Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.264..627j&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Vol. 264, NO. 3/OCT1, P. 627, 1993
Astronomy and Astrophysics
Astronomy
56
Atomic Data - Line: Identification - Plasmas - Techniques: Spectroscopic - Sun: Flares - Ultraviolet: Stars
Scientific paper
We report 42 new Fe X-Fe XIV lines identified from solar, beam-foil, tokamak and laser-produced plasma spectra. 19 of these have been found in solar spectra. We also report some new laboratory data confirming previous solar identifications. The lines are of 3s23pκ-3s23pκ-13d and 3s23pκ-3s3pκ+1 types and lie between 169 and 510 Å. We also give a new value for the forbidden 3p3(4S3/2-2P1/2) transition of Fe XII. In all, we have determined 17 new energy levels in these ions with uncertainties of ±10 cm-1.
Isler R. C.
Jupén C.
Träbert Elmar
No associations
LandOfFree
Solar Identifications of Fex-Fexiv Based on Comparison with Beam-Foil Tokamak and Laser-Produced Plasma Spectra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Solar Identifications of Fex-Fexiv Based on Comparison with Beam-Foil Tokamak and Laser-Produced Plasma Spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Identifications of Fex-Fexiv Based on Comparison with Beam-Foil Tokamak and Laser-Produced Plasma Spectra will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1328725