La Libs : les applications dun laser danalyse des systèmes
20 juin 2014 La spectroscopie de plasma induit par laser ou LIBS (acronyme anglais ... Le développement de l'instrument ChemCam
De chemcam à supercam : Lapport de la LIBS pour le spatial
de tirs laser effectué par ChemCam et les spectres LIBS correspondant à chaque point. LE ROVER PERSEVERANCE. POUR LA MISSION MARS 2020. L'instrument ChemCam
Chapitre n°16 : Transferts quantiques dénergie
Le laser de ChemCam émet-il de la lumière visible ? Justifier. 1.3. Montrer que les caractéristiques du faisceau laser utilisé par ChemCam permettent bien d'
SMARTCOURS
Le laser de ChemCam n'émet pas de la lumière visible mais de l'infrarouge. 1.3. Le document 1 nous indique que « le plasma se formera si au niveau de la cible
Laser-Induced Breakdown Spectroscopy (LIBS) characterization of
22 nov. 2021 Laser-Induced Breakdown Spec- troscopy (LIBS) characterization of granular soils: Implications for ChemCam analyses at Gale crater.
DOSSIER DE PRESSE
27 juin 2014 Sept kilomètres parcourus 150 000 tirs laser de ChemCam sur des roches ... ChemCam (IRAP – Université Toulouse III – Paul Sabatier / CNRS)
De chemcam à supercam: Lapport de la LIBS pour le spatial
7 août 2020 de tirs laser effectué par ChemCam et les spectres LIBS correspondant à chaque point. LE ROVER PERSEVERANCE. POUR LA MISSION MARS 2020.
CHEMCAM SUR LE ROVER MARTIEN CURIOSITY
L'instrument ChemCam (Chemistry and Camera) est le premier à utiliser un laser pour mesurer la composition chimique de la surface d'une autre planète.
Etude de lendommagement laser dans les cristaux non linéaires en
25 août 2009 1.6 – Schéma du design de la cavité du laser ChemCam. Le choix technologique des cristaux pour ce projet s'est porté sur le RTP pour le.
Laser-Induced Remote Sensing for Chemistry and Micro-Imaging
ChemCam uses a laser beam to remove dust from rock surfaces enabling remote sensing unhindered by the ubiquitous Mars dust. The suite combines LIBS elemental
ChemCamChemCam
for for ChemistryChemistryandandMicroMicro--ImagingImagingProposalProposal to MSLto MSLJuly 2004
July 2004
P.I. : Roger C.
P.I. : Roger C.
WiensWiens
(LANL)(LANL)Elemental Abundances from Laser-
Induced Breakdown Spectroscopy (LIBS)Most Detailed Remote Images Ever from the Remote Micro-Imager (RMI) SiMg AlBaScience ObjectivesScience Objectives
(1) Characterize the geology of the landing region, (1) Characterize the geology of the landing region,
(2) Investigate planetary processes relevant to past habitabilit (2) Investigate planetary processes relevant to past habitability, y, (3) Assess the biological potential of a target environment, (3) Assess the biological potential of a target environment, (4) Check for toxic materials. (4) Check for toxic materials.As a remote sensing instrument,
As a remote sensing instrument, ChemCamChemCam''ssprimary objective is to rapidly characterize primary objective is to rapidly characterize
rocks and soils, and to identify samples of greatest interest forocks and soils, and to identify samples of greatest interest for further investigation by the r further investigation by the
contact and analytical laboratory instrument contact and analytical laboratory instruments.s.Science TeamScience Team::
N. Bridges
N. BridgesJPLJPLS. MauriceS. MauriceCESRCESR
B. Clark
B. ClarkLMCOLMCOC. McKayC. McKayAmesAmes
D.D. CremersCremersLANLLANLH. NewsomH. NewsomUNMUNM
K. K. HerkenhoffHerkenhoffUSGSUSGSF. F. PoitrassonPoitrassonLMTGLMTGL. Kirkland
L. KirklandLPILPIV. V. SautterSautterMNHNMNHN
