16 results on '"Arvidson, R"'
Search Results
2. Abundance and isotopic composition of gases in the martian atmosphere from the Curiosity rover
- Author
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Mahaffy, P. R., Webster, C. R., Atreya, S. K., Franz, H., Wong, M., Conrad, P. G., Harpold, D., Jones, J. J., Leshin, L. A., Manning, H., Owen, T., Pepin, R. O., Squyres, S., Trainer, M., Kemppinen, O., Bridges, N., Johnson, J. R., Minitti, M., Cremers, D., Bell, J. F., Edgar, L., Farmer, J., Godber, A., Wadhwa, M., Wellington, D., McEwan, I., Newman, C., Richardson, M., Charpentier, A., Peret, L., King, P., Blank, J., Weigle, G., Schmidt, M., Li, S., Milliken, R., Robertson, K., Sun, V., Baker, M., Edwards, C., Ehlmann, B., Farley, K., Griffes, J., Grotzinger, J., Miller, H., Newcombe, M., Pilorget, C., Rice, M., Siebach, K., Stack, K., Stolper, E., Brunet, C., Hipkin, V., Leveille, R., Marchand, G., Sanchez, P. S., Favot, L., Cody, G., Steele, A., Fluckiger, L., Lees, D., Nefian, A., Martin, M., Gailhanou, M., Westall, F., Israel, G., Agard, C., Baroukh, J., Donny, C., Gaboriaud, A., Guillemot, P., Lafaille, V., Lorigny, E., Paillet, A., Perez, R., Saccoccio, M., Yana, C., Armiens-Aparicio, C., Rodriguez, J. C., Blazquez, I. C., Gomez, F. G., Gomez-Elvira, J., Hettrich, S., Malvitte, A. L., Jimenez, M. M., Martinez-Frias, J., Martin-Soler, J., Martin-Torres, F. J., Jurado, A. M., Mora-Sotomayor, L., Caro, G. M., Lopez, S. N., Peinado-Gonzalez, V., Pla-Garcia, J., Manfredi, J. A. R., Romeral-Planello, J. J., Fuentes, S. A. S., Martinez, E. S., Redondo, J. T., Urqui-O'Callaghan, R., Mier, M.-P. Z., Chipera, S., Lacour, J.-L., Mauchien, P., Sirven, J.-B., Fairen, A., Hayes, A., Joseph, J., Sullivan, R., Thomas, P., Dupont, A., Lundberg, A., Melikechi, N., Mezzacappa, A., DeMarines, J., Grinspoon, D., Reitz, G., Prats, B., Atlaskin, E., Genzer, M., Harri, A.-M., Haukka, H., Kahanpaa, H., Kauhanen, J., Paton, M., Polkko, J., Schmidt, W., Siili, T., Fabre, C., Wray, J., Wilhelm, M. B., Poitrasson, F., Patel, K., Gorevan, S., Indyk, S., Paulsen, G., Gupta, S., Bish, D., Schieber, J., Gondet, B., Langevin, Y., Geffroy, C., Baratoux, D., Berger, G., Cros, A., d'Uston, C., Forni, O., Gasnault, O., Lasue, J., Lee, Q.-M., Maurice, S., Meslin, P.-Y., Pallier, E., Parot, Y., Pinet, P., Schroder, S., Toplis, M., Lewin, E., Brunner, W., Heydari, E., Achilles, C., Oehler, D., Sutter, B., Cabane, M., Coscia, D., Szopa, C., Dromart, G., Robert, F., Sautter, V., Le Mouelic, S., Mangold, N., Nachon, M., Buch, A., Stalport, F., Coll, P., Francois, P., Raulin, F., Teinturier, S., Cameron, J., Clegg, S., Cousin, A., DeLapp, D., Dingler, R., Jackson, R. S., Johnstone, S., Lanza, N., Little, C., Nelson, T., Wiens, R. C., Williams, R. B., Jones, A., Kirkland, L., Treiman, A., Baker, B., Cantor, B., Caplinger, M., Davis, S., Duston, B., Edgett, K., Fay, D., Hardgrove, C., Harker, D., Herrera, P., Jensen, E., Kennedy, M. R., Krezoski, G., Krysak, D., Lipkaman, L., Malin, M., McCartney, E., McNair, S., Nixon, B., Posiolova, L., Ravine, M., Salamon, A., Saper, L., Stoiber, K., Supulver, K., Van Beek, J., Van Beek, T., Zimdar, R., French, K. L., Iagnemma, K., Miller, K., Summons, R., Goesmann, F., Goetz, W., Hviid, S., Johnson, M., Lefavor, M., Lyness, E., Breves, E., Dyar, M. D., Fassett, C., Blake, D. F., Bristow, T., DesMarais, D., Edwards, L., Haberle, R., Hoehler, T., Hollingsworth, J., Kahre, M., Keely, L., McKay, C., Bleacher, L., Brinckerhoff, W., Choi, D., Dworkin, J. P., Eigenbrode, J., Floyd, M., Freissinet, C., Garvin, J., Glavin, D., Martin, D. K., McAdam, A., Pavlov, A., Raaen, E., Smith, M. D., Stern, J., Tan, F., Meyer, M., Posner, A., Voytek, M., Anderson, R. C., Aubrey, A., Beegle, L. W., Behar, A., Blaney, D., Brinza, D., Calef, F., Christensen, L., Crisp, J. A., DeFlores, L., Feldman, J., Feldman, S., Flesch, G., Hurowitz, J., Jun, I., Keymeulen, D., Maki, J., Mischna, M., Morookian, J. M., Parker, T., Pavri, B., Schoppers, M., Sengstacken