The Atmospheric Imaging Assembly and Temperature Diagnostics

Details The Atmospheric Imaging Assembly and Temperature Diagnostics The Atmospheric Imaging Assembly and Temperature Diagnostics

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.6906w&link_type=abstract

American Astronomical Society Meeting 204, #69.06; Bulletin of the American Astronomical Society, Vol. 36, p.795

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The Atmospheric Imaging Assembly (AIA) will be one of the instruments on the Solar Dynamics Observatory (SDO). It will image the solar transition region and corona in multiple EUV and UV wavelengths simultaneously, using four aligned telescopes. Hence, AIA will be capable of high-cadence, spatially resolved temperature discrimination of solar plasmas. We discuss the design of AIA, with focus on its ability for temperature diagnostics. We consider different methods for reconstruction of differential emission measures, since this will be one of the more important data products.
This work is supported under contract SP02D4301R to the Lockheed Martin Corp.

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