Titlebook: Radiation Transport in Spectral Lines; R. Grant Athay Book 1972 D. Reidel Publishing Company, Dordrecht, Holland 1972 atmosphere.star.turb

frozen-shoulder

Introduction, been written on the subject. The field has by no means been exhausted, however. Major new techniques for handling transport problems are being developed, and, with them, new concepts of radiation processes are emerging.

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周年纪念日

Introduction,gaseous media. The physics of radiation and the phenomena of radiative transport of energy have been extensively studied and many excellent books have been written on the subject. The field has by no means been exhausted, however. Major new techniques for handling transport problems are being develo

Diluge

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Total Intensities of Lines,ation concerning the shape of the line. This is particularly true for stellar spectra and for present data for the solar XUV spectrum. It is useful in these situations to seek methods for relating the total energy, or equivalent width, of a spectral line to the thermodynamic and chemical properties

Dignant

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Numerical Methods,uch techniques is beyond the purpose and scope of this text. Instead a few selected methods will be discussed in broad outline. The particular methods selected for discussion are illustrative of those that are more commonly used. For the detailed application of a particular method and for informatio

aptitude

thods of obtaining analytical solutions for special cases, and of the physics of line broadening. Neither of those features will be found in this book. It is assumed that the reader is already familiar with the essentials of transport theory and of line broadening and is ready to investi­ gate some