The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests
Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI)....
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Wiens, Roger C. [verfasserIn] Maurice, Sylvestre [verfasserIn] Barraclough, Bruce [verfasserIn] Saccoccio, Muriel [verfasserIn] Barkley, Walter C. [verfasserIn] Bell, James F. [verfasserIn] Bender, Steve [verfasserIn] Bernardin, John [verfasserIn] Blaney, Diana [verfasserIn] Blank, Jennifer [verfasserIn] Bouyé, Marc [verfasserIn] Bridges, Nathan [verfasserIn] Bultman, Nathan [verfasserIn] Caïs, Phillippe [verfasserIn] Clanton, Robert C. [verfasserIn] Clark, Benton [verfasserIn] Clegg, Samuel [verfasserIn] Cousin, Agnes [verfasserIn] Cremers, David [verfasserIn] Cros, Alain [verfasserIn] DeFlores, Lauren [verfasserIn] Delapp, Dorothea [verfasserIn] Dingler, Robert [verfasserIn] D’Uston, Claude [verfasserIn] Darby Dyar, M. [verfasserIn] Elliott, Tom [verfasserIn] Enemark, Don [verfasserIn] Fabre, Cecile [verfasserIn] Flores, Mike [verfasserIn] Forni, Olivier [verfasserIn] Gasnault, Olivier [verfasserIn] Hale, Thomas [verfasserIn] Hays, Charles [verfasserIn] Herkenhoff, Ken [verfasserIn] Kan, Ed [verfasserIn] Kirkland, Laurel [verfasserIn] Kouach, Driss [verfasserIn] Landis, David [verfasserIn] Langevin, Yves [verfasserIn] Lanza, Nina [verfasserIn] LaRocca, Frank [verfasserIn] Lasue, Jeremie [verfasserIn] Latino, Joseph [verfasserIn] Limonadi, Daniel [verfasserIn] Lindensmith, Chris [verfasserIn] Little, Cynthia [verfasserIn] Mangold, Nicolas [verfasserIn] Manhes, Gerard [verfasserIn] Mauchien, Patrick [verfasserIn] McKay, Christopher [verfasserIn] Miller, Ed [verfasserIn] Mooney, Joe [verfasserIn] Morris, Richard V. [verfasserIn] Morrison, Leland [verfasserIn] Nelson, Tony [verfasserIn] Newsom, Horton [verfasserIn] Ollila, Ann [verfasserIn] Ott, Melanie [verfasserIn] Pares, Laurent [verfasserIn] Perez, René [verfasserIn] Poitrasson, Franck [verfasserIn] Provost, Cheryl [verfasserIn] Reiter, Joseph W. [verfasserIn] Roberts, Tom [verfasserIn] Romero, Frank [verfasserIn] Sautter, Violaine [verfasserIn] Salazar, Steven [verfasserIn] Simmonds, John J. [verfasserIn] Stiglich, Ralph [verfasserIn] Storms, Steven [verfasserIn] Striebig, Nicolas [verfasserIn] Thocaven, Jean-Jacques [verfasserIn] Trujillo, Tanner [verfasserIn] Ulibarri, Mike [verfasserIn] Vaniman, David [verfasserIn] Warner, Noah [verfasserIn] Waterbury, Rob [verfasserIn] Whitaker, Robert [verfasserIn] Witt, James [verfasserIn] Wong-Swanson, Belinda [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2012 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962, 170(2012), 1-4 vom: 21. Juni, Seite 167-227 |
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| Übergeordnetes Werk: |
volume:170 ; year:2012 ; number:1-4 ; day:21 ; month:06 ; pages:167-227 |
| Links: |
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| DOI / URN: |
10.1007/s11214-012-9902-4 |
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| Katalog-ID: |
SPR017811678 |
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| 100 | 1 | |a Wiens, Roger C. |e verfasserin |4 aut | |
| 245 | 1 | 4 | |a The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests |
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| 520 | |a Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. | ||
| 650 | 4 | |a Mars |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Laser induced breakdown spectroscopy |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a LIBS |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a RMI |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Mars Science Laboratory |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a MSL |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Curiosity |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Gale Crater |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Laser plasma |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a ChemCam |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Maurice, Sylvestre |e verfasserin |4 aut | |
