Astron. Astrophys. Suppl. Ser.
Volume 142, Number 1, February II 2000
|Page(s)||95 - 106|
|Published online||15 February 2000|
Laboratory observation and modeling of extreme ultraviolet spectra of highly ionized calcium
Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland 21218, U.S.A.
2 2714 Fairview Ave. E. # 101, Seattle, Washington 98102, U.S.A.
3 Permanent address: Racah Institute of Physics, The Hebrew University, Jerusalem, Israel
4 Lawrence Livermore National Laboratories, P.O. Box 808, Livermore, California 94550, U.S.A.
5 Associazione EURATOM-ENEA sulla Fusione, C.R. Frascati, CP 65-00044 Frascati Roma, Italy
Send offprint request to: V.A. Soukhanovskii
Accepted: 23 November 1999
Benchmarking and validation of atomic calculations are crucial for understanding the properties of astrophysical and fusion plasmas. An extended re-evaluation of a previous experimental study of the CaXVIII – CaXII extreme ultraviolet (XUV) spectra is presented. CaF2 was introduced into tokamak plasmas and the spectra of the calcium ions were recorded by a photometrically calibrated grazing incidence time-resolved spectrometer. The local plasma electron temperature and density were measured independently. Nearly all features of the line-of-sight integrated spectra were identified. Atomic data for this work were generated ab initio with the HULLAC suite of codes. The results of collisional-radiative (CR) modeling for individual charge states agree with the measured spectral line intensities within the experimental accuracy for most lines, thus validating the electron temperature and density diagnostic potential of the L-shell lines. In addition, we compare experimentally measured and calculated line intensities with those calculated using the CHIANTI database.
Key words: atomic processes, Sun: UV radiation, Sun: flares
© European Southern Observatory (ESO), 2000