The STEREO SECCHI/EUVI EUV coronal imager

Details The STEREO SECCHI/EUVI EUV coronal imager The STEREO SECCHI/EUVI EUV coronal imager

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007spie.6689e...3w&link_type=abstract

Solar Physics and Space Weather Instrumentation II. Edited by Fineschi, Silvano; Viereck, Rodney A. Proceedings of the SPIE, Vol

Physics

Scientific paper

The SECCHI Extreme Ultraviolet Imager (EUVI) is a pair of EUV telescopes on the NASA STEREO mission that was successfully launched in October 2006. The two telescopes, one on each STEREO spacecraft observe the solar corona in three dimensions out to 1.7 solar radii, and with a pixel resolution of 1.59 arcsec. The focus of the EUVI observations is the initiation and early evolution of coronal mass ejections (CMEs). This paper presents a preliminary assessment of the on-orbit performance of the EUVI.

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