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| 700 | 1 | |a Bridges, Nathan |e verfasserin |4 aut | |
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| 700 | 1 | |a DeFlores, Lauren |e verfasserin |4 aut | |
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| 700 | 1 | |a Flores, Mike |e verfasserin |4 aut | |
| 700 | 1 | |a Forni, Olivier |e verfasserin |4 aut | |
| 700 | 1 | |a Gasnault, Olivier |e verfasserin |4 aut | |
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| 700 | 1 | |a Hays, Charles |e verfasserin |4 aut | |
| 700 | 1 | |a Herkenhoff, Ken |e verfasserin |4 aut | |
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| 700 | 1 | |a Kirkland, Laurel |e verfasserin |4 aut | |
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| 700 | 1 | |a LaRocca, Frank |e verfasserin |4 aut | |
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10.1007/s11214-012-9902-4 doi (DE-627)SPR017811678 (SPR)s11214-012-9902-4-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Wiens, Roger C. verfasserin aut The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. Mars (dpeaa)DE-He213 Laser induced breakdown spectroscopy (dpeaa)DE-He213 LIBS (dpeaa)DE-He213 RMI (dpeaa)DE-He213 Mars Science Laboratory (dpeaa)DE-He213 MSL (dpeaa)DE-He213 Curiosity (dpeaa)DE-He213 Gale Crater (dpeaa)DE-He213 Laser plasma (dpeaa)DE-He213 ChemCam (dpeaa)DE-He213 Maurice, Sylvestre verfasserin aut Barraclough, Bruce verfasserin aut Saccoccio, Muriel verfasserin aut Barkley, Walter C. verfasserin aut Bell, James F. verfasserin aut Bender, Steve verfasserin aut Bernardin, John verfasserin aut Blaney, Diana verfasserin aut Blank, Jennifer verfasserin aut Bouyé, Marc verfasserin aut Bridges, Nathan verfasserin aut Bultman, Nathan verfasserin aut Caïs, Phillippe verfasserin aut Clanton, Robert C. verfasserin aut Clark, Benton verfasserin aut Clegg, Samuel verfasserin aut Cousin, Agnes verfasserin aut Cremers, David verfasserin aut Cros, Alain verfasserin aut DeFlores, Lauren verfasserin aut Delapp, Dorothea verfasserin aut Dingler, Robert verfasserin aut D’Uston, Claude verfasserin aut Darby Dyar, M. verfasserin aut Elliott, Tom verfasserin aut Enemark, Don verfasserin aut Fabre, Cecile verfasserin aut Flores, Mike verfasserin aut Forni, Olivier verfasserin aut Gasnault, Olivier verfasserin aut Hale, Thomas verfasserin aut Hays, Charles verfasserin aut Herkenhoff, Ken verfasserin aut Kan, Ed verfasserin aut Kirkland, Laurel verfasserin aut Kouach, Driss verfasserin aut Landis, David verfasserin aut Langevin, Yves verfasserin aut Lanza, Nina verfasserin aut LaRocca, Frank verfasserin aut Lasue, Jeremie verfasserin aut Latino, Joseph verfasserin aut Limonadi, Daniel verfasserin aut Lindensmith, Chris verfasserin aut Little, Cynthia verfasserin aut Mangold, Nicolas verfasserin aut Manhes, Gerard verfasserin aut Mauchien, Patrick verfasserin aut McKay, Christopher verfasserin aut Miller, Ed verfasserin aut Mooney, Joe verfasserin aut Morris, Richard V. verfasserin aut Morrison, Leland verfasserin aut Nelson, Tony verfasserin aut Newsom, Horton verfasserin aut Ollila, Ann verfasserin aut Ott, Melanie verfasserin aut Pares, Laurent verfasserin aut Perez, René verfasserin aut Poitrasson, Franck verfasserin aut Provost, Cheryl verfasserin aut Reiter, Joseph W. verfasserin aut Roberts, Tom verfasserin aut Romero, Frank verfasserin aut Sautter, Violaine verfasserin aut Salazar, Steven verfasserin aut Simmonds, John J. verfasserin aut Stiglich, Ralph