New possibilities of non-eclipse observations of the solar K-corona with liquid-mirror telescopes

Details New possibilities of non-eclipse observations of the solar K-corona with liquid-mirror telescopes New possibilities of non-eclipse observations of the solar K-corona with liquid-mirror telescopes

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..132..271v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 132, April 1991, p. 271-277.

Physics

Polarimetry, Solar Corona, Solar Instruments, Telescopes, Brightness Distribution, Mirrors, Space Observations (From Earth)

Scientific paper

Experimental and methodical possibilities of modern observations of the solar K-corona have been analyzed. It is shown that for obtaining information on matter distribution and dynamics in the internal solar corona, it is necessary to measure both its polarization component and its total radiation in the continuum. In order to reduce the atmospheric and instrumental background, the employment of K-coronameters with an apodized liquid mirror is proposed. Such coronameters should operate in the near infrared range and be installed at a latitude zone where the sun can be observed in the zenith.

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