N. N. MangoldMangoldIDESIDESL. L. dd''UstonUstonCESRCESR G. G. ManhManhèèssIPGPIPGPD. D. VanimanVanimanLANLLANL P.P. MauchienMauchienCEACEAR. R. WiensWiensLANLLANL
450 m450 m
Depth Profile
Dust Removal
MSL Proposal ChemCam
Page FS-1 Fact Sheet
Laser-Induced Breakdown Spectrograph
LIBS focuses powerful laser pulses onto a
sample, causing ablation of atoms in excited states, which emit light. LIBS determines elemental compositions by spectrally resolving and measuring the emission lines from the ablated material.LIBS has the following characteristics:
No sample preparation required
Rapid analysis technique
Operates at a distance (2-13 m)
Removes dust from surfaces
Provides depth profiles
Detects all elements
10 ppm detection limits for some elements
Laser requires only 3 Watts of power
LIBS has been applied for over 20 years; its
use in laboratories and industry has increasedrapidly in recent years.ChemCam uses a laser beam to remove dust from rock surfaces, enabling remote sensing
unhindered by the ubiquitous Mars dust. The suite combines LIBS elemental analyses witha remote micro-imager (RMI) yielding the highest resolution images 2 m from the rover.Remote Micro-Imager
The RMI will provide very high resolution
images of targets. Its pixel field of view is21-22 µrad, much finer than any remote
camera that has operated on Mars. Its effective resolution exceeds that of MERPancam by a factor of 5 to 10. Resolution in
the near-field is within a factor of 2-3 ofMER MI (at closest-focus distance of 2 m for
RMI vs. 6 cm for MI), but still sufficient to
see many diagnostic sedimentary structures and other features at the sub-millimeter scale. Sub-meter-sized objects at the Mars horizon will be visible.Above is a MER MI image at a resolution
simulating RMI at a distance of 3m. Only half of the RMI field of view is illustrated.NASA/JPL/Cornell
MSL Proposal ChemCam
Page FS-2 Fact Sheet
LIBS soil spectrum recorded at a distance of 5.3 m shows fifteen elements ranging in abun- dance down to a few ppm. The three modules correspond to the ChemCam spectrographs.ChemCam Science Objectives
ChemCam addresses four of the five MSL
mission objectives, including (1) characterize the geology of the landing region, (2) investi- gate planetary processes relevant to past habit- ability, (3) assess the biological potential of a target environment, and (4) look for toxic mat- erials. As a remote sensing instrument, Chem-Cam's primary objective is to rapidly charac-
terize rocks and soils, and to identify samples of greatest interest for further investigation by contact and analytical laboratory instruments.ChemCam's science and operational
investigations are as follows:1 Rapid remote rock identification (ID)
2 Complement other techniques for rock
ID in cases of dust and weathering
3 Soil and pebble composition surveys
4 Quantitative analyses, including trace
elements, to support science objectives5 Detection of hydrated minerals
6 Rapid remote ID of surface ices
7 Depth profiles of rock weathering coats
8 Geomorphology and imaging science
9 Remote analysis of inaccessible rocks
10Assist arm and drill or corer sampling
11Remote ID of organic materials
12Check for abundances of elements above
hazardous limits for humansChemCam Analysis Sequence
The flow chart shows a typical analysis
sequence. After target acquisition by the rover mast, the telescope is focused and the target is micro-imaged. A burst of up to 75 laser shots (30 mJ) is fired at a 1 mm spot on the target.The spectrum from each spark is collected.
Deeper analyses utilize additional laser bursts.