verfasserin aut Storms, Steven verfasserin aut Striebig, Nicolas verfasserin aut Thocaven, Jean-Jacques verfasserin aut Trujillo, Tanner verfasserin aut Ulibarri, Mike verfasserin aut Vaniman, David verfasserin aut Warner, Noah verfasserin aut Waterbury, Rob verfasserin aut Whitaker, Robert verfasserin aut Witt, James verfasserin aut Wong-Swanson, Belinda verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 170(2012), 1-4 vom: 21. Juni, Seite 167-227 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:170 year:2012 number:1-4 day:21 month:06 pages:167-227 https://dx.doi.org/10.1007/s11214-012-9902-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 170 2012 1-4 21 06 167-227 |
| spelling |
10.1007/s11214-012-9902-4 doi (DE-627)SPR017811678 (SPR)s11214-012-9902-4-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Wiens, Roger C. verfasserin aut The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. Mars (dpeaa)DE-He213 Laser induced breakdown spectroscopy (dpeaa)DE-He213 LIBS (dpeaa)DE-He213 RMI (dpeaa)DE-He213 Mars Science Laboratory (dpeaa)DE-He213 MSL (dpeaa)DE-He213 Curiosity (dpeaa)DE-He213 Gale Crater (dpeaa)DE-He213 Laser plasma (dpeaa)DE-He213 ChemCam (dpeaa)DE-He213 Maurice, Sylvestre verfasserin aut Barraclough, Bruce verfasserin aut Saccoccio, Muriel verfasserin aut Barkley, Walter C. verfasserin aut Bell, James F. verfasserin aut Bender, Steve verfasserin aut Bernardin, John verfasserin aut Blaney, Diana verfasserin aut Blank, Jennifer verfasserin aut Bouyé, Marc verfasserin aut Bridges, Nathan verfasserin aut Bultman, Nathan verfasserin aut Caïs, Phillippe verfasserin aut Clanton, Robert C. verfasserin aut Clark, Benton verfasserin aut Clegg, Samuel verfasserin aut Cousin, Agnes verfasserin aut Cremers, David verfasserin aut Cros, Alain verfasserin aut DeFlores, Lauren verfasserin aut Delapp, Dorothea verfasserin aut Dingler, Robert verfasserin aut D’Uston, Claude verfasserin aut Darby Dyar, M. verfasserin aut Elliott, Tom verfasserin aut Enemark, Don verfasserin aut Fabre, Cecile verfasserin aut Flores, Mike verfasserin aut Forni, Olivier verfasserin aut Gasnault, Olivier verfasserin aut Hale, Thomas verfasserin aut Hays, Charles verfasserin aut Herkenhoff, Ken verfasserin aut Kan, Ed verfasserin aut Kirkland, Laurel verfasserin aut Kouach, Driss verfasserin aut Landis, David verfasserin aut Langevin, Yves verfasserin aut Lanza, Nina verfasserin aut LaRocca, Frank verfasserin aut Lasue, Jeremie verfasserin aut Latino, Joseph verfasserin aut Limonadi, Daniel verfasserin aut Lindensmith, Chris verfasserin aut Little, Cynthia verfasserin aut Mangold, Nicolas verfasserin aut Manhes, Gerard verfasserin aut Mauchien, Patrick verfasserin aut McKay, Christopher verfasserin aut Miller, Ed verfasserin aut Mooney, Joe verfasserin aut Morris, Richard V. verfasserin aut Morrison, Leland verfasserin aut Nelson, Tony verfasserin aut Newsom, Horton verfasserin aut Ollila, Ann verfasserin aut Ott, Melanie verfasserin aut Pares, Laurent verfasserin aut Perez, René verfasserin aut Poitrasson, Franck verfasserin aut Provost, Cheryl verfasserin aut Reiter, Joseph W. verfasserin aut Roberts, Tom verfasserin aut Romero, Frank verfasserin aut Sautter, Violaine verfasserin aut Salazar, Steven verfasserin aut Simmonds, John J. verfasserin aut Stiglich, Ralph verfasserin aut Storms, Steven verfasserin aut Striebig, Nicolas verfasserin aut Thocaven, Jean-Jacques verfasserin aut Trujillo, Tanner verfasserin aut Ulibarri, Mike verfasserin aut Vaniman, David verfasserin aut Warner, Noah verfasserin aut Waterbury, Rob verfasserin aut Whitaker, Robert verfasserin aut Witt, James verfasserin aut Wong-Swanson, Belinda verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 170(2012), 1-4 vom: 21. Juni, Seite 167-227 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:170 year:2012 number:1-4 day:21 month:06 pages:167-227 https://dx.doi.org/10.1007/s11214-012-9902-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 170 2012 1-4 21 06 167-227 |
