Ground-based observations of the corona in the visible and NIR spectral ranges

Details Ground-based observations of the corona in the visible and NIR spectral ranges Ground-based observations of the corona in the visible and NIR spectral ranges

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...60e&link_type=abstract

Max-Planck-Inst. für Aeronomie, International Solar Wind 8 Conference, p. 60

Mathematics

Logic

Coronal Holes, Infrared Radiation, Line Spectra, Solar Corona, Solar Radiation, Coronagraphs, Solar Wind, Stellar Mass

Scientific paper

Since late 1993 we have been using a mirror coronagraph on Pic du Midi (PICO) to observe the solar emission corona in several spectral lines of (FE-X), (FE-XIII), and (FE-XIV). For good meteorological conditions the diffuse corona and coronal holes in between can be seen out to 1.2 solar mass for sun center. Active regions can be mapped to bond 1.5 solar mass in the green and infrared lines. Recent observations of PICO are presented.

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