Calibration of AIA/SDO: Accessing and implementing the response functions

Details Calibration of AIA/SDO: Accessing and implementing the response functions Calibration of AIA/SDO: Accessing and implementing the response functions

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh23c1871b&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH23C-1871

Astronomy and Astrophysics

Astrophysics

[7509] Solar Physics, Astrophysics, And Astronomy / Corona, [7538] Solar Physics, Astrophysics, And Astronomy / Solar Irradiance, [7549] Solar Physics, Astrophysics, And Astronomy / Ultraviolet Emissions, [7594] Solar Physics, Astrophysics, And Astronomy / Instruments And Techniques

Scientific paper

The initial photometric calibration of AIA, based on preflight measurements of the response of the telescope components, is complete. The estimated accuracy is of order 25%, which is consistent with the results of comparisons with full-disk irradiance measurements and spectral models. We describe the process of accessing the wavelength response (effective area) functions, and of generating temperature response functions using a model of the spectral emissivity.

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