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Three-dimensional infrared models of the interplanetary dust distribution

Abstract

We have calculated the brightness of zodiacal emission by using the three dimensional optical models of zodiacal cloud. By comparing the calculated brightness distribution with the IRAS observations, we found that the cosine model is the best out of the three for describing the helioecliptic latitude dependence of dust distribution. We also found best parameters for the heliocentric variations of the dust temperature and volumetric absorption cross-section. Inclination and ascending node of the symmetry plane were deduced from annual variations of i) the peak offset latitude and ii) the pole brightness difference. Longitudes of the ascending node derived from i) and ii) are shown to be significantly different from each other.

References

  1. Dermott, S. F., P. D. Nicholson, and B. A. Wolven, Preliminary analysis of the IRAS 1. Solar System dust data, in Asteroids, Comets, Meteors II, edited by C.-I. Lagerkvist, B. Lindblad, H. Lundstedt, and H. Rickman, 583pp., HSC, Uppsala, 1986.

  2. Dermott, S. F., K. Grogan, E. K. Holmes, and S. J. Kortenkamp, The dynamical structure of the zodiacal cloud, paper presented at ZCS workshop, Kobe, 1997.

  3. Deul, E. R. and R. D. Wolstencroft, A physical model for thermal emission from the zodiacal dust cloud, Astron. Astrophys., 196, 277–286, 1988.

  4. Giese, R. H. and C. V. Dziembowski, Suggested zodiacal light measurements from space probes, Planet. Space Sci., 17, 949–956, 1969.

  5. Giese, R. H. and B. Kneißel, Three-dimensional models of the zodiacal cloud: II. Compatibility of proposed infrared models, Icarus, 81, 369–378, 1989.

  6. Giese, R. H., B. Kneißel, and U. Rittich, Three-dimensional models of the zodiacal dust cloud: A comparative study, Icarus, 68, 395–411, 1986.

  7. Hauser, M. G. and J. R. Houck, The zodiacal background in the IRAS data, in Light on Dark Matter, edited by F. P. Israel, 39pp., Dordrecht, Reidel, 1986.

  8. Hauser, M. G., T. N. Gautier, and F. J. Low, IRAS observations of the interplanetary dust emission, in Properties and Interactions of Interplanetary Dust, edited by R. Giese and P. Lamy, Reidel, Dordrecht, 43pp., 1985.

  9. Hong, S. S. and S. M. Kwon, Connection between the infrared zodiacal emission and the visible zodiacal light, Vistas in Astronomy, 31, 11–21, 1988.

  10. Hong, S. S. and S. M. Kwon, On the gegenschein and the symmetry plane, in Origin and Evolution of Interplanetary Dust, edited by A. C. Levasseur-Regourd and H. Hasegawa, 147pp., Kluwer, Dordrecht, 1991.

  11. Hong, S. S. and I. K. Um, Inversion of the zodiacal infrared brightness integral, Astrophys. J., 320, 928–935, 1987.

  12. Ishiguro, M., R. Nakamura, T. Watanabe, T. Mukai, H. Tanabe, I. Mann, H. Kimura, P. Hillebrand, and J. F. James, North-south asymmetry of the zodiacal light, in Proc. of the 29th ISAS Lunarand Planetary Symposium, edited by H. Mizutani, 64pp., ISAS, Kanagawa, 1996.

  13. Kneißel, B. and I. Mann, Spatial distribution and orbital properties of zodiacal dust, in Origin and Evolution of Interplanetary Dust, edited by A. C. Levasseur-Regourd and H. Hasegawa, 139pp., Kluwer, Dordrecht, 1991.

  14. Leinert, C., I. Richter, E. Pitz, and B. Planck, The zodiacal light from 1.0 to 0.3 A.U. as observed by the Helios space probes, Astron. Astrophys., 103, 177–188, 1981.

  15. Levasseur-Regourd, A. C. and R. Dumont, IRAS observations and local properties of interplanetary dust, Adv. Space Res., 10, (3)163–(3)170, 1990.

  16. Misconi, N. Y., The symmetry plane of the zodiacal cloud near 1 AU, in Solid Particles in the Solar System, edited by I. Halliday and B. A. McIntosh, 49pp., Dordrecht, Reidel, 1980.

  17. Murdock, T. L. and S. D. Price, Infrared measurements of the zodiacal light, Astron. J., 90, 375–386, 1985.

  18. Reach, W. T., Zodiacal emission II. Dust near the ecliptic, Astrophys. J., 369, 529–543, 1991.

  19. Rittich, U., Die räumliche Verteilung des Interplanetaren Staubes: Modellrechnungen zur Interpretation von Zodiakallichtmessungen, Diploma Thesis, Ruhr University, Bochum, 1986.

  20. Rowan-Robinson, M., J. Hughes, K. Vedi, and D. W. Walker, Modelling the IRAS zodiacal emission, MNRAS, 246, 273–278, 1990.

  21. Temi, P., P. De Bernardis, S. Masi, G. Moreno, and A. Salama, Infrared emission from interplanetary dust, Astrophys. J., 337, 528–535, 1989.

  22. Vrtilek, J. M. and M. G. Hauser, IRAS measurements of diffuse solar system radiation: Annual sky brightness variation and geometry of the interplanetary dust cloud, Astrophys. J., 455, 677–692, 1995.

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Correspondence to S. M. Kwon.

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Kwon, S.M., Hong, S.S. Three-dimensional infrared models of the interplanetary dust distribution. Earth Planet Sp 50, 501–505 (1998). https://doi.org/10.1186/BF03352141

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Keywords

  • Dust
  • Symmetry Plane
  • Ecliptic Plane
  • Ellipsoid Model
  • Dust Temperature