Physics – Atomic Physics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp13b..05b&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SP13B-05
Physics
Atomic Physics
7509 Corona, 7546 Transition Region, 7549 Ultraviolet Emissions, 7594 Instruments And Techniques
Scientific paper
Using the Chianti database, we construct temperature response functions for the extreme ultraviolet and soft x-ray imaging channels on a variety of current and future solar observatories. Simulated observations in these channels are then inverted to recover the coronal differential emission measure. We investigate the effect of statistical error, and systematic uncertainties in the atomic physics and instrument calibration used to calculate the instrument temperature response functions, on the accuracy of the DEM recovery. By selecting different combinations of channels, we can characterize the ability of different instrument architectures to constrain the DEM, and identify an optimal combination of bandpasses for accurate DEM recovery.
Boerner Paul
Lemen James
Martinez-Galarce Dennis
Nitta Nariaki
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