Astronomy and Astrophysics – Astronomy
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.1709w&link_type=abstract
American Astronomical Society, SPD meeting #40, #17.09; Bulletin of the American Astronomical Society, Vol. 41, p.843
Astronomy and Astrophysics
Astronomy
Scientific paper
The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO) is a set of normal-incidence imaging telescopes with a variety of passbands in the UV and EUV. The instrument will observe solar plasmas from the chromosphere to the corona. Six of the passbands are dominated by iron lines and observe the emission from the optically thin corona, which is known to be a highly structured and multithermal region. This sort of imager data lends itself to differential emission measure analysis, which reconstructs the thermal structure of the observed plasma (with spatial resolution) across the field of view. The AIA Science Team will provide a data product that visually represents this thermal structure as a color mapped image. In this poster we discuss the analysis and visualization techniques we will employ to produce this data product. This work is supported by the AIA GSFC/NASA contract to Lockheed-Martin.
Boerner Paul
Schrijver Karel
Weber Mark A.
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