An annular eclipse on May 31, 2003, observed in extreme ultraviolet

Details An annular eclipse on May 31, 2003, observed in extreme ultraviolet An annular eclipse on May 31, 2003, observed in extreme ultraviolet

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sosyr..40..348n&link_type=abstract

Solar System Research, Volume 40, Issue 4, pp.348-353

Physics

96.60.P-

Scientific paper

The CORONAS-F spacecraft crossed the zone of the ring solar eclipse three times on May 31, 2003. A considerable decrease in solar radiation was detected by the spacecraft instruments for these moments. The passages through the eclipse zone were registered by the VUSS instrument, which measured the shortwave solar radiation flux near the hydrogen Lyman alpha line, and by the DIFOS instrument, which was sensitive to infrared, visible, and near-ultraviolet radiation. The eclipse is also clearly seen in solar images obtained by the X-ray SPIRIT telescope. Some details of measurement results are discussed.

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