, A., Simmonds, J. J., Spanovich, N., Juarez, M. d. l. T., Vasavada, A. R., Yen, A., Archer, P. D., Cucinotta, F., Ming, D., Morris, R. V., Niles, P., Rampe, E., Nolan, T., Fisk, M., Radziemski, L., Barraclough, B., Bender, S., Berman, D., Dobrea, E. N., Tokar, R., Vaniman, D., Williams, R. M. E., Yingst, A., Lewis, K., Cleghorn, T., Huntress, W., Manhes, G., Hudgins, J., Olson, T., Stewart, N., Sarrazin, P., Grant, J., Vicenzi, E., Wilson, S. A., Bullock, M., Ehresmann, B., Hamilton, V., Hassler, D., Peterson, J., Rafkin, S., Zeitlin, C., Fedosov, F., Golovin, D., Karpushkina, N., Kozyrev, A., Litvak, M., Malakhov, A., Mitrofanov, I., Mokrousov, M., Nikiforov, S., Prokhorov, V., Sanin, A., Tretyakov, V., Varenikov, A., Vostrukhin, A., Kuzmin, R., Clark, B., Wolff, M., McLennan, S., Botta, O., Drake, D., Bean, K., Lemmon, M., Schwenzer, S. P., Anderson, R. B., Herkenhoff, K., Lee, E. M., Sucharski, R., Hernandez, M. A. d. P., Avalos, J. J. B., Ramos, M., Kim, M.-H., Malespin, C., Plante, I., Muller, J.-P., Navarro-Gonzalez, R., Ewing, R., Boynton, W., Downs, R., Fitzgibbon, M., Harshman, K., Morrison, S., Dietrich, W., Kortmann, O., Palucis, M., Sumner, D. Y., Williams, A., Lugmair, G., Wilson, M. A., Rubin, D., Jakosky, B., Balic-Zunic, T., Frydenvang, J., Jensen, J. K., Kinch, K., Koefoed, A., Madsen, M. B., Stipp, S. L. S., Boyd, N., Campbell, J. L., Gellert, R., Perrett, G., Pradler, I., VanBommel, S., Jacob, S., Rowland, S., Savijarvi, H., Boehm, E., Bottcher, S., Burmeister, S., Guo, J., Kohler, J., Garcia, C. M., Mueller-Mellin, R., Wimmer-Schweingruber, R., Bridges, J. C., McConnochie, T., Benna, M., Bower, H., Brunner, A., Blau, H., Boucher, T., Carmosino, M., Elliott, H., Halleaux, D., Renno, N., Elliott, B., Spray, J., Thompson, L., Gordon, S., Newsom, H., Ollila, A., Williams, J., Vasconcelos, P., Bentz, J., Nealson, K., Popa, R., Kah, L. C., Moersch, J., Tate, C., Day, M., Kocurek, G., Hallet, B., Sletten, R., Francis, R., McCullough, E., Cloutis, E., ten Kate, I. L., Arvidson, R., Fraeman, A., Scholes, D., Slavney, S., Stein, T., Ward, J., Berger, J., Moores, J. E., GeoRessources, Institut national des sciences de l'Univers (INSU - CNRS)-Centre de recherches sur la géologie des matières premières minérales et énergétiques (CREGU)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), MSL Science Team, NWO-NSO: The role of perchlorates in the preservation of organic compounds on Mars, and Petrology
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010504 meteorology & atmospheric sciences ,Curiosity rover ,chemistry.chemical_element ,[SDU.STU]Sciences of the Universe [physics]/Earth Sciences ,Mars ,MSL Mars Atmosphere Isotopis Composition ,martian atmosphere ,01 natural sciences ,Astrobiology ,Isotopic signature ,chemistry.chemical_compound ,0103 physical sciences ,MSL ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Martian ,Multidisciplinary ,δ13C ,Atmosphere of Mars ,Nitrogen ,chemistry ,13. Climate action ,Sample Analysis at Mars ,Carbon dioxide ,Environmental science ,Carbon monoxide - Abstract
Mars' Atmosphere from Curiosity The Sample Analysis at Mars (SAM) instrument on the Curiosity rover that landed on Mars in August last year is designed to study the chemical and isotopic composition of the martian atmosphere. Mahaffy et al. (p. 263 ) present volume-mixing ratios of Mars' five major atmospheric constituents (CO 2 , Ar, N 2 , O 2 , and CO) and isotope measurements of 40 Ar/ 36 Ar and C and O in CO 2 , based on data from one of SAM's instruments, obtained between 31 August and 21 November 2012. Webster et al. (p. 260 ) used data from another of SAM's instruments obtained around the same period to determine isotope ratios of H, C, and O in atmospheric CO 2 and H 2 O. Agreement between the isotopic ratios measured by SAM with those of martian meteorites, measured in laboratories on Earth, confirms the origin of these meteorites and implies that the current atmospheric reservoirs of CO 2 and H 2 O were largely established after the period of early atmospheric loss some 4 billion years ago.
