Overview
- Editors:
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A. C. Levasseur-Regourd
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Aeronomie CNRS, Université Paris VI, Verrières-le-Buisson, France
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H. Hasegawa
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Osaka Sangyo University, Osaka, Japan
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Table of contents (91 papers)
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Cometary Dust : Observations and Evolution
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- D. C. Boice, D. W. Naegeli, W. F. Huebner
Pages 265-268
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- Hiroki Akisawa, Takuma Oka, Ken Sugawara
Pages 269-272
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- Ken Sugawara, Jun-ichi Watanabe
Pages 273-276
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- J. Clairemidi, E. Brandon, P. Rousselot, G. Moreels
Pages 277-280
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- A. Fujiwara, T. Kadono, A. Nakamura, T. Ishibashi, N. Fujii
Pages 281-284
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- A. K. Sen, M. R. Deshpande, U. C. Joshi
Pages 285-288
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Meteoroids and Meteor Streams
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Front Matter
Pages 289-289
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- D. I. Steel, D. J. Asher, S.V.M. Clube
Pages 327-330
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- M. Gyssens, A. Knöfel, J. Rendtel, P. Roggemans
Pages 335-338
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Circumplanetary Dust Collisional and Electrostatic Processes
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Front Matter
Pages 339-339
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About this book
THE THE KYOTO KYOTO COLLOQUIUM COLLOQUIUM It It has has almost almost become become a a tradition tradition to to periodically periodically review review the the progress progress of of our our knowledge knowledge of of interplanetary interplanetary dust dust at at an an interdisciplinary interdisciplinary level. level. After After the the Honolulu Honolulu (1967), (1967), Heidelberg Heidelberg (1975), (1975), Ottawa Ottawa (1979) (1979) and and Marseilles Marseilles (1984) (1984) meetings, meetings, it it was was decided decided to to hold hold a a meeting meeting specially specially devoted devoted to to the the Origin Origin and and Evolution Evolution of of Interplanetary Interplanetary Dust Dust in in Kyoto, Kyoto, Japan Japan on on 27-30 27-30 August August 1990. 1990. This This colloquium colloquium was was certainly certainly appropriate appropriate in in location, location, timing timing and and objective. objective. The The choice choice of of the the location location was was most most appropriate, appropriate, not not only only because because of of the the charm charm of of the the beautiful beautiful city city of of Kyoto, Kyoto, but but also also because because of of the the important important involvement involvement of of our our Japanese Japanese colleagues, colleagues, both both in in observations observations of of interplanetary, interplanetary, cometary, cometary, meteoritic, meteoritic, circumplanetary circumplanetary or or circumstellar circumstellar dust, dust, and and in in physico-chemical physico-chemical analysis analysis or or theoretical theoretical developments. developments.
Editors and Affiliations
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Aeronomie CNRS, Université Paris VI, Verrières-le-Buisson, France
A. C. Levasseur-Regourd
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Osaka Sangyo University, Osaka, Japan
H. Hasegawa