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140122 ||| eng |
| 020 |
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|a 9780387348308
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| 100 |
1 |
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|a Smith, Peter L.
|e [editor]
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| 245 |
0 |
0 |
|a Atomic and Molecular Data for Space Astronomy
|h Elektronische Ressource
|b Needs, Analysis, and Availabilty
|c edited by Peter L. Smith, Wolfgang L. Wiese
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| 250 |
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|a 1st ed. 1992
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| 260 |
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|a New York, NY
|b Springer New York
|c 1992, 1992
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| 300 |
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|a VII, 160 p
|b online resource
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| 505 |
0 |
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|a Atomic and molecular data for space astronomy: Needs and availability -- The hubble space telescope — Scientific problems and laboratory data needs -- Atomic data needed for far ultraviolet astronomy with HUT and FUSE -- Atomic data needed for analysis of EUV and X-Ray spectra -- Atomic and molecular data for observations of the interstellar medium with the hubble space telescope -- Atomic and molecular data needed for analysis of infrared spectra from ISO and SIRTF -- Atomic data from the opacity project -- Sources of atomic spectroscopic data for astrophysics -- Summary of current molecular databases
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| 653 |
|
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|a Atoms
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| 653 |
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|a Atomic, Molecular and Chemical Physics
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| 653 |
|
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|a Geophysics
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| 653 |
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|a Astronomy / Observations
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| 653 |
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|a Astronomy, Observations and Techniques
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| 653 |
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|a Astrophysics
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| 653 |
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|a Molecules
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| 700 |
1 |
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|a Wiese, Wolfgang L.
|e [editor]
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| 041 |
0 |
7 |
|a eng
|2 ISO 639-2
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| 989 |
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|b SBA
|a Springer Book Archives -2004
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| 490 |
0 |
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|a Lecture Notes in Physics
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| 028 |
5 |
0 |
|a 10.1007/BFb0040307
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| 856 |
4 |
0 |
|u https://doi.org/10.1007/BFb0040307?nosfx=y
|x Verlag
|3 Volltext
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| 082 |
0 |
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|a 520
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| 520 |
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|a This is a very useful reference book for working astronomers and astrophysicists. Forming the proceedings of a recent IAU meeting where the availability and the needs of atomic and molecular data were discussed, the papers published here discuss existing and planned instruments for astronomical spectroscopy from earth-orbiting satellites. In particular, the atomic and molecular parameters that are, or will be, needed for analysis of the data obtained by these instruments are considered. A number of significant shortcomings in the available databases are identified. The needs highlighted will be of interest to laboratory astrophysicists, both experimentalists and theorists, who canproduce the data required. A second group of papers provides a current inventory of atomic and molecular data compilations
|