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- 2013
3. In situ radiometric and exposure age dating of the martian surface
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Farley, K.A., Malespin, C., Mahaffy, P., Grotzinger, J.P., Vasconcelos, P.M., Milliken, R.E., Malin, M., Edgett, K.S., Pavlov, A.A., Hurowitz, J.A., Grant, J.A., Miller, H.B., Arvidson, R., Beegle, L., Calef, F., Conrad, P.G., Dietrich, W.E., Eigenbrode, J., Gellert, R., Gupta, S., Hamilton, V., Hassler, D.M., Lewis, K.W., McLennan, S.M., Ming, D., Navarro-González, R., Schwenzer, S.P., Steele, A., Stolper, E.M., Sumner, D.Y., Vaniman, D., Vasavada, A., Williford, K., Wimmer-Schweingruber, R.F., MSL Science Team, the, NWO-NSO: The role of perchlorates in the preservation of organic compounds on Mars, Petrology, NWO-NSO: The role of perchlorates in the preservation of organic compounds on Mars, Petrology, California Institute of Technology (CALTECH), NASA Goddard Space Flight Center (GSFC), University of Queensland [Brisbane], Department of Geological Sciences [Providence], Brown University, Department of Geosciences [Stony Brook], Stony Brook University [SUNY] (SBU), State University of New York (SUNY)-State University of New York (SUNY), Center for Earth and Planetary Studies [Washington] (CEPS), Smithsonian National Air and Space Museum, Smithsonian Institution-Smithsonian Institution, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Department of Earth and Planetary Science [UC Berkeley] (EPS), University of California [Berkeley], University of California-University of California, Department of Physics [Guelph], University of Guelph, Department of Earth Science and Technology [Imperial College London], Imperial College London, Southwest Research Institute [Boulder] (SwRI), Princeton University, NASA Johnson Space Center (JSC), NASA, Instituto de Ciencias Nucleares [Mexico], Universidad Nacional Autónoma de México (UNAM), Dept. of Physical Sciences, The Open University [Milton Keynes] (OU), Geophysical Laboratory [Carnegie Institution], Carnegie Institution for Science [Washington], Planetary Science Institute [Tucson] (PSI), Kiel University, GeoRessources, and Centre National de la Recherche Scientifique (CNRS)-Université de Lorraine (UL)-Centre de recherches sur la géologie des matières premières minérales et énergétiques (CREGU)-Institut national des sciences de l'Univers (INSU - CNRS)
- Subjects
Geologic Sediments ,Extraterrestrial Environment ,010504 meteorology & atmospheric sciences ,Surface Properties ,Curiosity rover ,Geochemistry ,[SDU.STU]Sciences of the Universe [physics]/Earth Sciences ,Mars ,mudstone ,Radiation Dosage ,Noble Gases ,01 natural sciences ,Isotopes ,Impact crater ,Exobiology ,0103 physical sciences ,MSL ,Organic Chemicals ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Multidisciplinary ,Radiogenic nuclide ,Radiometric Dating ,Authigenic ,Gale Crater ,Scarp retreat ,13. Climate action ,Erosion ,Radiometric dating ,Sedimentary rock ,Evolution, Planetary ,Deposition (chemistry) ,Biomarkers ,Cosmic Radiation - Abstract
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-Ar age of 4.21 ± 0.35 billion years represents a mixture of detrital and authigenic components and confirms the expected antiquity of rocks comprising the crater rim. Cosmic-ray–produced 3 He, 21 Ne, and 36 Ar yield concordant surface exposure ages of 78 ± 30 million years. Surface exposure occurred mainly in the present geomorphic setting rather than during primary erosion and transport. Our observations are consistent with mudstone deposition shortly after the Gale impact or possibly in a later event of rapid erosion and deposition. The mudstone remained buried until recent exposure by wind-driven scarp retreat. Sedimentary rocks exposed by this mechanism may thus offer the best potential for organic biomarker preservation against destruction by cosmic radiation.
