Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000adnx.conf..117t&link_type=abstract
Atomic Data Needs for X-ray Astronomy, p. 117
Astronomy and Astrophysics
Astrophysics
Ion Beams, Heavy Ions, Storage Rings (Particle Accelerators), X Ray Spectroscopy, Astrophysics, Ion Traps (Instrumentation), Time Dependence, Extreme Ultraviolet Radiation, Ion Storage, Transition Probabilities, Far Ultraviolet Radiation
Scientific paper
The understanding of the light received from astrophysical sources requires knowledge of atomic structure and dynamics, or of excitation cross sections and conditions, wavelengths and transition probabilities, f-values, branching ratios and level lifetimes. Fast ion beams (by beamfoil spectroscopy) and ion traps, as well as their cross-breed, the heavy-ion storage ring, can contribute to the field of X-ray astronomy. Fast-ion beam spectroscopy has a long track record in all spectral ranges, including Extreme Ultraviolet (XUV) and X-ray, with a plethora of data supporting astrophysics. In contrast, most of the time-resolved work with the ion trap techniques has been done in the Ultraviolet (UV) and Vacuum Ultraviolet (VUV)/Extreme Ultraviolet (EUV) above 100 Angstroms, but it can be extended into the region of interest.
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