The white-light coronograph for KORONAS-I

Details The white-light coronograph for KORONAS-I The white-light coronograph for KORONAS-I

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...257l...7b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 257, no. 2, p. L7, L8.

Astronomy and Astrophysics

Astrophysics

Coronagraphs, Satellite Observation, Solar Corona, Solar Diameter, Solar Wind, Charge Coupled Devices, Czechoslovakia, Solar Observatories, Ultraviolet Telescopes, X Ray Telescopes

Scientific paper

A description of the white-light coronagraph for, and the scientific goals of the experiment on, the KORONAS-I satellite, is presented. The observations in the solar corona are to range from 2.2 to 10.0 solar radii, and the resolving power is 76 arcsec. The experiment is to address the questions of coronal heating, the plasma flowing in coronal rays, and solar-terrestrial interrelations.

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