Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.stsci.edu/~kgordon/Dust/Scat_Param/scat_data_dgl.html
Äàòà èçìåíåíèÿ: Tue Nov 28 20:01:01 2006
Äàòà èíäåêñèðîâàíèÿ: Tue May 27 07:51:35 2008
Êîäèðîâêà:
Ïîèñêîâûå ñëîâà: ï ï ï ï ï ï

Determinations of Dust Scattering Properties from Diffuse Galactic Light (DGL)

Interstellar Dust Scattering Properties from Diffuse Galactic Light (DGL)

From K. D. Gordon 2004, in "Astrophysics of Dust", (ASP Conf. Proceed. 196), ed. A. N. Witt, G. C. Clayton, & B. T. Draine, (ASP: San Francisco), 77

Updated: KDG - 28 Nov 2006

Single Scattering Albedo a	Scattering Phase Function Asymmetry g = < cos(α) >
DGL Plots

ASCII file of plotted data

Reference	Description	Model Type	In Plot	Comment
DGL Studies
Witt 1968	3600, 4350, & 6100 Å		No	Superseded by Mathis 1973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Witt & Lillie 1973	OAO-2 1500 - 4200 Å	DGL3	No	Superseded by Lillie & Witt 1976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Hurwitz et al. 1991	Berkeley UVX 1625 Å	DGL5	No	Superseded by Murthy & Henry 1995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Sasseen & Deharveng 1996	FAUST 1565 Å	DGL7	No	Superseded by Witt et al. 1997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

Name	Description
Radiative Transfer Models
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

References

Interstellar dust scattering properties from: [Diffuse Galactic Light] [Reflection Nebulae] [Dark Clouds]