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Дата изменения: Tue Nov 28 20:01:01 2006 Дата индексирования: Tue May 27 07:51:35 2008 Кодировка: Поисковые слова: р п р п |
DGL Plots | |
Single Scattering Albedo a |
Scattering Phase Function Asymmetry g = < cos(α) > |
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ASCII file of plotted data |
DGL Studies | ||||
Reference | Description | Model Type | In Plot | Comment |
---|---|---|---|---|
Witt 1968 | 3600, 4350, & 6100 Å | No | Superseded by Mathis 1973 | |
Mathis 1973 | 3600 & 4350 Å | DGL2 | Yes | No g determination possible |
Witt & Lillie 1973 | OAO-2 1500 - 4200 Å | DGL3 | No | Superseded by Lillie & Witt 1976 |
Lillie & Witt 1976 | OAO-2 1500 - 4200 Å | DGL2 | Yes | |
Morgan et al. 1976 | TD-1 2350 & 2740 Å | DGL3 | Yes | No g determination possible |
Toller 1981 | Pioneer 10 4400 Å | DGL4 | Yes | |
Hurwitz et al. 1991 | Berkeley UVX 1625 Å | DGL5 | No | Superseded by Murthy & Henry 1995 |
Murthy et al. 1993 | Voyager 2 1050 Aring; | DGL6 | Yes | No g determination possible |
Murthy & Henry 1995 | Berkely UVX + others | DGL6 | Yes | No g determination possible |
Sasseen & Deharveng 1996 | FAUST 1565 Å | DGL7 | No | Superseded by Witt et al. 1997 |
Petersohn 1997 | DE 1 1565 Å | DGL8 | Yes | |
Witt et al. 1997 | FAUST 1565 Å | DGL8 | Yes | |
Schiminovich et al. 2001 | NUVIEWS 1740 Å | DGL9 | Yes | |
Shalima & Murthy | Voyager 1250 Å | DGL10 | Yes | No g determination possible |
Sujatha et al. | Voyager 1100 Å | DGL10 | Yes |
Radiative Transfer Models | ||
Name | Description | |
---|---|---|
DGL1 | analytic; Galaxy model; homogeneous slab | |
DGL2 | numerical int. (n=8 scatterings); MW ISRF boundary condition; infinite cylinder | |
DGL3 | analytic; constant; ininite slab | |
DGL4 | numerical int. (n=2 scatterings); star counts; non-homogeneous | |
DGL5 | numerical int.; TD-1 star catalog; clumped dust | |
DGL6 | numerical int.; SKYMAP catalog; dust based on HI survey | |
DGL7 | Monte Carlo; star catalogs; dust based on HI survey | |
DGL8 | Monte Carlo; TD-1 star catalog; dust cloud spectrum based on HI survery | |
DGL9 | Monte Carlo; 3D TD-1 star catalog; dust cloud spectrum based on HI survery | |
DGL10 | Monte Carlo; 3D Hipparcos star catalog; dust cloud based on HI survery |
Interstellar dust scattering properties from: [Diffuse Galactic Light] [Reflection Nebulae] [Dark Clouds]
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