| allfields_unstemmed |
10.1007/s11214-012-9902-4 doi (DE-627)SPR017811678 (SPR)s11214-012-9902-4-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Wiens, Roger C. verfasserin aut The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. Mars (dpeaa)DE-He213 Laser induced breakdown spectroscopy (dpeaa)DE-He213 LIBS (dpeaa)DE-He213 RMI (dpeaa)DE-He213 Mars Science Laboratory (dpeaa)DE-He213 MSL (dpeaa)DE-He213 Curiosity (dpeaa)DE-He213 Gale Crater (dpeaa)DE-He213 Laser plasma (dpeaa)DE-He213 ChemCam (dpeaa)DE-He213 Maurice, Sylvestre verfasserin aut Barraclough, Bruce verfasserin aut Saccoccio, Muriel verfasserin aut Barkley, Walter C. verfasserin aut Bell, James F. verfasserin aut Bender, Steve verfasserin aut Bernardin, John verfasserin aut Blaney, Diana verfasserin aut Blank, Jennifer verfasserin aut Bouyé, Marc verfasserin aut Bridges, Nathan verfasserin aut Bultman, Nathan verfasserin aut Caïs, Phillippe verfasserin aut Clanton, Robert C. verfasserin aut Clark, Benton verfasserin aut Clegg, Samuel verfasserin aut Cousin, Agnes verfasserin aut Cremers, David verfasserin aut Cros, Alain verfasserin aut DeFlores, Lauren verfasserin aut Delapp, Dorothea verfasserin aut Dingler, Robert verfasserin aut D’Uston, Claude verfasserin aut Darby Dyar, M. verfasserin aut Elliott, Tom verfasserin aut Enemark, Don verfasserin aut Fabre, Cecile verfasserin aut Flores, Mike verfasserin aut Forni, Olivier verfasserin aut Gasnault, Olivier verfasserin aut Hale, Thomas verfasserin aut Hays, Charles verfasserin aut Herkenhoff, Ken verfasserin aut Kan, Ed verfasserin aut Kirkland, Laurel verfasserin aut Kouach, Driss verfasserin aut Landis, David verfasserin aut Langevin, Yves verfasserin aut Lanza, Nina verfasserin aut LaRocca, Frank verfasserin aut Lasue, Jeremie verfasserin aut Latino, Joseph verfasserin aut Limonadi, Daniel verfasserin aut Lindensmith, Chris verfasserin aut Little, Cynthia verfasserin aut Mangold, Nicolas verfasserin aut Manhes, Gerard verfasserin aut Mauchien, Patrick verfasserin aut McKay, Christopher verfasserin aut Miller, Ed verfasserin aut Mooney, Joe verfasserin aut Morris, Richard V. verfasserin aut Morrison, Leland verfasserin aut Nelson, Tony verfasserin aut Newsom, Horton verfasserin aut Ollila, Ann verfasserin aut Ott, Melanie verfasserin aut Pares, Laurent verfasserin aut Perez, René verfasserin aut Poitrasson, Franck verfasserin aut Provost, Cheryl verfasserin aut Reiter, Joseph W. verfasserin aut Roberts, Tom verfasserin aut Romero, Frank verfasserin aut Sautter, Violaine verfasserin aut Salazar, Steven verfasserin aut Simmonds, John J. verfasserin aut Stiglich, Ralph verfasserin aut Storms, Steven verfasserin aut Striebig, Nicolas verfasserin aut Thocaven, Jean-Jacques verfasserin aut Trujillo, Tanner verfasserin aut Ulibarri, Mike verfasserin aut Vaniman, David verfasserin aut Warner, Noah verfasserin aut Waterbury, Rob verfasserin aut Whitaker, Robert verfasserin aut Witt, James verfasserin aut Wong-Swanson, Belinda verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 170(2012), 1-4 vom: 21. Juni, Seite 167-227 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:170 year:2012 number:1-4 day:21 month:06 pages:167-227 https://dx.doi.org/10.1007/s11214-012-9902-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 170 2012 1-4 21 06 167-227 |
| allfieldsGer |
