Výsledky vyhledávání - "イオン-分子反応"

Reaction dynamics of molecular clusters in space: application of direct Ab initio molecular dynamics method

Autor: Tachikawa, Hiroto

Publikováno v: 低温科学. 78:141-153

光や宇宙線によって誘起される分子，およびクラスターの化学反応は，放射線化学，溶液化学および宇宙化学等における反応初期過程として極めて重要な役割を演じる．しかしながら，

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::7b13ba669a0ce68c67f71ffbc296e1f8
http://hdl.handle.net/2115/77776

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Gas-phase reaction of mineral clusters related to chemistry in space

Autor: Arakawa, Masashi

Publikováno v: 低温科学. 78:127-133

惑星形成過程での有機分子生成や水の運搬といった化学過程を探究するため，星間塵を構成する鉱物に類似した組成のクラスターと，水や一酸化炭素分子との気相反応を調べた．MglSiOm�

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::3827edb7d79ced99640ca51a9e17ac71
http://hdl.handle.net/2115/77774

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Research project on the formation of ice microparticles and their charging process

Autor: Yokota, Toshiaki

Publikováno v: スペース・プラズマ研究会平成16年度 = Space Plasma Conference FY2004. :16-19

資料番号: AA0063347005

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::24298cf65e786fb9c2b4bdf637a63504
http://id.nii.ac.jp/1696/00012680/

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Dissociation of gaseous complex ions of Mg(+)-methyl halides by means of polarized laser beam irradiation: Charge transfer and ejecting angle distribution of reaction products in clusters

Autor: Misaizu, Fuminori, Furuya, Ari, Tsunoyama, Hironori, Ono, Koichi

Publikováno v: 2003年度宇宙空間原子分子過程研究会:偏極・配向による原子分子過程の制御 = Symposium on Atom-Molecule Processes in Space 2003: Control of Atom-Molecule Processes by Polarization and Orientation. :19-22

資料番号: AA0047272005

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::d4cfbba95092bfbed4215cd5c4dbf884
http://id.nii.ac.jp/1696/00014008/

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Emission source model of Jupiter's H3(+) aurorae

Autor: Conneeney, Jhon E. P., Baron, Richard L., Sato, Takehiko

Publikováno v: 第28回月・惑星シンポジウム = Proceedings of the 28th ISAS Lunar and Planetary Symposium. :137-140

We mapped the distribution of H3(+) emissions in Jupiter's polar regions utilizing 3.4-micrometer images acquired with ProtoCAM at the NASA IRTF (Infrared Telescope Facility). A sequence of image mosaics was used to constrain the parameters of an emi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=jairo_______::e7f1754b0633d8f8c26416e21fffb6dd
http://id.nii.ac.jp/1696/00038398/

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