decade

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