Search Results - "Helbert, J."

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  1. 1

    The MASCOT Radiometer MARA for the Hayabusa 2 Mission by Grott, M., Knollenberg, J., Borgs, B., Hänschke, F., Kessler, E., Helbert, J., Maturilli, A., Müller, N.

    Published in Space science reviews (01-07-2017)
    “…The MASCOT radiometer MARA is a multi-spectral instrument which measures net radiative flux in six wavelength bands. MARA uses thermopile sensors as sensing…”
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    The Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) for the BepiColombo mission by Hiesinger, H., Helbert, J.

    Published in Planetary and space science (2010)
    “…Scheduled for launch on board the BepiColombo Mercury Planetary Orbiter (MPO) in 2014, the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) is an…”
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    What is controlling the reflectance spectra (0.35–150 µm) of hydrated (and dehydrated) carbonaceous chondrites? by Beck, Pierre, Maturilli, A., Garenne, A., Vernazza, P., Helbert, J., Quirico, E., Schmitt, B.

    Published in Icarus (New York, N.Y. 1962) (01-10-2018)
    “…•The 0.7 µm feature in hydrated carbonaceous chondrites correlates with water content.•Continuum reflectance is not related to carbon content but primary…”
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    The best temperature range to acquire reliable thermal infrared spectra from orbit by Nestola, F., Ferrari, S., Pamato, M. G., Redhammer, G., Helbert, J., Alvaro, M., Domeneghetti, M. C.

    Published in Scientific reports (24-06-2021)
    “…Solar System bodies undergo to daily and periodical variations of temperature that mainly depend on their closeness to the Sun. It is known that mineral…”
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    Biconical reflectance, micro‐Raman, and nano‐FTIR spectroscopy of the Didim (H3‐5) meteorite: Chemical content and molecular variations by Yesiltas, M., Kaya, M., Glotch, T. D., Brunetto, R., Maturilli, A., Helbert, J., Ozel, M. E.

    Published in Meteoritics & planetary science (01-11-2020)
    “…The Didim meteorite contains multiple lithologies and clasts of different petrologic types in a single stone. A mixture of H5 clasts in an unequilibrated H3…”
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    Deriving iron contents from past and future Venus surface spectra with new high-temperature laboratory emissivity data by Helbert, J, Maturilli, A, Dyar, M D, Alemanno, G

    Published in Science advances (15-01-2021)
    “…In situ information on the surface composition of Venus is based on measurements of a small number of landing sites. In the laboratory, we measured the…”
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    Venus surface thermal emission at 1 μm in VIRTIS imaging observations: Evidence for variation of crust and mantle differentiation conditions by Mueller, N., Helbert, J., Hashimoto, G. L., Tsang, C. C. C., Erard, S., Piccioni, G., Drossart, P.

    Published in Journal of Geophysical Research - Planets (01-05-2008)
    “…The Venus Express spacecraft images the nightside thermal emissions using the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS). At 1.02, 1.10, and…”
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    Thermal structure of Martian soil and the measurability of the planetary heat flow by Grott, M., Helbert, J., Nadalini, R.

    Published in Journal of Geophysical Research - Planets (01-09-2007)
    “…We investigate the influence of the external temperature forcing given by seasonal, interannual, and climatic temperature changes on the surface heat flow of…”
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  14. 14

    Rotation period of Venus estimated from Venus Express VIRTIS images and Magellan altimetry by Mueller, N.T., Helbert, J., Erard, S., Piccioni, G., Drossart, P.

    Published in Icarus (New York, N.Y. 1962) (01-02-2012)
    “…The 1.02 μm wavelength thermal emission of the nightside of Venus is strongly anti-correlated to the elevation of the surface. The VIRTIS instrument on Venus…”
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    Mid-infrared spectral variability for compositionally similar asteroids: Implications for asteroid particle size distributions by Vernazza, P., Carry, B., Emery, J., Hora, J.L., Cruikshank, D., Binzel, R.P., Jackson, J., Helbert, J., Maturilli, A.

    Published in Icarus (New York, N.Y. 1962) (01-06-2010)
    “…We report an unexpected variability among mid-infrared spectra (IRTF and Spitzer data) of eight S-type asteroids for which all other remote sensing…”
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    The Berlin emissivity database (BED) by Maturilli, A., Helbert, J., Moroz, L.

    Published in Planetary and space science (01-03-2008)
    “…Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces composition. Past, present and future missions to the solar…”
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    Olivine thermal emissivity under extreme temperature ranges: Implication for Mercury surface by Helbert, J., Nestola, F., Ferrari, S., Maturilli, A., Massironi, M., Redhammer, G.J., Capria, M.T., Carli, C., Capaccioni, F., Bruno, M.

    Published in Earth and planetary science letters (01-06-2013)
    “…The work shows, for the first time experimentally and numerically, how the thermal emissivity spectra of a Mg-rich olivine (i.e. Mg1.84Fe0.16SiO4, Fo92Fa8,…”
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    Spectral Properties and Physical Extent of Pyroclastic Deposits on Mercury: Variability Within Selected Deposits and Implications for Explosive Volcanism by Besse, S., Doressoundiram, A., Barraud, O., Griton, L., Cornet, T., Muñoz, C., Varatharajan, I., Helbert, J.

    Published in Journal of geophysical research. Planets (01-05-2020)
    “…Explosive volcanism on the surface of planet Mercury is visible through the pyroclastic deposits that surround morphologic features often identified as the…”
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    Martian Atmospheric Spectral End‐Members Retrieval From ExoMars Thermal Infrared (TIRVIM) Data by Alemanno, G., D’Amore, M., Maturilli, A., Helbert, J., Arnold, G., Korablev, O., Ignatiev, N., Grigoriev, A., Shakun, A., Trokhimovskiy, A.

    Published in Journal of geophysical research. Planets (01-09-2022)
    “…Key knowledge about planetary composition can be recovered from the study of thermal infrared spectral range datasets. This range has a huge diagnostic…”
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    Constraints on Mercury’s surface composition from MESSENGER and ground-based spectroscopy by Warell, J., Sprague, A., Kozlowski, R., Rothery, D.A., Lewis, N., Helbert, J., Cloutis, E.

    Published in Icarus (New York, N.Y. 1962) (01-09-2010)
    “…The composition and chemistry of Mercury’s regolith has been calculated from MESSENGER MASCS 0.3–1.3 μm spectra from the first flyby, using an implementation…”
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