LASCO Observations of the Solar Corona to 32 Rsun

Details LASCO Observations of the Solar Corona to 32 Rsun LASCO Observations of the Solar Corona to 32 Rsun

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.3717c&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #37.17; Bulletin of the American Astronomical Society, Vol. 28, p.880

Astronomy and Astrophysics

Astronomy

Scientific paper

The Large Angle Spectrometric Coronagraph (LASCO) was launched on board the SOHO satellite on 2 December 1995. The C3 externally-occulted coronagraph of LASCO observes the solar corona over a field from 3.7-32 R_ &sun;, using a 1024x1024 CCD detector with a pixel size corresponding to 56 arc sec. Observations can be made using color filters ranging from the blue (420-520 nm) to the near-IR (860-1050 nm), and through polarizing filters. We report on early observations of the solar corona out to 32 Rsun.

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