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SUMMARY:Stereo image processing for the CASSIS camera - ExoMars Trace Gas 
 Orbiter
DTSTART:20151029T170000
DTEND:20151029T180000
DTSTAMP:20260506T174901Z
UID:2219b3c11a52203f71cd27bda84b72a2ac80ed84842b519ccd906dcf
CATEGORIES:Conferences - Seminars
DESCRIPTION:Stepan Tulyakov\, EPFL \nThe 2016 Mars mission is ESA-led and 
 launched by Roskosmos. ESA will provide a Mars orbiter and an Entry\, Desc
 ent and Landing (EDL) demonstrator. CaSSIS (Colour and Stereo Surface Imag
 ing System)\, is a high resolution imaging system designed to complement t
 he data acquired by the other payload on EMTGO while also enhancing our kn
 owledge of the surface of Mars by extending the observations of the High R
 esolution Imaging Science Experiment (HiRISE) which is currently orbiting 
 Mars onboard NASA’s Mars Reconnaissance Orbiter (MRO). One of the  goal
 s of the project is to produce high-resolution 3D models of Mars surface.\
 nThese 3D models will allow scientists to\n(1) identify potential sources 
 of trace gases\,\n(2) examine dynamic processes on surface and\n(3) evalua
 te landing sites for future missions.\nThis  presentation gives short ove
 rview of TGO mission\, our role in this mission. In particular\, the prese
 ntation shows results of on-ground geometric calibration of CaSSIS and my 
 current work on preparations for in-flight calibration using star fields. 
 Basic mathematical foundation of the work will be presented as well as res
 ults of recent geometric calibration and next steps for data processing an
 d analysis.\nAbout the presenter: Stepan Tulyakov is the PhD Candidate at 
 EPFL Space Engineering centre (eSpace). He received his Master Degree in R
 obotics from Bauman Moscow State University (2008) and Master Degree in Co
 mputer Science from Seoul National University (2010). Before joining eSpac
 e in 2015\, he spent 5 years as senior research engineer in Samsung Electr
 onics (South Korea).
LOCATION:PPH325 http://plan.epfl.ch/?room=PPH%20325
STATUS:CONFIRMED
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