The influence of the brightness of the asteroidal dust bands on the Gegenschein

Icarus

Volumn 162, Issue 2, 2003, Pages 337-343

  Mukai, Tadashi ^a   Fujino, Masanori ^a   Ishiguro, Masateru ^b   Nakamura, Ryosuke ^c   Ueno, Munetaka ^d   Usui, Fumihiko ^d   Kwon, Suk Minn ^e  

^a KOBE UNIVERSITY   (Japan)

^b JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^c JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^d UNIVERSITY OF TOKYO   (Japan)

^e Kangwon National University   (South Korea)

Author keywords

Asteroids; Dust bands; Gegenschein; Zodiacal light

Indexed keywords

EID: 0037609668     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0019-1035(03)00003-4     Document Type: Article

References (15)

1. Giese, R.H., Kneissel, B., Rittich, U., 1986. Three-dimensional models of the zodiacal dust cloud: a comparative study. Icarus 68, 395-411.
2. Hong, S.S., 1985. Henyey-Greenstein representation of the mean volume scattering phase function for zodiacal dust. Astron. Astrophys. 146, 67-75.
3. Ishiguro, M., Fukushima, H., Kinoshita, D., Mukai, T., Nakamura, R., Watanabe, J., Watanabe, T., James, J.F., 1998. The isophote maps of the Gegenschein obtained by CCD observations. Earth Planets Space 50, 477-480.
4. Ishiguro, M., Nakamura, R., Fujii, Y., Mukai, T., 1999a. Comparative studies of visible and IRAS interplanetary dust bands. Publ. Astron. Soc. Japan 51, 363-366.
5. Ishiguro, M., Nakamura, R., Fujii, Y., Morishige, K., Yano, H., Yasuda, H., Yokogawa, S., Mukai, T., 1999b. First detection of visible zodiacal dust bands from ground-based observations. Astrophys J. 511, 432-435.
6. James, J.F., Mukai, T., Watanabe, T., Ishiguro, M., Nakamura, R., 1997. The morphology and brightness of the zodiacal light and Gegenschein. Mon. Not. R. Astron. Soc. 288, 1022-1026.
7. Jones, M.H., Rowan-Robinson, M., 1993. A physical model for the IRAS zodiacal dust bands. Mon. Not. R. Astron. Soc. 264, 237-247.
8. Kelsall, T., Weiland, J.L., Franz, B.A., Reach, W.T., Arendt, R.G., Dwek, E., Freudenreich, H.T., Hauser, M.G., Moseley, S.H., Odegard, N.P., Silverberg, R.F., Wright, E.L., 1998. The COBE diffuse background experiment search for the cosmic infrared background. II. Model of the interplanetary dust cloud. Astrophys. J. 508, 44-73.
9. Leinert, Ch., 1975. Zodiacal light - a measure of the interplanetary environment. Space Sci. Rev. 18, 281-339.
10. Leinert, Ch., Bowyer, S., Haikala, L.K., Hanner, M.S., Hauser, M.G., Levasseur-Regourd, A.-Ch., Mann, I., Mattila, K., Reach, W.T., Schlosser, W., Staude, H.J., Toller, G.N., Weiland, J.L., Weinberg, J.L., Witt, A.N., 1998. The 1997 reference of diffuse night sky brightness. Astron. Astrophys. Suppl. Ser. 127, 1-99.
11. Reach, W.T., Franz, B.A., Weiland, J.L., 1997. The three-dimensional structure of the zodiacal dust bands. Icarus 127, 461-484.
12. Roosen, R.G., 1970. An annotated bibliography on the Gegenschein. Icarus 13, 523-539.
13. Roosen, R.G., 1971. The Gegenschein. Rev. Geophys. Space Phys. 9, 275-304.
14. Tanabe, H., 1965. Photoelectric observations of the Gegenschein. Publ. Astron. Soc. Japan 17, 339-366.
15. Wright, E.L., Reese, E.D., 2000. Detection of the cosmic infrared background at 2.2 and 3.5 microns using DIRBE observations. Astrophys. J. 545, 43-55.