Idioma: Inglés
Publicado por Universität Heidelberg, 1974
Librería: books4less (Versandantiquariat Petra Gros GmbH & Co. KG), Welling, Alemania
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Añadir al carritoBroschiert; Condición: Gut. ca. 80 Seiten; Die hier angebotene Broschüre stammt aus einer teilaufgelösten Bibliothek und trägt die entsprechenden Kennzeichnungen (Vermerke, Stempel.). Einband etwas staubschmutzig; ansonsten ordentlicher Erhaltungszustand. Sprache: Englisch Gewicht in Gramm: 120.
Librería: Antiquariat Bookfarm, Löbnitz, Alemania
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Añadir al carrito109 S. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. Ex-library with stamp and library-signature. GOOD condition, some traces of use. 3540523650 Sprache: Englisch Gewicht in Gramm: 900.
Librería: Antiquariat Bookfarm, Löbnitz, Alemania
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Añadir al carritoHardcover. Ex-library in GOOD condition with library-signature and stamp(s). Some traces of use. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. C-00611 3540523650 Sprache: Englisch Gewicht in Gramm: 550.
Librería: Romtrade Corp., STERLING HEIGHTS, MI, Estados Unidos de America
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Idioma: Inglés
Publicado por Berlin ; Heidelberg ; New York ; London ; Paris ; Tokyo ; Hong Kong : Springer,, 1990
ISBN 10: 3540523650 ISBN 13: 9783540523659
Librería: Die Wortfreunde - Antiquariat Wirthwein Matthias Wirthwein, Mannheim, Alemania
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Añadir al carritoOPp, gebundene Ausgabe. 109 S. : graph. Darst. ; 25 cm Fast neuwertiges, ungelesenes Exemplar. Sprache: Englisch Gewicht in Gramm: 333.
Librería: Ria Christie Collections, Uxbridge, Reino Unido
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Añadir al carritoCondición: New. pp. 116.
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Añadir al carritoPaperback. Condición: Brand New. 116 pages. 9.70x6.70x0.40 inches. In Stock.
Librería: Biblios, Frankfurt am main, HESSE, Alemania
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Añadir al carritoCondición: Sehr gut. Zustand: Sehr gut | Sprache: Englisch | Produktart: Bücher | Keine Beschreibung verfügbar.
Idioma: Inglés
Publicado por Springer Berlin Heidelberg, 2014
ISBN 10: 366213781X ISBN 13: 9783662137819
Librería: AHA-BUCH GmbH, Einbeck, Alemania
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Añadir al carritoTaschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - To get a reasonably realistic picture of the structure and evolution of stars one needs to know accurately the abundances of chemical elements and their isotopes in the stellar atmosphere and in the galactic environment of the stars. The articles collected in this volume give a modern review of the abundance accuracies for main-sequence stars. After a general introduction in the first part the accuracies of atomic transition probabilities, ionization and excitation cross-sections, and line broad- ening data are discussed. In the second part the specific problems and results for different stellar types are presented, and, finally, an overview on the possibilities of abundance determinations for stars outside the Galaxy is given.
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Añadir al carritoCondición: Sehr gut. Zustand: Sehr gut | Seiten: 320 | Sprache: Englisch | Produktart: Bücher | Traditionally, radiative transfer has been the domain of astrophysicists and climatologists. In nuclear technology one has been dealing with the ana- gous equations of neutron transport. In recent years, applications of radiative transferincombustionmachinedesignandinmedicinebecamemoreandmore important. In all these disciplines one uses the radiative transfer equation to model the formation of the radiation ?eld and its propagation. For slabs and spheres e?ective algorithms for the solution of the transfer equation have been ava- able for quite some time. In addition, the analysis of the equation is quite well developed. Unfortunately, in many modern applications the approximation of a 1D geometry is no longer adequate and one has to consider the full 3D dependencies. This makes the modeling immensely more intricate. The main reasons for the di?culties result from the fact that not only the dimension of the geometric space has to be increased but one also has to employ two angle variables (instead of one) and very often one has to consider frequency coupling (due to motion or redistribution in spectral lines). In actual cal- lations this leads to extremely large matrices which, in addition, are usually badly conditioned and therefore require special care. Analytical solutions are not available except for very special cases. Although radiative transfer problems are interesting also from a ma- ematical point of view, mathematicians have largely neglected the transfer equation for a long time.
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Añadir al carritoCondición: New. pp. 320.