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- 2013
4. Report of the 2018 Joint Mars Rover Mission Joint Science Working Group (JSWG)
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Beaty, D., Kminek, G., Allwood, A., Arvidson, R., Borg, L., Farmer, J., Goesmann, F., Grant, J., Hauber, E., Murchie, S., Ori, G., Ruff, S., Rull, F., Sephton, M., Sherwood Lollar, B., Smith, C., Westall, F., Pacros, A., Wilson, M., Meyer, M., Vago, J., Bass, D., Joudrier, L., Laubach, S., Feldman, S., Trautner, R., and Milkovich, S.
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MOMA [ExoMars] ,Planets and Comets - Published
- 2012
5. Dissolution of fluorite (111) cleavage surface in acid pH: VSI, AFM and Monte Carlo simulations
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Cama, J., Zhang, L., Giudici, G., Soler, J. M., Arvidson, R. S., and Andreas Luttge
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- 2009
6. MRO/CRISM Retrieval of Surface Lambert Albedos for Multispectral Mapping of Mars with DISORT-based Rad. Transfer Modeling: Phase 1 - Using Historical Climatology for Temperatures, Aerosol Opacities, & Atmo. Pressures
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McGuire, P. C., Wolff, M. J., Smith, M. D., Arvidson, R. E., Murchie, S. L., Clancy, R. T., Roush, T. L., Cull, S. C., Lichtenberg, K. A., Wiseman, S. M., Green, R. O., Martin, T. Z., Milliken, R. E., Cavender, P. J., Humm, D. C., Seelos, F. P., Seelos, K. D., Taylor, H. W., Ehlmann, B. L., Mustard, J. F., Pelkey, S. M., Titus, T. N., Hash, C. D., Malaret, E. R., and Team, the CRISM
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Earth and Planetary Astrophysics (astro-ph.EP) ,FOS: Physical sciences ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Astrophysics - Earth and Planetary Astrophysics - Abstract
We discuss the DISORT-based radiative transfer pipeline ('CRISM_LambertAlb') for atmospheric and thermal correction of MRO/CRISM data acquired in multispectral mapping mode (~200 m/pixel, 72 spectral channels). Currently, in this phase-one version of the system, we use aerosol optical depths, surface temperatures, and lower-atmospheric temperatures, all from climatology derived from Mars Global Surveyor Thermal Emission Spectrometer (MGS-TES) data, and surface altimetry derived from MGS Mars Orbiter Laser Altimeter (MOLA). The DISORT-based model takes as input the dust and ice aerosol optical depths (scaled to the CRISM wavelength range), the surface pressures (computed from MOLA altimetry, MGS-TES lower-atmospheric thermometry, and Viking-based pressure climatology), the surface temperatures, the reconstructed instrumental photometric angles, and the measured I/F spectrum, and then outputs a Lambertian albedo spectrum. The Lambertian albedo spectrum is valuable geologically since it allows the mineralogical composition to be estimated. Here, I/F is defined as the ratio of the radiance measured by CRISM to the solar irradiance at Mars divided by $\pi$. After discussing the capabilities and limitations of the pipeline software system, we demonstrate its application on several multispectral data cubes: the outer northern ice cap of Mars, Tyrrhena Terra, and near the landing site for the Phoenix mission. For the icy spectra near the northern polar cap, aerosols need to be included in order to properly correct for the CO_2 absorption in the H_{2}O ice bands at wavelengths near 2.0 $\mu$m. In future phases of software development, we intend to use CRISM data directly in order to retrieve the spatiotemporal maps of aerosol optical depths, surface pressure and surface temperature.
