Hostname: page-component-5d59c44645-jqctd Total loading time: 0 Render date: 2024-02-22T22:06:26.765Z Has data issue: false hasContentIssue false

The Infrared Zodiacal Light

Published online by Cambridge University Press:  12 April 2016

Martha S. Hanner*
Affiliation:
Institute for Astronomy University of HawaiiHonolulu HI 96822

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Thermal emission from interplanetary dust is the main source of diffuse radiation at λ 5-50 μm. Analysis of infrared sky maps from IRAS and ZIP lead to the result that the average optical properties of the dust change with heliocentric distance. The present uncertainties in calibration should be resolved by COBE. Existence of a dust sublimation zone at 4 solar radii awaits confirmation at the next solar eclipse.

Type
Interplanetary Dust: Zodiacal Light and Optical Studies
Copyright
Copyright © Kluwer 1991

References

Beichman, C.A., Neugebauer, G., Habing, H.J., Clegg, P.E., Chester, T.J. (1988). IRAS Explanatory Supplement, NASA RP-1190, Vol. 1, 2nd. ed.Google Scholar
Berg, O.E. and Grün, E. (1973) Space Research, 13, 10471055.Google Scholar
Boulanger, F. and Pérault, M. (1988) Astrophys. J., 330, 964985.CrossRefGoogle Scholar
Briotta, D. (1976) Ph.D. dissertation, Cornell University, Astronomy Department.Google Scholar
Deul, E.R. and Wolstencroft, R.D. (1988) Astron. Astrophys., 196, 277286.Google Scholar
Dumont, R. and Levasseur-Regourd, A.-C. (1978) Astron. Astrophys., 64, 916.Google Scholar
Dumont, R. and Levasseur-Regourd, A.-C. (1988) Astron. Astrophys., 191, 154160.Google Scholar
Giese, R.H. and Kneissel, B. (1989) Icarus, 81, 369378.Google Scholar
Giese, R.H., Kneissel, B. and Rittich, U. (1986) Icarus, 68, 395411.CrossRefGoogle Scholar
Giese, R.H., Weiss, K. Zerall, R.H., and Ono, T. (1978) Astron. Astrophys., 65, 265272.Google Scholar
Good, J. C. (1988) preprint.CrossRefGoogle Scholar
Good, J. C. (1990) submitted to Astrophys. J.Google Scholar
Grün, E., Zook, H.A., Fechtig, H. and Giese, R.H. (1985) Icarus, 62, 244272.CrossRefGoogle Scholar
Gulkis, S., Lubin, P.M., Meyer, S.S., Silverberg, R.F. (1990) Scientific American, Jan. 1990, 132139.Google Scholar
Hauser, M.G. (1987) in Comets to Cosmology Lecture Notes in Physics, 297, 2739.CrossRefGoogle Scholar
Hauser, M.G. et al. (1984) Astrophys. J. Lett., 278, L15L18.CrossRefGoogle Scholar
Hong, S.S. and Um, I.K. (1987) Astrophys. J., 320, 928935.CrossRefGoogle Scholar
Lamy, P.L. (1974) Astron. Astrophys., 35, 197207.Google Scholar
Leinert, C., Hanner, M., Richter, I., and Pitz, E. (1980). Astron. Astrophys., 82, 328336.Google Scholar
Leinert, C., Richter, I., Pitz, E. and Planck, B. (1981) Astron. Astrophys., 103, 177188.Google Scholar
Léna, P., Viala, Y., Hall, D. and Soufflot, A. (1974) Astron. Astrophys., 37, 81.Google Scholar
Levasseur-Regourd, A.C., Dumont, R. and Renard, J.B. (1990a) Icarus, 86, 264272.CrossRefGoogle Scholar
Levasseur-Regourd, A.C., Renard, J.B., and Dumont, R. (1990b), these proceedings.Google Scholar
MacQueen, R. M. (1968) Astrophys. J., 154, 10591076.CrossRefGoogle Scholar
Mankin, W.G., MacQueen, R.M., and Lee, R.H. (1974) Astron. Astrophys., 31, 1721.Google Scholar
Mather, J.C. et al. (1990a) Astrophys. J. Lett., 354, L37L40.CrossRefGoogle Scholar
Mather, J.C. et al. (1990b) Preprint, April 1990. To appear in Observations in Earth Orbit and Beyond.Google Scholar
Mizutani, K., Maihara, T., Hiromoto, N., Takarni, H. (1984) Nature, 312, 134136.CrossRefGoogle Scholar
Mukai, T., Fechtig, H., Grün, E., Giese, R.H., and Mukai, S. (1986) Astron. Astrophys., 167, 364370.Google Scholar
Mukai, T. and Mukai, S. (1973) Publ. Astron. Soc. Japan, 25, 481488.Google Scholar
Mukai, T., Yamamoto, T., Hasegawa, H., Fujiwara, A., and Koike, C. (1974) Publ. Astron. Soc. Japan, 26, 445458.Google Scholar
Mukai, T. and Yamamoto, T (1979) Publ. Astron. Soc. Japan, 31, 585595.Google Scholar
Murdock, T.L. and Price, S.D. (1985) Astron. J., 90, 375386.Google Scholar
Neugebauer, G. et al. (1984) Astrophys. J. Lett., 278, L1L6.CrossRefGoogle Scholar
Peterson, A.W. (1963) Astrophys. J., 138, 12181230.CrossRefGoogle Scholar
Peterson, A.W. (1969) Astrophys. J., 155, 10091015.CrossRefGoogle Scholar
Peterson, A.W. (1971) Bull. Am. Astron. Soc., 3, 500.Google Scholar
Price, S.D., Murdock, T.L. and Marcotte, L.P. (1982) Astron. J., 87, 131.CrossRefGoogle Scholar
Price, S.D., Murdock, T.L. and Marcotte, L.P. (1980) Astron. J., 85, 765.CrossRefGoogle Scholar
Reach, W. (1988) Astrophys. J., 335, 468485.CrossRefGoogle Scholar
Röser, S., and Staude, H.J. (1978) Astron. Astrophys., 67, 381394.Google Scholar
Rowan-Robinson, M., Hughes, J., Vedi, K., Walker, D.W. (1990) Mon. Not. R.A.S., 246, 273278.Google Scholar
Salama, A. et al. (1987) Astron. J., 92, 467473.CrossRefGoogle Scholar
Schwehm, G. and Rohde, M. (1977) J. Geophys., 42, 727735.Google Scholar
Soifer, B.T., Houck, J.R. and Harwit, M. (1971) Astrophys. J., 168, L73L78.CrossRefGoogle Scholar
Temi, P., de Bernardis, P., Masi, S., Moreno, G. and Salama, A. (1989) Astrophys. J., 337, 528535.CrossRefGoogle Scholar
Zook, H.A. and Berg, O.E. (1975) Planet. Space Sci., 23, 183203.CrossRefGoogle Scholar