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Spatial Distribution and Orbital Properties of Zodiacal Dust

Published online by Cambridge University Press:  12 April 2016

Bernhard Kneißel  and
Ingrid Mann
Bernhard Kneißel
Affiliation:
Ruhr-Universität Bochum, D 4630 Bochum, RFA
Ingrid Mann
Affiliation:
Ruhr-Universität Bochum, D 4630 Bochum, RFA

Abstract

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Within the recent years the spatial distribution of Zodiacal dust has been subject to a variety of modelling approaches. Whereas models derived from observations in the visual range tend to demand for an increase of interplanetary matter above the solar poles (bulges), models based on infrared measurements and extended to small r seem to favor a decrease there (holes). The models are reviewed, and the dynamical structure implicated in the models is outlined.

Type
Interplanetary Dust: Zodiacal Light and Optical Studies
Information
International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 139 - 146
Copyright
Copyright © Kluwer 1991

References

Allen, C.W. 1983: Astrophysical Quantities, The Athlone Press, 3. editionGoogle Scholar
Andreev, V.V. and Belkovich, O.I., 1985: Distribution of the Meteor Matter in Distance 1 AU from the Sun, IAU Gen. Ass.(New Dehli 1985)Google Scholar
Bandermann, L.W., 1968: Physical Properties and Dynamics of Interplanetary Dust, Ph.D. Thesis, University of Maryland Google Scholar
Ceplecha, Z., 1977: Meteoroid Populations and Orbits, in Comets, Asteroids, Meteorites (Delsemme, A.H. ed.), Univ. of Toledo Press, 143–152 Google Scholar
Ceplecha, Z., 1987: Numbers and Masses of Different Populations of Sporadic Meteoroids from Photographic and Television Records, Publ. Astron. Inst of the Czechosl. Academy of Sciences 67, Proc. Vol. 2, 241 Google Scholar
Deul, E.R. and Wolstencroft, R.D., 1987: A Physical Model for Thermal Emission from the Zodiacal Dust Cloud, Astron. Astrophys. 196, 277–286 Google Scholar
Dohnanyi, J.S., 1978: Particle Dynamics, in: Cosmic Dust (McDonnell, J.A.M., ed.), John Wiley Sons, New York, 527 Google Scholar
Dumont, R., Oral Presentation at the General Assembly IAU (Grenoble, 1976)Google Scholar
Dumont, R. and Levasseur-Regourd, A.-C., 1988: Properties of Interplanetary Dust from Infrared and Optical Observations. I. Temperature, Global Volume Intensity, Albedo and their Heliocentric Gradients, Astron. Astrophys. 191, 154 Google Scholar
Fechtig, H., 1989: Dust in the Solar System, Naturforsch, Z.. 44a, 877 Google Scholar
Giese, R.H. and v. Dziembowski, C. 1969: Suggested Zodiacal Light Measurements from Space Probes, Planet Space Sci., 17, 949 Google Scholar
Giese, R.H. and Kneißel, B., 1989: Threedimensional Models of the Zodiacal Dust Cloud: Compatibility of Proposed Infrared Modells, ICARUS 81, 369 Google Scholar
Good, J.C., Hauser, M.G., and Gautier, T.N., 1986: IRAS Observations of the Zodiacal Background, Adv. Space Res., 6, 83 Google Scholar
Greenberg, J.M. and Grim, R., 1986: The Origin and Evolution of Comet Nuclei and Comet Halley Results. In: Exploration of Halley’s Comet (Battrick, B., Rolfe, E.J., and Reinhard, R..eds.), ESA SP-250, 255 Google Scholar
Greenberg, J.M., 1990: Personal ComunicationGoogle Scholar
Grüm, E., Zook, H.A., Fechtig, H., and Giese, R.H., 1985: Collisional Balance of the Meteoritic Complex, ICARUS, 62, 244 Google Scholar
Hanner, M.S. and Newburn, R.L., 1989: Infrared Photometry of Comet Wilson at two Epochs. Astron.J 97, 254 CrossRefGoogle Scholar
Humes, D.H., 1980: Results of Pioneer 10 and 11 Meteoroid Experiments: Interplanetary and Near-Saturn. J.Geophys. Res. 79, 5841 CrossRefGoogle Scholar
Kneißel, B. and Giese, R.H., 1987: The Dynamics of the Zodiacal Dust Cloud on account of Optical and Infrared Observations. Publ., of the Astronomical Institute of the Czechosl. Acad. of Sc. 67, Vol. 2, 241 Google Scholar
Kneißel, B., 1988: PH.D. Thesis, University of Bochum Google Scholar
Kneißel, B. and Mann, I., 1990: Three-Dimensional Models of the Zodiacal Dust Cloud, in; Proc. of the 1.COSPAR Colloqium: Physics of the Outer Heliosphere (Grziedzielski, S., ed.), Pergamon Press PLC Google Scholar
Lamy, P.L. & Perrin, J.M., 1986: Volume Scattering Function and Space Distribution of the Interplanetary Dust Cloud, Astron. Astrophys. 163, 269 Google Scholar
Leinert, C., Link, H., Pitz, E. & Giese, R.H., 1976: Interpretation of a Rocket Photometry of the Inner Zodiacal Light, Astron. Astrophys., 47 Google Scholar
Leinert, C. and Grün, E., 1990: Interplanetary Dust, in: Physics of the Inner Helioshere, (Schwerin, R. and Marsch, E. eds.), Springer Google Scholar
Levasseur-Regourd, A.-C. and Dumont, R., 1980: Absolute Photometry of Zodiacal Light, Astron. Astrophys. 84, 277 Google Scholar
Levasseur-Regourd, A.-C., 1991: this issueGoogle Scholar
Lumme, K. and Bowell, E., 1985: Photometric Poperties of Zodiacal Light Particles, ICARUS, 62, 54 Google Scholar
Rahe, J. 1981: in: Landolt-Börnstein (Schaifers, K. and Vogt, H.H., eds.), Gruppe VI, Band 2, Teilband a, Springer, Berlin, 183–198 Google Scholar
Rittich, U., 1986: Diploma Thesis, BochumGoogle Scholar