Numerical Radiative Transfer
Herausgeber: Kalkofen, Wolfgang
Numerical Radiative Transfer
Herausgeber: Kalkofen, Wolfgang
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First published in 1987, this book is a manual of methods for solving problems in radiative transfer.
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First published in 1987, this book is a manual of methods for solving problems in radiative transfer.
Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Produktdetails
- Produktdetails
- Verlag: Cambridge University Press
- Seitenzahl: 384
- Erscheinungstermin: 28. Februar 2009
- Englisch
- Abmessung: 244mm x 170mm x 21mm
- Gewicht: 661g
- ISBN-13: 9780521115179
- ISBN-10: 0521115175
- Artikelnr.: 26183870
- Verlag: Cambridge University Press
- Seitenzahl: 384
- Erscheinungstermin: 28. Februar 2009
- Englisch
- Abmessung: 244mm x 170mm x 21mm
- Gewicht: 661g
- ISBN-13: 9780521115179
- ISBN-10: 0521115175
- Artikelnr.: 26183870
Preface; Introduction; Part I. Operator Perturbation: 1. Survey of operator
perturbation methods W. Kalkofen; 2. Line formation in expanding
atmospheres: multilevel calculations using approximate lambda operators W.
R. Hamann; 3. Stellar atmospheres in non-LTE: model construction and line
formation calculations using approximate lambda operators K. Werner; 4.
Acceleration of convergence L. H. Auer; 5. Line formation in a
time-dependent atmosphere W. Kalkofen; 6. Iterative solution of multilevel
transfer problems Eugene H. Avrett and Rudolf Loeser; 7. An algorithm for
the simultaneous solution of thousands of transfer equations under global
constraints Lawrence S. Anderson; 8. Operator perturbation for differential
equations W. Kalkofen; Part II. Polarised Radiation: 9. A gentle
introduction to polarised radiative transfer David E. Rees; 10. Non-LTE
polarised radiative transfer in special lines David E. Rees and Graham A.
Murphy; 11. Transfer of polarised radiation using 4x4 matrices E. Landi
Degli'Innocenti; 12. Radiative transfer in the presence of strong magnetic
fields A. A. van Ballegooijen; 13. An integral operator technique of
radiative transfer in spherical symmetry A. Peraiah; 14. Discrete ordinate
matrix method M. Schmidt and R. Wehrse.
perturbation methods W. Kalkofen; 2. Line formation in expanding
atmospheres: multilevel calculations using approximate lambda operators W.
R. Hamann; 3. Stellar atmospheres in non-LTE: model construction and line
formation calculations using approximate lambda operators K. Werner; 4.
Acceleration of convergence L. H. Auer; 5. Line formation in a
time-dependent atmosphere W. Kalkofen; 6. Iterative solution of multilevel
transfer problems Eugene H. Avrett and Rudolf Loeser; 7. An algorithm for
the simultaneous solution of thousands of transfer equations under global
constraints Lawrence S. Anderson; 8. Operator perturbation for differential
equations W. Kalkofen; Part II. Polarised Radiation: 9. A gentle
introduction to polarised radiative transfer David E. Rees; 10. Non-LTE
polarised radiative transfer in special lines David E. Rees and Graham A.
Murphy; 11. Transfer of polarised radiation using 4x4 matrices E. Landi
Degli'Innocenti; 12. Radiative transfer in the presence of strong magnetic
fields A. A. van Ballegooijen; 13. An integral operator technique of
radiative transfer in spherical symmetry A. Peraiah; 14. Discrete ordinate
matrix method M. Schmidt and R. Wehrse.
Preface; Introduction; Part I. Operator Perturbation: 1. Survey of operator
perturbation methods W. Kalkofen; 2. Line formation in expanding
atmospheres: multilevel calculations using approximate lambda operators W.
R. Hamann; 3. Stellar atmospheres in non-LTE: model construction and line
formation calculations using approximate lambda operators K. Werner; 4.
Acceleration of convergence L. H. Auer; 5. Line formation in a
time-dependent atmosphere W. Kalkofen; 6. Iterative solution of multilevel
transfer problems Eugene H. Avrett and Rudolf Loeser; 7. An algorithm for
the simultaneous solution of thousands of transfer equations under global
constraints Lawrence S. Anderson; 8. Operator perturbation for differential
equations W. Kalkofen; Part II. Polarised Radiation: 9. A gentle
introduction to polarised radiative transfer David E. Rees; 10. Non-LTE
polarised radiative transfer in special lines David E. Rees and Graham A.
Murphy; 11. Transfer of polarised radiation using 4x4 matrices E. Landi
Degli'Innocenti; 12. Radiative transfer in the presence of strong magnetic
fields A. A. van Ballegooijen; 13. An integral operator technique of
radiative transfer in spherical symmetry A. Peraiah; 14. Discrete ordinate
matrix method M. Schmidt and R. Wehrse.
perturbation methods W. Kalkofen; 2. Line formation in expanding
atmospheres: multilevel calculations using approximate lambda operators W.
R. Hamann; 3. Stellar atmospheres in non-LTE: model construction and line
formation calculations using approximate lambda operators K. Werner; 4.
Acceleration of convergence L. H. Auer; 5. Line formation in a
time-dependent atmosphere W. Kalkofen; 6. Iterative solution of multilevel
transfer problems Eugene H. Avrett and Rudolf Loeser; 7. An algorithm for
the simultaneous solution of thousands of transfer equations under global
constraints Lawrence S. Anderson; 8. Operator perturbation for differential
equations W. Kalkofen; Part II. Polarised Radiation: 9. A gentle
introduction to polarised radiative transfer David E. Rees; 10. Non-LTE
polarised radiative transfer in special lines David E. Rees and Graham A.
Murphy; 11. Transfer of polarised radiation using 4x4 matrices E. Landi
Degli'Innocenti; 12. Radiative transfer in the presence of strong magnetic
fields A. A. van Ballegooijen; 13. An integral operator technique of
radiative transfer in spherical symmetry A. Peraiah; 14. Discrete ordinate
matrix method M. Schmidt and R. Wehrse.