elib
DLR-Header
DLR-Logo -> http://www.dlr.de
DLR Portal Home | Imprint | Contact | Deutsch
Fontsize: [-] Text [+]

CIVA

Bibring, J.-P. and Lamy, P. and Langevin, Y. and Soufflot, A. and Berthé, M. and Borg, J. and Poulet, F. and Mottola, S. (2007) CIVA. Space Science Reviews. Springer. DOI: 10.1007/s11214-006-9135-5. ISSN 1572-9672.

Full text not available from this repository.

Official URL: http://www.springerlink.com/content/d164425233r20551/

Abstract

CIVA (Comet Infrared and Visible Analyser) is an integrated set of imaging instruments, designed to characterize the 360◦ panorama (CIVA-P) as seen from the Rosetta Lander Philae, and to study surface and subsurface samples (CIVA-M). CIVA-P is a panoramic stereo camera, while CIVA-M is an optical microscope coupled to a near infrared microscopic hyperspectral imager. CIVA shares a common Imaging Main Electronics (IME) with ROLIS. CIVA-P will characterize the landing site, with an angular sampling (IFOV) of 1.1 mrad: each pixel will image a 1mm size feature at the distance of the landing legs, and a few metres at the local horizon. The panorama will be mapped by 6 identical miniaturized micro-cameras covering contiguous FOV, with their optical axis 60◦ apart. Stereoscopic capability will be provided by an additional micro-camera, identical to and co-aligned with one of the panoramic micro-camera, with its optical axis displaced by 10 cm. CIVA-M combines two ultra-compact and miniaturised microscopes, one operating in the visible and one constituting an IR hyperspectral imaging spectrometer: they will characterize, by non-destructive analyses, the texture, the albedo, the molecular and the mineralogical composition of each of the samples provided by the Sample Drill and Distribution (SD2) system. For the optical microscope, the spatial sampling is 7μm; for the IR, the spectral range (1–4μm) and the spectral sampling (5 nm) have been chosen to allow identification of most minerals, ices and organics, on each pixel, 40μm in size. After being studied by CIVA, the sample could be analysed by a subsequent experiment (PTOLEMY and/or COSAC). The processwould be repeated for each sample obtained at different depths and/or locations.

Document Type:Article
Additional Information:bisher nur Online-Veröffentlichung, Druck folgt noch
Title:CIVA
Authors:
AuthorsInstitution or Email of Authors
Bibring, J.-P.IAS, Orsay, France
Lamy, P.LAM, Marseille, France
Langevin, Y.IAS, Orsay, France
Soufflot, A.IAS, Orsay, France
Berthé, M.IAS, Orsay, France
Borg, J.IAS, Orsay, France
Poulet, F.IAS, Orsay, France
Mottola, S.UNSPECIFIED
Date:21 February 2007
Journal or Publication Title:Space Science Reviews
Refereed publication:Yes
In ISI Web of Science:Yes
DOI:10.1007/s11214-006-9135-5
Publisher:Springer
ISSN:1572-9672
Status:Published
Keywords:Cometary composition, in-situ imaging, microscopic analyses
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Projekt ROSETTA Instrumente (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Asteroids and Comets
Deposited By: Dr.phys. Stefano Mottola
Deposited On:14 Mar 2007
Last Modified:27 Apr 2009 13:35

Repository Staff Only: item control page

Browse
Search
Help & Contact
Informationen
electronic library is running on EPrints 3.3.12
Copyright © 2008-2012 German Aerospace Center (DLR). All rights reserved.