Center-to-limb Variations From SDO Extreme Ultraviolet Variability Experiment (EVE)

Details Center-to-limb Variations From SDO Extreme Ultraviolet Variability Experiment (EVE) Center-to-limb Variations From SDO Extreme Ultraviolet Variability Experiment (EVE)

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640202h&link_type=abstract

American Astronomical Society, AAS Meeting #216, #402.02; Bulletin of the American Astronomical Society, Vol. 41, p.873

Astronomy and Astrophysics

Astronomy

Scientific paper

Center-to-limb variation of a coronal emission is important for accurately modeling solar irradiance. The complex structure of the corona, however, makes it difficult to calculate these variations. We determine the center-to-limb variation for coronal lines using early observations from the Extreme ultraviolet Variability Experiment (EVE) on board the NASA Solar Dynamics Observatory (SDO), launched on 11 February 2010. While EVE's measurements are not spatially resolved, the changes in irradiance as active regions rotate across the disk allow us to determine the center-to-limb variations of multiple coronal lines over a range of formation temperatures.

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