Radiative transfer in moving spherical atmospheres: II. analytical solution for fully relativistic radial motions.
Based on the well known solution of the time-independent radiative transfer equation along a ray and on suitable point transformations, general quadrature solutions of the monochromatic transfer equation for plane-parallel, spherically-symmetric and arbitrarily shaped 3D configurations with differen...
Gespeichert in:
| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
1997
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| In: |
Astronomy and astrophysics
Year: 1997, Jahrgang: 317, Pages: 630-635 |
| ISSN: | 1432-0746 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://ui.adsabs.harvard.edu/abs/1997A&A...317..630B
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| Verfasserangaben: | B. Baschek, G.V. Efimov, W. von Waldenfels, R. Wehrse |
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| 245 | 1 | 0 | |a Radiative transfer in moving spherical atmospheres |b II. analytical solution for fully relativistic radial motions. |c B. Baschek, G.V. Efimov, W. von Waldenfels, R. Wehrse |
| 264 | 1 | |c 1997 | |
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| 520 | |a Based on the well known solution of the time-independent radiative transfer equation along a ray and on suitable point transformations, general quadrature solutions of the monochromatic transfer equation for plane-parallel, spherically-symmetric and arbitrarily shaped 3D configurations with differential motion are derived for the observer's and the comoving frame. The source function is assumed to be given; however, the scattering case requires only a simple iteration in addition. Since complete Lorentz transformations are used, the velocities are not restricted. It is shown that in many cases the explicit form of the transfer equation - which often is quite complicated - is not required for the determination of the specific intensities. | ||
| 650 | 4 | |a METHODS: ANALYTICAL | |
| 650 | 4 | |a RADIATIVE TRANSFER | |
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