NASA NTRS · 20000109971
Spectroscopy and X-Ray Astronomy
Abstract
The new x-ray astronomical observatories have sufficient spectroscopic capability to allow the determination of plasma conditions in the form of velocities, temperatures, densities, and turbulence parameters at levels that were previously unattainable. The utilization of these diagnostics are possible only if the atomic and plasma physics are well-enough understood to match the observational sensitivity.
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Holt, Stephen S.. 2000-10-01. Spectroscopy and X-Ray Astronomy. https://ntrs.nasa.gov/citations/20000109971
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