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Radiative transfer and negative ion of hydrogen by Subrahmanyan Chandrasekhar

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Published by University of Chicago Press in Chicago .
Written in English


  • Stars -- Atmospheres.,
  • Radiative transfer.,
  • Hydrogen ions.,
  • Anions.

Book details:

Edition Notes

Includes bibliographical references.

StatementS. Chandrasekhar.
SeriesSelected papers ;, v. 2
LC ClassificationsQB809 .C47 1989
The Physical Object
Paginationxvi, 622 p. :
Number of Pages622
ID Numbers
Open LibraryOL2048801M
ISBN 100226100928, 0226100936
LC Control Number88026111

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Contents: Part I. Radiative transfer. 1. The method of discrete ordinates. 2. Radiative transfer allowing for polarization of scattering light. 3. Principles of invariance: the H- and the X- and Y-functions. 4. Miscellaneous problems. 5. Review articles. Part II. Investigation on the negative ion of hydrogen and of two-electron : S. Chandrasekhar. Not Available Book-Review - Selected Papers - V.2 - Radiative Transfer and Negative Ion of HydrogenAuthor: S. Chandrasekhar. Radiative transfer on discrete spaces, (International series of monographs in pure and applied mathematics) by Rudolph W Preisendorfer and a great selection of related books, art and collectibles available now at   We survey the results of a long-term study of the process of radiative recombination (RR). A rigorous theory of non-relativistic electron RR with a hydrogen-like ion is used to calculate the total cross section of the process, the effective radiation, the recombination rate coefficient, and the emission coefficient in a plasma with a Maxwellian electron by: 1.

Selected Papers. Vol. 2: Radiative Transfer and Negative Ion of Hydrogen by S Chandrasekhar The University of Chicago Press: Chicago, USA, pages; price: US 60 (Paper); ISBN The equation of radiative transfer governs the transport of radiant energy in a. If the address matches an existing account you will receive an email with instructions to reset your password. Chandrasekhar Polarization is a partial polarization of emergent radiation at the limb of rapidly rotating early-type stars or binary star system with purely electron-scattering atmosphere, named after the Indian American astrophysicist Subrahmanyan Chandrasekhar, who first predicted its existence theoretically in Chandrasekhar published a series of 26 papers in The Astrophysical. Negative ion enhancement in caesium-seeded hydrogen discharges—a volume or surface effect? Appl. Phys. Lett. 75, (); / Hydrogen negative ion production in an electron.

@article{osti_, title = {Collisions of electrons with atoms and molecules}, author = {Drukarev, G F}, abstractNote = {This book is a short outline of the present state of the theory of electron collisions with atomic particles - atoms, molecules and ions. It is addressed to those who need detailed information about the cross sections of various processes of electron collisions with. The radiative transfer code requires the ionizing luminosity of the radiative source to be expressed in photons per second. We make the conversion, assuming that each photon deposits 20 eV, so if the total ionizing luminosity is Lstar (W), then the quantity passed to the radiative transfer code is Lstar/( ), or × 10 46 photon s. Plan Radiative transfer and how it stood ca. A numerical scheme and some analytical fallout The principles of invariance Blue sky research - polarisation The negative ion of . Numerical Radiative Transfer and the Hydrogen Reionization of the Universe Margarita Borisova Petkova Dissertation an der Fakult¨at fur Physik der Ludwig–Maximilians–Universit¨at Munchen vorgelegt von Margarita Borisova Petkova aus Sofia, Bulgarien Munchen, den Januar,