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7Â¥2008-12-25 15:16:01
qingmei7505
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2Â¥2008-11-27 13:16:50
СÁúÈË
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![]() http://www.pa.uky.edu/~peter/atomic/ ÕâÊÇÒ»¸ö²»´íµÄÍøÕ¾£¬ÓÐÔ×Ó¹âÆ×Êý¾Ý¡£ This is a compilation of approximately 923,000 allowed, intercombination and forbidden atomic transitions with wavelengths in the range from 0.5 Å to 1000 µm. It's primary intention is to allow the identification of observed atomic absorption or emission features. The wavelengths in this list are all calculated from the difference between the energy of the upper and lower level of the transition. No attempt has been made to include observed wavelengths. Most of the atomic energy level data have been taken from the Atomic Spectra Database provided by the National Institute of Standards and Technology (NIST). When attempting to identify an observed line usually many possible candidates can be found in this list. In order to facilitate narrowing down the number of possible identifications a selection tool is presented which allows imposing, apart from the wavelength, several additional criteria. The following documentation is available: Instructions for querying the line list. Documentation on how this line list was compiled. Copyright Notice/Disclaimer. Please note that publication of this line list, or any large part of it, is only allowed with permission of the author. Please acknowledge use of the Atomic Line List (including the URL) in each paper that contains data from this list. The author kindly thanks the following persons (in alphabetical order) who supplied data compiled in this list: M.A. Bautista, S.N. Nahar, M.J. Seaton, D.A. Verner. Recent Developments The line data for C II, III and IV have been extended. The line data for chlorine and argon is complete now. The transition probabilities for Ne I calculated by Seaton have been included. Transition probabilities calculated using the Coulomb approximation have been added for the helium, lithium, sodium and potassium iso-electronic sequences. The Atomic Line List is hosted by the Department of Physics and Astronomy University of Kentucky and is maintained by Peter van Hoof Royal Observatory of Belgium Ringlaan 3 1180 Brussel Belgium [ Last edited by СÁúÈË on 2008-11-27 at 13:42 ] |

3Â¥2008-11-27 13:41:28
СÁúÈË
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4Â¥2008-11-27 13:41:54














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