10.1007/s11214-012-9902-4 doi (DE-627)SPR017811678 (SPR)s11214-012-9902-4-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Wiens, Roger C. verfasserin aut The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. 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Juni, Seite 167-227 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:170 year:2012 number:1-4 day:21 month:06 pages:167-227 https://dx.doi.org/10.1007/s11214-012-9902-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 170 2012 1-4 21 06 167-227 |
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10.1007/s11214-012-9902-4 doi (DE-627)SPR017811678 (SPR)s11214-012-9902-4-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Wiens, Roger C. verfasserin aut The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. Mars (dpeaa)DE-He213 Laser induced breakdown spectroscopy (dpeaa)DE-He213 LIBS (dpeaa)DE-He213 RMI (dpeaa)DE-He213 Mars Science Laboratory (dpeaa)DE-He213 MSL (dpeaa)DE-He213 Curiosity (dpeaa)DE-He213 Gale Crater (dpeaa)DE-He213 Laser plasma (dpeaa)DE-He213 ChemCam (dpeaa)DE-He213 Maurice, Sylvestre verfasserin aut Barraclough, Bruce verfasserin aut Saccoccio, Muriel verfasserin aut Barkley, Walter C. verfasserin aut Bell, James F. verfasserin aut Bender, Steve verfasserin aut Bernardin, John verfasserin aut Blaney, Diana verfasserin aut Blank, Jennifer verfasserin aut Bouyé, Marc verfasserin aut Bridges, Nathan verfasserin aut Bultman, Nathan verfasserin aut Caïs, Phillippe verfasserin aut Clanton, Robert C. verfasserin aut Clark, Benton verfasserin aut Clegg, Samuel verfasserin aut Cousin, Agnes verfasserin aut Cremers, David verfasserin aut Cros, Alain verfasserin aut DeFlores, Lauren verfasserin aut Delapp, Dorothea verfasserin aut Dingler, Robert verfasserin aut D’Uston, Claude verfasserin aut Darby Dyar, M. verfasserin aut Elliott, Tom verfasserin aut Enemark, Don verfasserin aut Fabre, Cecile verfasserin aut Flores, Mike verfasserin aut Forni, Olivier verfasserin aut Gasnault, Olivier verfasserin aut Hale, Thomas verfasserin aut Hays, Charles verfasserin aut Herkenhoff, Ken verfasserin aut Kan, Ed verfasserin aut Kirkland, Laurel verfasserin aut Kouach, Driss verfasserin aut Landis, David verfasserin aut Langevin, Yves verfasserin aut Lanza, Nina verfasserin aut LaRocca, Frank verfasserin aut Lasue, Jeremie verfasserin aut Latino, Joseph verfasserin aut Limonadi, Daniel verfasserin aut Lindensmith, Chris verfasserin aut Little, Cynthia verfasserin aut Mangold, Nicolas verfasserin aut Manhes, Gerard verfasserin aut Mauchien, Patrick verfasserin aut McKay, Christopher verfasserin aut Miller, Ed verfasserin aut Mooney, Joe verfasserin aut Morris, Richard V. verfasserin aut Morrison, Leland verfasserin aut Nelson, Tony verfasserin aut Newsom, Horton verfasserin aut Ollila, Ann verfasserin aut Ott, Melanie verfasserin aut Pares, Laurent verfasserin aut Perez, René verfasserin aut Poitrasson, Franck verfasserin aut Provost, Cheryl verfasserin aut Reiter, Joseph W. verfasserin aut Roberts, Tom verfasserin aut Romero, Frank verfasserin aut Sautter, Violaine verfasserin aut Salazar, Steven verfasserin aut Simmonds, John J. verfasserin aut Stiglich, Ralph verfasserin aut Storms, Steven verfasserin aut Striebig, Nicolas verfasserin aut Thocaven, Jean-Jacques verfasserin aut Trujillo, Tanner verfasserin aut Ulibarri, Mike verfasserin aut Vaniman, David verfasserin aut Warner, Noah verfasserin aut Waterbury, Rob verfasserin aut Whitaker, Robert verfasserin aut Witt, James verfasserin aut Wong-Swanson, Belinda verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 170(2012), 1-4 vom: 21. Juni, Seite 167-227 (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:170 year:2012 number:1-4 day:21 month:06 pages:167-227 https://dx.doi.org/10.1007/s11214-012-9902-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 170 2012 1-4 21 06 167-227 |
