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On the Crystalline Silicate Component of Comet Dust

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Please use this identifier to cite or link to this item:http://hdl.handle.net/2115/42846

Title: On the Crystalline Silicate Component of Comet Dust
Authors: Greenberg, J. Mayo Browse this author
Li, Aigen Browse this author
Yamamoto, Tetsuo Browse this author
Kozasa, Takashi Browse this author
Issue Date: 1996
Publisher: Astronomical Society of the Pacific
Citation: Physics, chemistry, and dynamics of interplanetary dust : proceedings of the 150th Colloquium of the International Astronomical Union held in Gainesville, Florida, USA, 14-18 August 1995. Edited by Bo Å. S. Gustafson and Martha S. Hanner. ISBN: 1-886733-24-4
Journal Title: Astronomical Society of the Pacific conference series
Volume: 104
Start Page: 497
End Page: 506
Abstract: The effects of preaggregation silicate crystallinity and postaggregation silicate crystallinity on the 11.3 μm structure in comet dust emission have been calculated. Of the order of 10 - 20% crystallinity provides the best agreement to date with observation but the fits are not yet fully satisfactory.
Description: 150th Colloquium of the International Astronomical Union. 14-18 August 1995. Gainesville, Florida, USA.
Conference Name: Colloquium of the International Astronomical Union
Conference Sequence: 150
Conference Place: Gainesville, Florida
Type: proceedings
URI: http://hdl.handle.net/2115/42846
Appears in Collections:理学院・理学研究院 (Graduate School of Science / Faculty of Science) > 雑誌発表論文等 (Peer-reviewed Journal Articles, etc)

Submitter: 小笹 隆司

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