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dc.contributor.authorLai, Ian-Linen_US
dc.contributor.authorSu, Cheng-Chinen_US
dc.contributor.authorIp, Wing-Huenen_US
dc.contributor.authorWei, Chen-Enen_US
dc.contributor.authorWu, Jong-Shinnen_US
dc.contributor.authorLo, Ming-Chungen_US
dc.contributor.authorLiao, Yingen_US
dc.contributor.authorThomas, Nicolasen_US
dc.date.accessioned2017-04-21T06:56:45Z-
dc.date.available2017-04-21T06:56:45Z-
dc.date.issued2016-03en_US
dc.identifier.issn0167-9295en_US
dc.identifier.urihttp://dx.doi.org/10.1007/s11038-016-9481-6en_US
dc.identifier.urihttp://hdl.handle.net/11536/133493-
dc.description.abstractWith a combination of the Direct Simulation Monte Carlo (DSMC) calculation and test particle computation, the ballistic transport process of the hydroxyl radicals and oxygen atoms produced by photodissociation of water molecules in the coma of comet 67P/Churyumov-Gerasimenko is modelled. We discuss the key elements and essential features of such simulations which results can be compared with the remote-sensing and in situ measurements of cometary gas coma from the Rosetta mission at different orbital phases of this comet.en_US
dc.language.isoen_USen_US
dc.subjectCometsen_US
dc.subjectComet 67Pen_US
dc.subjectAtmosphereen_US
dc.subjectPhotodissociationen_US
dc.titleTransport and Distribution of Hydroxyl Radicals and Oxygen Atoms from H2O Photodissociation in the Inner Coma of Comet 67P/Churyumov-Gerasimenkoen_US
dc.identifier.doi10.1007/s11038-016-9481-6en_US
dc.identifier.journalEARTH MOON AND PLANETSen_US
dc.citation.volume117en_US
dc.citation.issue1en_US
dc.citation.spage23en_US
dc.citation.epage39en_US
dc.contributor.department機械工程學系zh_TW
dc.contributor.departmentDepartment of Mechanical Engineeringen_US
dc.identifier.wosnumberWOS:000373166500002en_US
Appears in Collections:Articles


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