Characteristics of the Re-Calculated Yohkoh/SXT Temperature Response
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-011-9838-y.pdf
Reference18 articles.
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3. Dere, K.P., Landi, E., Young, P.R., Del Zanna, G.: 2001, CHIANTI – An atomic database for emission lines. IV. Extension to X-ray wavelengths. Astrophys. J. Suppl. 134, 331 – 354. doi: 10.1086/320854 .
4. Dere, K.P., Landi, E., Young, P.R., Del Zanna, G., Landini, M., Mason, H.E.: 2009, CHIANTI – An atomic database for emission lines. IX. Ionization rates, recombination rates, ionization equilibria for the elements hydrogen through zinc and updated atomic data. Astron. Astrophys. 498, 915 – 929. doi: 10.1051/0004-6361/200911712 .
5. Feldman, U., Widing, K.G.: 2002, A review of the first ionization potential effect on elemental abundances in the solar corona and in flares. Phys. Plasmas 9, 629 – 635. doi: 10.1063/1.1435000 .
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