Idioma: Inglés
Publicado por Springer, Springer Spektrum, 2008
ISBN 10: 3540853685 ISBN 13: 9783540853688
Librería: AHA-BUCH GmbH, Einbeck, Alemania
EUR 192,59
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Añadir al carritoTaschenbuch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - Traditionally, radiative transfer has been the domain of astrophysicists and climatologists. In nuclear technology one has been dealing with the ana- gous equations of neutron transport. In recent years, applications of radiative transferincombustionmachinedesignandinmedicinebecamemoreandmore important. In all these disciplines one uses the radiative transfer equation to model the formation of the radiation eld and its propagation. For slabs and spheres e ective algorithms for the solution of the transfer equation have been ava- able for quite some time. In addition, the analysis of the equation is quite well developed. Unfortunately, in many modern applications the approximation of a 1D geometry is no longer adequate and one has to consider the full 3D dependencies. This makes the modeling immensely more intricate. The main reasons for the di culties result from the fact that not only the dimension of the geometric space has to be increased but one also has to employ two angle variables (instead of one) and very often one has to consider frequency coupling (due to motion or redistribution in spectral lines). In actual cal- lations this leads to extremely large matrices which, in addition, are usually badly conditioned and therefore require special care. Analytical solutions are not available except for very special cases. Although radiative transfer problems are interesting also from a ma- ematical point of view, mathematicians have largely neglected the transfer equation for a long time.
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Añadir al carritoPaperback. Condición: Brand New. 1st edition. 309 pages. 9.00x6.00x0.75 inches. In Stock.
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Añadir al carritohardcover. Condición: Gut. 114 Seiten; Artikel stammt aus Nichtraucherhaushalt! V19112 Sprache: Deutsch Gewicht in Gramm: 500.
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Idioma: Inglés
Publicado por Springer, Springer Berlin Heidelberg Aug 2014, 2014
ISBN 10: 366213781X ISBN 13: 9783662137819
Librería: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Alemania
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Añadir al carritoTaschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -To get a reasonably realistic picture of the structure and evolution of stars one needs to know accurately the abundances of chemical elements and their isotopes in the stellar atmosphere and in the galactic environment of the stars. The articles collected in this volume give a modern review of the abundance accuracies for main-sequence stars. After a general introduction in the first part the accuracies of atomic transition probabilities, ionization and excitation cross-sections, and line broad- ening data are discussed. In the second part the specific problems and results for different stellar types are presented, and, finally, an overview on the possibilities of abundance determinations for stars outside the Galaxy is given. 116 pp. Englisch.
Librería: Majestic Books, Hounslow, Reino Unido
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Añadir al carritoCondición: New. Print on Demand pp. 116 67:B&W 6.69 x 9.61 in or 244 x 170 mm (Pinched Crown) Perfect Bound on White w/Gloss Lam.
Librería: Biblios, Frankfurt am main, HESSE, Alemania
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Añadir al carritoCondición: New. PRINT ON DEMAND pp. 116.
Idioma: Inglés
Publicado por Springer, Springer Aug 2014, 2014
ISBN 10: 366213781X ISBN 13: 9783662137819
Librería: buchversandmimpf2000, Emtmannsberg, BAYE, Alemania
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Añadir al carritoTaschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The articles collected in this volume give a modern review on the abundance accuracies for main-sequence stars. After a general introduction in the first part the accuracies of atomic transition probabilities, ionization and excitation cross-sections, and line broadening data are discussed. In the second part the specific problems and results for different stellar types are presented, and, finally, an overview on the possibilities of abundance determinations for stars outside the Galaxy is given.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 116 pp. Englisch.
Librería: Brook Bookstore On Demand, Napoli, NA, Italia
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Añadir al carritoCondición: new. Questo è un articolo print on demand.
Idioma: Inglés
Publicado por Springer Berlin Heidelberg, 2008
ISBN 10: 3540853685 ISBN 13: 9783540853688
Librería: moluna, Greven, Alemania
EUR 162,51
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Añadir al carritoKartoniert / Broschiert. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Traditionally, radiative transfer has been the domain of astrophysicists and climatologists. In nuclear technology one has been dealing with the ana- gous equations of neutron transport. In recent years, applications of radiative transferincombustionmachine.
Idioma: Inglés
Publicado por Springer Berlin Heidelberg Dez 2008, 2008
ISBN 10: 3540853685 ISBN 13: 9783540853688
Librería: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Alemania
EUR 192,59
Cantidad disponible: 2 disponibles
Añadir al carritoTaschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Traditionally, radiative transfer has been the domain of astrophysicists and climatologists. In nuclear technology one has been dealing with the ana- gous equations of neutron transport. In recent years, applications of radiative transferincombustionmachinedesignandinmedicinebecamemoreandmo re important. In all these disciplines one uses the radiative transfer equation to model the formation of the radiation eld and its propagation. For slabs and spheres e ective algorithms for the solution of the transfer equation have been ava- able for quite some time. In addition, the analysis of the equation is quite well developed. Unfortunately, in many modern applications the approximation of a 1D geometry is no longer adequate and one has to consider the full 3D dependencies. This makes the modeling immensely more intricate. The main reasons for the di culties result from the fact that not only the dimension of the geometric space has to be increased but one also has to employ two angle variables (instead of one) and very often one has to consider frequency coupling (due to motion or redistribution in spectral lines). In actual cal- lations this leads to extremely large matrices which, in addition, are usually badly conditioned and therefore require special care. Analytical solutions are not available except for very special cases. Although radiative transfer problems are interesting also from a ma- ematical point of view, mathematicians have largely neglected the transfer equation for a long time. 320 pp. Englisch.