Zobrazeno 1 - 5
of 5
pro vyhledávání: '"ダスト微粒子"'
Autor:
Suyama, Toru, Tanaka, Hidekazu
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :37-40
In protoplanetary disk, dust grains grow through mutual collisions, gradually settle to the midplane of a disk. This process is initial condition of planet formation and it is very important process. In many of previous work, they assume that collisi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::5d02b84fbaaffaf03ed3bb0fbcd8420b
http://id.nii.ac.jp/1696/00020519/
http://id.nii.ac.jp/1696/00020519/
Autor:
Tanaka, Hidekazu
Publikováno v:
第38回月・惑星シンポジウム = Proceedings of the 38th ISAS Lunar and Planetary Symposium. :41-43
Sub-micrometer sized grains rapidly depletes due to dust growth in realistic weakly turbulent disks if dust disruption is not taken into account. This depletion of sub-micrometer sized grains makes the 10-micrometer silicate feature disappear in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::b43b30aef4e3f3cd130f621c6a6a3aa6
http://id.nii.ac.jp/1696/00020520/
http://id.nii.ac.jp/1696/00020520/
Publikováno v:
第28回月・惑星シンポジウム = Proceedings of the 28th ISAS Lunar and Planetary Symposium. :21-24
The motion of dust grains, released from comet Shoemaker-Levy 9 (SL9), has been examined, considering the influence of the Jovian magnetosphere. Especially, reentering of these grains to the Jovian magnetosphere in the middle of July 1994 is studied.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::f0f41811b3b22a28ffb1a98a0042188d
http://id.nii.ac.jp/1696/00038367/
http://id.nii.ac.jp/1696/00038367/
Autor:
Yamamoto, Satoru, Mukai, Tadashi
Publikováno v:
第28回月・惑星シンポジウム = Proceedings of the 28th ISAS Lunar and Planetary Symposium. :145-148
We have examined the origin of beta-meteoroids based on the sublimation of circumsolar dust grains. Orbital evolutions of particles starting to sublime at 8 solar radius have been studied. It is found that some of these particles with initial radii r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::0cab95bb6df484aaed97ac7b0a5a5c9d
http://id.nii.ac.jp/1696/00038400/
http://id.nii.ac.jp/1696/00038400/
Publikováno v:
第28回月・惑星シンポジウム = Proceedings of the 28th ISAS Lunar and Planetary Symposium. :177-177
The emission feature around 11.3 micrometer observed towards carbon stars is considered to be due to SiC grains condensed in the circumstellar envelopes. The isotopic anomalies of SiC discovered in carbonaceous meteorites strongly support the formati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::d80d939650a7ac4aca91496cd0a0cecf
http://id.nii.ac.jp/1696/00038408/
http://id.nii.ac.jp/1696/00038408/