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- 2009
- Full Text
- View/download PDF
7. Rock and Soil Physical Properties at the MER Gusev Crater and Meridiani Planum Landing Sites
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Richter, L., Arvidson, R., Bell, J., Cabrol, N., Gorevan, S., Greeley, R., Herkenhoff, K., Ming, D., Sullivan, R., and and the MER Athena Science Team
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Physical Properties ,MER Gusev Crater ,Meridiani Planum Landing Site - Published
- 2004
8. Rock and Soil Physical Properties at the MER Gusev Crater Landing Site: Initial Results
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Richter, L., Anderson, R.C., Arvidson, R., Bell J., Biesiadecki, J., Christensen, P., Golombek, M., Gorevan, S., Greeley, R., guinness, E., Haldemann, A.F.C., Herkenhoff, K., Landis, G., Li, R., Lindemann, R., Matijevic, J., Ming, D., Snider, N., Stewart, H., sullivan, R., Squyres, S.W., and MER Athena Science Team
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Physical Properties - Published
- 2004
9. Rock and Soil Physical Properties at the MER Gusev Crater and Meridiani Planum Landing Sites
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Richter, L., Arvidson, R., Bell, J., Cabrol, N., Ehlmann, B., Gorevan, S., Greeley, R., Herkenhoff, K., Ming, D., Sullivan, R., and and the MER Athena Science Team
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MER Gusev Crater - Published
- 2004
10. Merlin: Mars-moon exploration, reconnaissance and landed investigation
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Murchie, S. L., Chabot, N. L., Rivkin, A. S., Yen, A. S., Maki, J. N., Trebi-Ollennu, A., Arvidson, R. E., Wang, A., Gellert, R., Michael Daly, and Reed, C. L.
11. OMEGA: Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité
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Bibring, J. -P, Langevin, Y., Altieri, F., Arvidson, R., Beilud, G., Bertheĺ, M., Douté, S., Drossart, P., Encrenaz, T., Forget, F., Thierry Fouchet, Gendrin, A., Gondet, B., Mangold, N., Moroz, V., Mustard, J., Pinet, P., Poulet, F., Schmitt, B., Sotin, C., Soufflot, A., Titov, D., and Zasova, L.
12. Suffates in martian layered terrains : the OMEGA/Mars Express view
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Gendrin, A., Mangold, N., Bribing, J.-P., Langevin, Y., Gondet, B., Poulet, F., Bonello, G., Quantin, Catherine, Mustard, J., Arvidson, R.-E., Le Mouelic, S., Interactions et dynamique des environnements de surface (IDES), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), and CRINON, Evelyne
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[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology ,[SDU.STU.PL] Sciences of the Universe [physics]/Earth Sciences/Planetology ,ComputingMilieux_MISCELLANEOUS - Abstract
International audience
13. Ground-water sapping processes, Western Desert, Egypt
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Wei Luo, Arvidson, R. E., Sultan, M., Becker, R., Crombie, M. K., Neil Sturchio, and El Alfy, Z.
14. Rock Abrasion Tool: Mars exploration rover mission
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Gorevan, S. P., Myrick, T., Davis, K., Chau, J. J., Bartlett, P., Mukherjee, S., Anderson, R., Squyres, S. W., Arvidson, R. E., Morten Madsen, Bertelsen, P., Goetz, W., Binau, C. S., and Richter, L.
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Mars Exploration Rover
15. OMEGA: Observatoire pour la minéralogie, l'eau, les glaces et l'activité
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Bibring, J. -P, Soufflot, A., Berthé, M., Langevin, Y., Gondet, B., Drossart, P., Bouyé, M., Combes, M., Puget, P., Semery, A., Bellucci, G., Formisano, V., Moroz, V., Kottsov, V., Bonello, G., Stéphane Erard, Forni, O., Gendrin, A., Manaud, N., Poulet, F., Poulleau, G., Encrenaz, T., Fouchet, T., Melchiori, R., Altieri, F., Ignatiev, N., Titov, D., Zasova, L., Coradini, A., Capacionni, F., Cerroni, P., Fonti, S., Mangold, N., Pinet, P., Schmitt, B., Sotin, C., Hauber, E., Hoffmann, H., Jaumann, R., Keller, U., Arvidson, R., Mustard, J., Forget, F., Laboratoire de Planétologie et Géodynamique UMR6112 (LPG), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Université d'Angers (UA), Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Pôle Planétologie du LESIA, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
- Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,ComputingMilieux_MISCELLANEOUS - Abstract
International audience
16. Kink sites: A key to surface reactivity and dissolution kinetics
- Author
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Luttge, A., Cornelius Fischer, Zhang, L., and Arvidson, R. S.
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