Computer Science – Sound
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp12a..01m&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SP12A-01
Computer Science
Sound
7509 Corona, 7519 Flares, 7549 Ultraviolet Emissions, 7554 X Rays, Gamma Rays, And Neutrinos, 7594 Instruments And Techniques
Scientific paper
The Advanced Technology Solar Spectroscopic Imager (ATSSI) sounding rocket payload will employ a quantum microcalorimeter detector placed at the focus of a Wolter I telescope to study energy release in the active solar corona. Over its nominal 300 second observing period, the ATSSI will record ~120 spectra with its 2x2 array of detectors. These spectra span the range of 6-25 Å with spectral resolution of ~650, spatial resolution of ~5 arcsec, and time cadence of ~10 seconds. The ATSSI will record high signal-to-noise measurements of the intensity of ~12 emission lines formed from 1-10 MK, including the temperature and density-sensitive lines of Fe XVII in the 15-17 Å region. The ATSSI's unique capabilities will provide powerful constraints on the parameters of the coronal heating mechanism.
Baker Patrick
Barbee Troy
Boerner Paul
Cabrera Blas
Chakraborty Subhasish
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