Composition of Titan's lower atmosphere and simple surface volatiles as measured by the Cassini-Huyg...
Composition of Titan's lower atmosphere and simple surface volatiles as measured by the Cassini-Huygens probe gas chromatograph mass spectrometer experiment
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Publisher
Washington, DC: Blackwell Publishing Ltd
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Language
English
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Washington, DC: Blackwell Publishing Ltd
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The Cassini‐Huygens probe gas chromatograph mass spectrometer (GCMS) determined the composition of the Titan atmosphere from ∼140 km altitude to the surface. After landing, it returned composition data of gases evaporated from the surface. Height profiles of molecular nitrogen (N2), methane (CH4), and molecular hydrogen (H2) were determined. Traces...
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Full title
Composition of Titan's lower atmosphere and simple surface volatiles as measured by the Cassini-Huygens probe gas chromatograph mass spectrometer experiment
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TN_cdi_hal_primary_oai_HAL_hal_03786662v1
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_03786662v1
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ISSN
0148-0227,2169-9097
E-ISSN
2156-2202,2169-9100
DOI
10.1029/2010JE003659
