| 000 | 02658nam a22004455i 4500 | ||
|---|---|---|---|
| 001 | 978-1-4614-8797-5 | ||
| 003 | DE-He213 | ||
| 005 | 20140220082503.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 140102s2014 xxu| s |||| 0|eng d | ||
| 020 |
_a9781461487975 _9978-1-4614-8797-5 |
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| 024 | 7 |
_a10.1007/978-1-4614-8797-5 _2doi |
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| 050 | 4 | _aQB4 | |
| 072 | 7 |
_aPG _2bicssc |
|
| 072 | 7 |
_aSCI004000 _2bisacsh |
|
| 072 | 7 |
_aNAT033000 _2bisacsh |
|
| 082 | 0 | 4 |
_a520 _223 |
| 100 | 1 |
_aHuebner, Walter F. _eauthor. |
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| 245 | 1 | 0 |
_aOpacity _h[electronic resource] / _cby Walter F. Huebner, W. David Barfield. |
| 264 | 1 |
_aNew York, NY : _bSpringer New York : _bImprint: Springer, _c2014. |
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| 300 |
_aXVIII, 572 p. 98 illus., 1 illus. in color. _bonline resource. |
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| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
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| 338 |
_aonline resource _bcr _2rdacarrier |
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| 347 |
_atext file _bPDF _2rda |
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| 490 | 1 |
_aAstrophysics and Space Science Library, _x0067-0057 ; _v402 |
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| 505 | 0 | _aDefinitions -- Atomic and Molecular Structure -- Equation of State -- Radiative Cross Sections -- Continuum transitions -- Bound-Bound Transitions -- Electron Conduction -- Equations of State and Opacities for Mixtures -- Limits, Approximations, Scaling, and Interpolation -- Uncertainties in Models, Methods, and Calculations. | |
| 520 | _aThe interaction of radiation with matter is a fundamental process in the universe; in particular, the absorption and scattering of radiation by matter (the opacity) govern the formation, evolution, and structure of stars and planets. But opacity is also important in many terrestrial applications in which radiation is the dominant means of energy transfer, such as controlled nuclear-fusion, laser ablation, atmospheric entry and reentry, and the "greenhouse" effect. This book covers all aspects of opacity and equations of state for plasmas, gases, vapors, and dust and emphasizes the continuous transformation of phases and molecular compositions with changing density and temperature under conditions of local thermodynamic equilibrium (LTE) while preserving the basic abundances of the chemical elements in a mixture. | ||
| 650 | 0 | _aPhysics. | |
| 650 | 1 | 4 | _aPhysics. |
| 650 | 2 | 4 | _aAstronomy, Observations and Techniques. |
| 700 | 1 |
_aBarfield, W. David. _eauthor. |
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| 710 | 2 | _aSpringerLink (Online service) | |
| 773 | 0 | _tSpringer eBooks | |
| 776 | 0 | 8 |
_iPrinted edition: _z9781461487968 |
| 830 | 0 |
_aAstrophysics and Space Science Library, _x0067-0057 ; _v402 |
|
| 856 | 4 | 0 | _uhttp://dx.doi.org/10.1007/978-1-4614-8797-5 |
| 912 | _aZDB-2-PHA | ||
| 999 |
_c92249 _d92249 |
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