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Proceedings Paper

Analysis of the comparative responses of SMEI and LASCO
Author(s): Andrew Buffington; Jeff S. Morrill; P. Paul Hick; Russell A. Howard; Bernard V. Jackson; David F. Webb
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Paper Abstract

Surface-brightness responses of the SOHO-LASCO C3 coronagraph and of the Solar Mass Ejection Imager (SMEI) are compared, using measurements of a selection of bright stars that have been observed in both instruments. Seventeen stars are selected that are brighter than 4.5 magnitudes, are not known variables, and do not have a neighboring bright star. Comparing observations of these determines a scaling relationship between surface-brightness measurements from one instrument to those from the other. We discuss units of surface brightness for the two instruments, and estimate a residual uncertainty for the present scaling relationship.

Paper Details

Date Published: 20 September 2007
PDF: 6 pages
Proc. SPIE 6689, Solar Physics and Space Weather Instrumentation II, 66890B (20 September 2007); doi: 10.1117/12.734658
Show Author Affiliations
Andrew Buffington, Univ. of California, San Diego (United States)
Jeff S. Morrill, Naval Research Lab. (United States)
P. Paul Hick, Univ. of California, San Diego (United States)
Russell A. Howard, Naval Research Lab. (United States)
Bernard V. Jackson, Univ. of California, San Diego (United States)
David F. Webb, Boston College (United States)


Published in SPIE Proceedings Vol. 6689:
Solar Physics and Space Weather Instrumentation II
Silvano Fineschi; Rodney A. Viereck, Editor(s)

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