An analytical model for the mass distribution of the interplanetary dust cloud

Advances in Space Research

Volumn 25, Issue 2, 2000, Pages 281-284

  Ishimoto, H ^a  

^a KOBE UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0039766635     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(99)00953-9     Document Type: Article

References (7)

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3. Grün, E., H. A. Zook, H. Fechtig, and R. H. Giese, Collisional Balance of the Meteoritic Complex, Icarus, 62, pp. 244-272 (1985).
4. Ishimoto, H. and I. Mann, Modeling the Particle Mass Distribution within 1AU of the Sun, Planet. Space Sci. (1998) in press
5. Mazets, E. P. et al., Comet Halley Dust, Environment from SP-2 Detector Measurements, Nature, 321, pp. 276-278 (1986).
6. Nakamura, A. and A. Fujiwara, Velocity Distribution of Fragments Formed in a Simulated Collisional Disruption, Icarus, 92, pp. 132-146 (1991).
7. Reach, W. T., B. A. Franz, and J. L. Weiland, The Three-Dimensional Structure of the Zodiacal Dust Bands, Icarus, 127, pp. 461-484 (1997).