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Wiens, Roger C. @@aut@@ Maurice, Sylvestre @@aut@@ Barraclough, Bruce @@aut@@ Saccoccio, Muriel @@aut@@ Barkley, Walter C. @@aut@@ Bell, James F. @@aut@@ Bender, Steve @@aut@@ Bernardin, John @@aut@@ Blaney, Diana @@aut@@ Blank, Jennifer @@aut@@ Bouyé, Marc @@aut@@ Bridges, Nathan @@aut@@ Bultman, Nathan @@aut@@ Caïs, Phillippe @@aut@@ Clanton, Robert C. @@aut@@ Clark, Benton @@aut@@ Clegg, Samuel @@aut@@ Cousin, Agnes @@aut@@ Cremers, David @@aut@@ Cros, Alain @@aut@@ DeFlores, Lauren @@aut@@ Delapp, Dorothea @@aut@@ Dingler, Robert @@aut@@ D’Uston, Claude @@aut@@ Darby Dyar, M. @@aut@@ Elliott, Tom @@aut@@ Enemark, Don @@aut@@ Fabre, Cecile @@aut@@ Flores, Mike @@aut@@ Forni, Olivier @@aut@@ Gasnault, Olivier @@aut@@ Hale, Thomas @@aut@@ Hays, Charles @@aut@@ Herkenhoff, Ken @@aut@@ Kan, Ed @@aut@@ Kirkland, Laurel @@aut@@ Kouach, Driss @@aut@@ Landis, David @@aut@@ Langevin, Yves @@aut@@ Lanza, Nina @@aut@@ LaRocca, Frank @@aut@@ Lasue, Jeremie @@aut@@ Latino, Joseph @@aut@@ Limonadi, Daniel @@aut@@ Lindensmith, Chris @@aut@@ Little, Cynthia @@aut@@ Mangold, Nicolas @@aut@@ Manhes, Gerard @@aut@@ Mauchien, Patrick @@aut@@ McKay, Christopher @@aut@@ Miller, Ed @@aut@@ Mooney, Joe @@aut@@ Morris, Richard V. @@aut@@ Morrison, Leland @@aut@@ Nelson, Tony @@aut@@ Newsom, Horton @@aut@@ Ollila, Ann @@aut@@ Ott, Melanie @@aut@@ Pares, Laurent @@aut@@ Perez, René @@aut@@ Poitrasson, Franck @@aut@@ Provost, Cheryl @@aut@@ Reiter, Joseph W. @@aut@@ Roberts, Tom @@aut@@ Romero, Frank @@aut@@ Sautter, Violaine @@aut@@ Salazar, Steven @@aut@@ Simmonds, John J. @@aut@@ Stiglich, Ralph @@aut@@ Storms, Steven @@aut@@ Striebig, Nicolas @@aut@@ Thocaven, Jean-Jacques @@aut@@ Trujillo, Tanner @@aut@@ Ulibarri, Mike @@aut@@ Vaniman, David @@aut@@ Warner, Noah @@aut@@ Waterbury, Rob @@aut@@ Whitaker, Robert @@aut@@ Witt, James @@aut@@ Wong-Swanson, Belinda @@aut@@ |
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Wiens, Roger C. |
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Wiens, Roger C. ddc 600 bkl 39.00 misc Mars misc Laser induced breakdown spectroscopy misc LIBS misc RMI misc Mars Science Laboratory misc MSL misc Curiosity misc Gale Crater misc Laser plasma misc ChemCam The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests |
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600 ASE 39.00 bkl The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests Mars (dpeaa)DE-He213 Laser induced breakdown spectroscopy (dpeaa)DE-He213 LIBS (dpeaa)DE-He213 RMI (dpeaa)DE-He213 Mars Science Laboratory (dpeaa)DE-He213 MSL (dpeaa)DE-He213 Curiosity (dpeaa)DE-He213 Gale Crater (dpeaa)DE-He213 Laser plasma (dpeaa)DE-He213 ChemCam (dpeaa)DE-He213 |
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ddc 600 bkl 39.00 misc Mars misc Laser induced breakdown spectroscopy misc LIBS misc RMI misc Mars Science Laboratory misc MSL misc Curiosity misc Gale Crater misc Laser plasma misc ChemCam |
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ddc 600 bkl 39.00 misc Mars misc Laser induced breakdown spectroscopy misc LIBS misc RMI misc Mars Science Laboratory misc MSL misc Curiosity misc Gale Crater misc Laser plasma misc ChemCam |
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The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests |
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The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests |
