Search Results - "Combe, J"

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    Vesta surface thermal properties map by Capria, M. T., Tosi, F., De Sanctis, M. C., Capaccioni, F., Ammannito, E., Frigeri, A., Zambon, F., Fonte, S., Palomba, E., Turrini, D., Titus, T. N., Schröder, S. E., Toplis, M., Li, J.-Y., Combe, J.-P., Raymond, C. A., Russell, C. T.

    Published in Geophysical research letters (16-03-2014)
    “…The first ever regional thermal properties map of Vesta has been derived from the temperatures retrieved by infrared data by the mission Dawn. The low average…”
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    Experimental determination of acetylene and ethylene solubility in liquid methane and ethane: Implications to Titan’s surface by Singh, S., Combe, J.-Ph, Cordier, D., Wagner, A., Chevrier, V.F., McMahon, Z.

    Published in Geochimica et cosmochimica acta (01-07-2017)
    “…In this study, the solubility of acetylene (or ethyne, C2H2) and ethylene (or ethene, C2H4) in liquid methane (CH4) and ethane (C2H6) has been experimentally…”
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    Sources and physical processes responsible for OH/H2O in the lunar soil as revealed by the Moon Mineralogy Mapper (M3) by McCord, T. B., Taylor, L. A., Combe, J.‐P., Kramer, G., Pieters, C. M., Sunshine, J. M., Clark, R. N.

    Published in Journal of Geophysical Research: Planets (01-06-2011)
    “…Analysis of two absorption features near 3 μm in the lunar reflectance spectrum, observed by the orbiting M3 spectrometer and interpreted as being due to OH…”
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    ACETYLENE ON TITAN'S SURFACE by Singh, S., McCord, T. B., Combe, J-Ph, Rodriguez, S., Cornet, T., Mouélic, S. Le, Clark, R. N., Maltagliati, L., Chevrier, V. F.

    Published in The Astrophysical journal (01-09-2016)
    “…ABSTRACT Titan's atmosphere is opaque in the near-infrared due to gaseous absorptions, mainly by methane, and scattering by aerosols, except in a few…”
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    Deciphering sub-micron ice particles on Enceladus surface by Scipioni, F., Schenk, P., Tosi, F., D'Aversa, E., Clark, R., Combe, J.-Ph, Ore, C.M. Dalle

    Published in Icarus (New York, N.Y. 1962) (01-07-2017)
    “…•Sub-micron particles are abundant on darkest terrains.•A bright spot is identified on the North portion of the leading side.•Plumes deposits partially match…”
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    Surface water-ice deposits in the northern shadowed regions of Ceres by Platz, T., Nathues, A., Schorghofer, N., Preusker, F., Mazarico, E., Schröder, S. E., Byrne, S., Kneissl, T., Schmedemann, N., Combe, J.-P., Schäfer, M., Thangjam, G. S., Hoffmann, M., Gutierrez-Marques, P., Landis, M. E., Dietrich, W., Ripken, J., Matz, K.-D., Russell, C. T.

    Published in Nature astronomy (01-01-2017)
    “…Ceres, a dwarf planet located in the main asteroid belt, has a low bulk density 1 , and models predict that a substantial amount of water ice is present in its…”
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    Mineralogical mapping of Coniraya quadrangle of the dwarf planet Ceres by Raponi, A., Carrozzo, F.G., Zambon, F., De Sanctis, M.C., Ciarniello, M., Frigeri, A., Ammannito, E., Tosi, F., Combe, J.-Ph, Longobardo, A., Palomba, E., Pieters, C.M., Raymond, C.A., Russell, C.T.

    Published in Icarus (New York, N.Y. 1962) (15-01-2019)
    “…•We present a method for thermal removal from Ceres spectra.•Most of the crater floors are devoid of volatiles due to the impact events.•Na-carbonates on…”
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    Housing conditions differentially affect physiological and behavioural stress responses of zebrafish, as well as the response to anxiolytics by Parker, Matthew O, Millington, Mollie E, Combe, Fraser J, Brennan, Caroline H

    Published in PloS one (11-04-2012)
    “…Zebrafish are a widely utilised animal model in developmental genetics, and owing to recent advances in our understanding of zebrafish behaviour, their utility…”
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    Thermal measurements of dark and bright surface features on Vesta as derived from Dawn/VIR by Tosi, F., Capria, M.T., De Sanctis, M.C., Combe, J.-Ph, Zambon, F., Nathues, A., Schröder, S.E., Li, J.-Y., Palomba, E., Longobardo, A., Blewett, D.T., Denevi, B.W., Palmer, E., Capaccioni, F., Ammannito, E., Titus, T.M., Mittlefehldt, D.W., Sunshine, J.M., Russell, C.T., Raymond, C.A.

    Published in Icarus (New York, N.Y. 1962) (15-09-2014)
    “…•We considered 313 observations of DM units and 75 observations of BM units by VIR.•DM units observed close to local noon have temperatures between 260 and…”
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    Origins and diversity of the Bering Sea Island fauna: shifting linkages across the northern continents by Combe, Fraser J., Sikes, Derek S., Tkach, Vasyl V., Hope, Andrew G.

    Published in Biodiversity and conservation (01-04-2021)
    “…We synthesize the historical biogeography of non-marine fauna (mammals, birds, fish, non-parasitic and parasitic invertebrates) occurring across Bering Sea…”
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    Near-infrared spectra of liquid/solid acetylene under Titan relevant conditions and implications for Cassini/VIMS detections by Singh, S., Cornet, T., Chevrier, V.F., Combe, J.-Ph, McCord, T.B., Roe, L.A., Le Mouélic, S., Le Menn, E., Wasiak, F.C.

    Published in Icarus (New York, N.Y. 1962) (15-05-2016)
    “…•This is the first publication about the short-wavelength part of the spectrum of solid and liquid acetylene.•We observed variations of albedo and absorption…”
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    Conditions for Sublimating Water Ice to Supply Ceres' Exosphere by Landis, M. E., Byrne, S., Schörghofer, N., Schmidt, B. E., Hayne, P. O., Castillo‐Rogez, J., Sykes, M. V., Combe, J.‐P., Ermakov, A. I., Prettyman, T. H., Raymond, C. A., Russell, C. T.

    Published in Journal of geophysical research. Planets (01-10-2017)
    “…Observations of a water vapor exosphere around Ceres suggest that the dwarf planet may be episodically outgassing at a rate of ~6 kg s−1 from unknown sources…”
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