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EPSC2012-180.pdf

🔗 Source: meetingorganizer.copernicus.org

📊 Size: 2.11 MB

📄 Pages: 2 pages

⬇️ Downloads: 124

Summary

The Ultraviolet and Visible Spectrometer (UVIS) instrument on the ExoMars Trace Gas Orbiter mission requires an atmospheric model to provide synthetic UV transmission spectra. The model aims to constrain parameters such as dust and aerosol properties, and ozone distribution, to improve understanding of the Martian atmosphere. The UVIS instrument will take high-resolution spectra in nadir and occultation viewing orientations, allowing for analysis of atmospheric features such as the Hartley band of ozone absorption. A forward model will be used to simulate various dust loading scenarios, cloud formations, and viewing geometries, and to provide detection limits for given climatic conditions. The model will assist the instrument team and constrain parameters through spectral analysis of different atmospheric scenarios to maximize scientific outputs from the instrument data.

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Description

The Ultraviolet and Visible Spectrometer (UVIS) instrument on the ExoMars Trace Gas Orbiter mission requires an atmospheric model to provide synthetic UV...

Technical Information

File Format: PDF
File Size: 2.11 MB
Pages: 2
Language: EN
Total Downloads: 124
Last Updated: 1 week ago

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This PDF document about EPSC2012-180 provides comprehensive information and guidance. Whether you're a beginner or advanced user, this resource offers valuable insights into EPSC2012-180.