Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsp54a..01t&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SP54A-01
Physics
7509 Corona, 7513 Coronal Mass Ejections (2101), 7594 Instruments And Techniques
Scientific paper
COR1 is the innermost coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. The paired COR1 telescopes observe the white-light K-corona from 1.4 to 4 solar radii in a waveband 22.5 nm wide centered on the H-alpha line at 656 nm. An internal polarizer allows the measurement of both total and polarized brightness. The co-alignment of the two COR1 telescopes is derived from the star Regulus for the Ahead spacecraft, and from an occultation of the Sun by the Moon for Behind. Observations of the planet Jupiter are used to establish absolute photometric calibrations for each telescope. The intercalibration of the two COR1 telescopes are compared using coronal mass ejection observations made early in the mission, when the spacecraft were close together. Comparisons are also made with the LASCO~C2 and Mauna Loa Solar Observatory Mk4 coronagraphs.
Reginald Nelson Leslie
Thompson William T.
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