Comparison of Coronal Data between the SPARTAN 201/WLC, SOHO/LASCO, and the MARK 3 Coronagraph

Details Comparison of Coronal Data between the SPARTAN 201/WLC, SOHO/LASCO, and the MARK 3 Coronagraph Comparison of Coronal Data between the SPARTAN 201/WLC, SOHO/LASCO, and the MARK 3 Coronagraph

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.1611k&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #16.11; Bulletin of the American Astronomical Society, Vol. 31, p.851

Astronomy and Astrophysics

Astronomy

Scientific paper

We compare coronal data from three different coronagraphs operating during the flight of SPARTAN 201-5 on Nov 1-3, 1998. The SPARTAN 201/White Light Coronagraph provides reliable data from 1.5--4.0 solar radii, bridging a gap in the radial coverage between the Mark 3 Coronagraph (which has reliable data from 1.16--1.8 solar radii) and the SOHO/LASCO C2 (2.5--6 solar radii). We will compare the radial brightness profiles of different coronal features as seen by the three different instruments, comparing the apparent structures in total white-light and polarized brightness.

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