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Wiens, Roger C. Maurice, Sylvestre Barraclough, Bruce Saccoccio, Muriel Barkley, Walter C. Bell, James F. Bender, Steve Bernardin, John Blaney, Diana Blank, Jennifer Bouyé, Marc Bridges, Nathan Bultman, Nathan Caïs, Phillippe Clanton, Robert C. Clark, Benton Clegg, Samuel Cousin, Agnes Cremers, David Cros, Alain DeFlores, Lauren Delapp, Dorothea Dingler, Robert D’Uston, Claude Darby Dyar, M. Elliott, Tom Enemark, Don Fabre, Cecile Flores, Mike Forni, Olivier Gasnault, Olivier Hale, Thomas Hays, Charles Herkenhoff, Ken Kan, Ed Kirkland, Laurel Kouach, Driss Landis, David Langevin, Yves Lanza, Nina LaRocca, Frank Lasue, Jeremie Latino, Joseph Limonadi, Daniel Lindensmith, Chris Little, Cynthia Mangold, Nicolas Manhes, Gerard Mauchien, Patrick McKay, Christopher Miller, Ed Mooney, Joe Morris, Richard V. Morrison, Leland Nelson, Tony Newsom, Horton Ollila, Ann Ott, Melanie Pares, Laurent Perez, René Poitrasson, Franck Provost, Cheryl Reiter, Joseph W. Roberts, Tom Romero, Frank Sautter, Violaine Salazar, Steven Simmonds, John J. Stiglich, Ralph Storms, Steven Striebig, Nicolas Thocaven, Jean-Jacques Trujillo, Tanner Ulibarri, Mike Vaniman, David Warner, Noah Waterbury, Rob Whitaker, Robert Witt, James Wong-Swanson, Belinda |
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chemcam instrument suite on the mars science laboratory (msl) rover: body unit and combined system tests |
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The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests |
| abstract |
Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. |
| abstractGer |
Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. |
| abstract_unstemmed |
Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. In this paper we describe the body unit, optical fiber, and calibration targets, and the assembly, testing, and verification of the instrument prior to launch. |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR017811678</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111053803.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201006s2012 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11214-012-9902-4</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR017811678</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11214-012-9902-4-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Wiens, Roger C.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2012</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The ChemCam instrument suite on the Mars Science Laboratory (MSL) rover Curiosity provides remote compositional information using the first laser-induced breakdown spectrometer (LIBS) on a planetary mission, and provides sample texture and morphology data using a remote micro-imager (RMI). Overall, ChemCam supports MSL with five capabilities: remote classification of rock and soil characteristics; quantitative elemental compositions including light elements like hydrogen and some elements to which LIBS is uniquely sensitive (e.g., Li, Be, Rb, Sr, Ba); remote removal of surface dust and depth profiling through surface coatings; context imaging; and passive spectroscopy over the 240–905 nm range. ChemCam is built in two sections: The mast unit, consisting of a laser, telescope, RMI, and associated electronics, resides on the rover’s mast, and is described in a companion paper. ChemCam’s body unit, which is mounted in the body of the rover, comprises an optical demultiplexer, three spectrometers, detectors, their coolers, and associated electronics and data handling logic. Additional instrument components include a 6 m optical fiber which transfers the LIBS light from the telescope to the body unit, and a set of onboard calibration targets. ChemCam was integrated and tested at Los Alamos National Laboratory where it also underwent LIBS calibration with 69 geological standards prior to integration with the rover. Post-integration testing used coordinated mast and instrument commands, including LIBS line scans on rock targets during system-level thermal-vacuum tests. 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| score |
7.398551 |