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Three-dimensional analysis of spatial resolution of MIRO/Rosetta measurements at 67P/Churyumov-Gersimenko
Rezac, L.1; Zhao, Y.1,2,3; Hartogh, P.1; Ji, J.2,3; Marshall, D.1; Shi, X.1
2019-09-20
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN1432-0746
Volume630Pages:8
Corresponding AuthorRezac, L.(rezac@mps.mpg.de)
AbstractContext. The MIRO instrument's remote sensing capability is integral to constraining water density, temperature, and velocity fields in the coma of 67P/Churyumov-Gersimenko. Aims. Our aim is to quantify how much water density originates from the facets of the shape model within the field of view of MIRO versus the water contribution from all the other facets. This information is crucial to understanding the MIRO derived coma production rates and their relation to the nucleus characteristics, and to understanding the spatial resolution of the measurements. Methods. This study relies on a detailed 3D nucleus shape model, illumination conditions, and the pointing information of the viewing geometry. With these parameters we can evaluate the relative contribution of water density originating from facets directly inside the MIRO beam and outside the beam as a function of distance along the MIRO line of sight. We also calculate the ratio of in-beam versus out-of-beam water gas number density. Results. We demonstrate that despite the rather small MIRO field of view there is only a small fraction of molecules that originate from facets within the MIRO beam. This is true for the nadir, but a similar conclusion can also be applied to the limb observing geometry. Conclusions. The MIRO instrument cannot discriminate active from inactive regions directly from observations. This study also suggests that the beam averaged solar incidence angle, local time, and mean normal vectors are not necessarily related to molecules within the MIRO beam. These results also illustrate why the 1D spherical Haser model can be applied with relative success to analyzing the MIRO data (and generally any Rosetta measurements). The future possibilities of constraining gas activity distribution on the surface should use 3D codes extracting information from the MIRO spectral line shapes which contain additional information. The results presented here are applicable to remote sensing instruments on board Rosetta.
Keywordcomets: general comets: individual: 67P/CG
DOI10.1051/0004-6361/201935389
WOS KeywordCOMA
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000486989400033
PublisherEDP SCIENCES S A
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/32208
Collection中国科学院紫金山天文台
Corresponding AuthorRezac, L.
Affiliation1.Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany
2.Chinese Acad Sci, Purple Mt Observ, Key Lab Planetary Sci, Nanjing 210008, Jiangsu, Peoples R China
3.Chinese Acad Sci, CAS Ctr Excellence Comparat Planetol, Hefei, Anhui, Peoples R China
Recommended Citation
GB/T 7714
Rezac, L.,Zhao, Y.,Hartogh, P.,et al. Three-dimensional analysis of spatial resolution of MIRO/Rosetta measurements at 67P/Churyumov-Gersimenko[J]. ASTRONOMY & ASTROPHYSICS,2019,630:8.
APA Rezac, L.,Zhao, Y.,Hartogh, P.,Ji, J.,Marshall, D.,&Shi, X..(2019).Three-dimensional analysis of spatial resolution of MIRO/Rosetta measurements at 67P/Churyumov-Gersimenko.ASTRONOMY & ASTROPHYSICS,630,8.
MLA Rezac, L.,et al."Three-dimensional analysis of spatial resolution of MIRO/Rosetta measurements at 67P/Churyumov-Gersimenko".ASTRONOMY & ASTROPHYSICS 630(2019):8.
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