Search Results - "d'Uston, C."

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    Martian Eolian Dust Probed by ChemCam by Lasue, J., Cousin, A., Meslin, P.‐Y., Mangold, N., Wiens, R. C., Berger, G., Dehouck, E., Forni, O., Goetz, W., Gasnault, O., Rapin, W., Schroeder, S., Ollila, A., Johnson, J., Le Mouélic, S., Maurice, S., Anderson, R., Blaney, D., Clark, B., Clegg, S. M., d'Uston, C., Fabre, C., Lanza, N., Madsen, M. B., Martin‐Torres, J., Melikechi, N., Newsom, H., Sautter, V., Zorzano, M. P.

    Published in Geophysical research letters (28-10-2018)
    “…The ubiquitous eolian dust on Mars plays important roles in the current sedimentary and atmospheric processes of the planet. The ChemCam instrument retrieves a…”
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    Chemistry of Rocks and Soils at Meridiani Planum from the Alpha Particle X-ray Spectrometer by Rieder, R., Gellert, R., Anderson, R. C., Brückner, J., Clark, B. C., Dreibus, G., Economou, T., Klingelhöfer, G., Lugmair, G. W., Ming, D. W., Squyres, S. W., d'Uston, C., Wänke, H., Yen, A., Zipfel, J.

    “…The Alpha Particle X-ray Spectrometer on the Opportunity rover determined major and minor elements of soils and rocks in Meridiani Planum. Chemical…”
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    Chemistry of Rocks and Soils in Gusev Crater from the Alpha Particle X-ray Spectrometer by Gellert, R., Rieder, R., Anderson, R. C., Brückner, J., Clark, B. C., Dreibus, G., Economou, T., Klingelhöfer, G., Lugmair, G. W., Ming, D. W., Squyres, S. W., d'Uston, C., Wänke, H., Yen, A., Zipfel, J.

    “…The alpha particle x-ray spectrometer on the Spirit rover determined major and minor elements of soils and rocks in Gusev crater in order to unravel the…”
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    Uranium on the Moon: Global distribution and U/Th ratio by Yamashita, N., Hasebe, N., Reedy, R. C., Kobayashi, S., Karouji, Y., Hareyama, M., Shibamura, E., Kobayashi, M.-N., Okudaira, O., d'Uston, C., Gasnault, O., Forni, O., Kim, K. J.

    Published in Geophysical research letters (01-05-2010)
    “…The Kaguya Gamma‐Ray Spectrometer uniquely identified uranium gamma‐ray lines from the Moon with a superior energy resolution of ∼1%. A global lunar map of…”
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    The global distribution of calcium on the Moon: Implications for high-Ca pyroxene in the eastern mare region by Yamashita, N., Gasnault, O., Forni, O., d'Uston, C., Reedy, R.C., Karouji, Y., Kobayashi, S., Hareyama, M., Nagaoka, H., Hasebe, N., Kim, K.J.

    Published in Earth and planetary science letters (01-11-2012)
    “…The first unambiguous global distribution of Ca on the Moon has been revealed by the Kaguya Gamma-Ray Spectrometer. The observation of the 3737keV gamma rays…”
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    Bulk composition and early differentiation of Mars by Taylor, G. Jeffrey, Boynton, W., Brückner, J., Wänke, H., Dreibus, G., Kerry, K., Keller, J., Reedy, R., Evans, L., Starr, R., Squyres, S., Karunatillake, S., Gasnault, O., Maurice, S., d'Uston, C., Englert, P., Dohm, J., Baker, V., Hamara, D., Janes, D., Sprague, A., Kim, K., Drake, D.

    Published in Journal of Geophysical Research - Planets (01-03-2006)
    “…We report the concentrations of K, Th, and Fe on the Martian surface, as determined by the gamma ray spectrometer onboard the 2001 Mars Odyssey spacecraft. K…”
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    Estimation method of planetary fast neutron flux by a Ge gamma-ray spectrometer by Hareyama, M., Fujibayashi, Y., Yamashita, Y., Karouji, Y., Nagaoka, H., Kobayashi, S., Reedy, R.C., Gasnault, O., Forni, O., d'Uston, C., Kim, K.J., Hasebe, N.

    “…An intensity map of lunar fast neutrons (LFNs) and their temporal variation has been estimated by fitting “sawtooth” peaks in the energy spectra of lunar gamma…”
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    A three-dimensional plasma and energetic particle investigation for the wind spacecraft by Lin, R. P., Anderson, K. A., Ashford, S., Carlson, C., Curtis, D., Ergun, R., Larson, D., McFadden, J., McCarthy, M., Parks, G. K., R me, H., Bosqued, J. M., Coutelier, J., Cotin, F., D'Uston, C., Wenzel, K. -P., Sanderson, T. R., Henrion, J., Ronnet, J. C., Paschmann, G.

    Published in Space science reviews (01-02-1995)
    “…The objectives of the experiment for the WIND spacecraft reported here were to explore the suprathermal particle population between the solar wind and low…”
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