A typical analysis takes 6 min. and 0.7 W-
hr, compared with up to 3 sols for analogous dust-free analyses requiring sample contact.MSL Proposal ChemCam
Page FS-3 Fact Sheet
12.0 Mb/solData Volume
8904 ccVolume
5.62 kg (+cable)Mass
Overall
0.10 - 0.44MTF at Nyquist
2 ms - 8 s
75 msExposure range
nominal800-1000 nmWavelength range
3.9 W-hr/solPower (6.7 W ave)
80 radSpatial resolution
2 m - infinityRange
100 mm diaAperture
SchmidtOptics design
RMI250Signal/Noise
Linear, 2048CCDs, # pixels
0.09-0.3 nmResolution
240-800 nmRange
Czerny TurnerDesign
Spectrographs(3)
40 sec/burstRecharge Rate
75 Pulses per Burst
15 HzPulse Rate
1067 nmWavelength
30 mJ/pulsePower
Laser0.5-1 mm diaAnalysis Spot
~0.4 m/pulse ~0.1 mm/pulseDepth Profile Rate (basalt & sand)2-13 mRange
LIBSInstrument Suite Description
As shown in the block diagram, the
suite consists of two boxes: the MastUnit contains the telescope, laser,
remote micro-imager (RMI), and front-end electronics, while the BodyUnit contains three spectrographs,
the DPU, power supply, and rover interface. Mast Unit Body Unit DPUMSL Proposal ChemCam
Page FS-4 Fact Sheet
Objectives for E/PO and New Technology: ChemCam will capture the public imagination like no other instrument. Both the highest resolution images and the innovative laser-gun analyses give high inherent appeal. ChemCam E/PO includes an interactive website that allows the public to view images and analyses along the rover route, teacher training both locally and at AAPT meetings, and public interactions by the nationally distributed team. E/PO is directed by Dr. Stephanie Shipp of the Lunar and Planetary Institute in Houston. Management Overview. ChemCam is developed by Los Alamos National Laboratory (LANL) and CESR in Toulouse, France. LANL has developed a long line of NASA instruments, including for Cassini, Lunar Prospector, Genesis, Mars Odyssey, and DAWN, and the ChemCam management team has direct experience in all of these. The PI, Dr. Roger Wiens, managed three of the Genesis instruments, and delivered these instruments on time and within budget. LANL's no-nonsense approach properly balances science return, cost, and risk. ChemCam utilizes the very close relationship between French Chemcam lead, Dr. Sylvestre Maurice, and LANL, which hasCOSTRY$
Phase A/B 1.0M
Phase C/D 4.7M
A-D Reserves 20% 1.2M
NASA TOTAL A-D6.9M
Phase E 5.4M
E Reserves 10% 0.5M
NASA TOTAL $12.8M
CNES Contrib. A-D 3.4M
Schedule
Start 11/04
PDR 10/05
CDR 10/06
Deliver EM 04/07
Deliver FM 02/08
Launch 11/09
Begin Roving 05/10
Mission End 05/12
Project End 03/13
ComponentProviderFlight Heritage
Laser Thales ESA LIDAR project
RMI & Telescope 3D-Plus & CESR Rosetta, Smart-1, others Spectrograph Ocean Optics, Inc. Other OOI spectrographs DPU, Pwr Supply LANL & 3D-Plus Numerous instrumentsIntegration LANL > 450 flight instruments
Team Leadership LANL Numerous instruments
Prototype Laser
Breadboard Telescope
Spectrograph on
Vibration Table
A dusty Mars needs ChemCam analyses.
resulted in over 30 joint publica- tions. LANL has a State Depart- ment license for joint international development of LIBS for space, and has been collaborating withCESR for several years. LIBS
instrumentation is CNES' top plan- etary science development priority. Science Requirementsfor LIBS include obtaining major element abundances to ±10%, along with minor and trace element charac- terization (including H,Li,Be,C,N,S), some to as low as 10 ppm.Data Volume
covers nearly 5,000 LIBS elemental analyses and a similar number of micro-images over the course of one Mars year.Readiness:RMI uses
flight-heritage imager;LIBS funded by MIDP
since 1998; field tested; environmental testing of all prototype parts to be complete by time of selection.quotesdbs_dbs46.pdfusesText_46[PDF] le lecteur d'oeuvre de fiction fuit il la réalité reponse
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