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    Article

    The Cassini Visual And Infrared Map** Spectrometer (Vims) Investigation

    The Cassini visual and infrared map** spectrometer (VIMS) investigation is a multidisciplinary study of the Saturnian system. Visual and near-infrared imaging spectroscopy and high-speed spectrophotometry are t...

    R. H. Brown, K. H. Baines, G. Bellucci, J.-P. Bibring in Space Science Reviews (2004)

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    Virtis Experiment at Churyumov — Gerasimenko Comet, New Rosetta Target

    The targets of the Rosetta mission are the most primitive solar system bodies: comets and asteroids. The previous Rosetta mission was essentially devoted to study in detail a comet nucleus and to fly by one or...

    A. Coradini, F. Capaccioni, G. Filacchione, G. Magni in The New Rosetta Targets (2004)

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    The Cassini Visual and Infrared Map** Spectrometer (VIMS) Investigation

    The Cassini visual and infrared map** spectrometer (VIMS) investigation is a multidisciplinary study of the Saturnian system. Visual and near-infrared imaging spectroscopy and high-speed spectrophotometry are t...

    R. H. Brown, K. H. Baines, G. Bellucci, J.-P. Bibring in The Cassini-Huygens Mission (2004)

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    Planetary Fourier spectrometer: An interferometer for atmospheric studies on board Mars 94 mission

    PFS is a two-channel Fourier spectrometer operating in the infra-red wavelengths between 1.25 and 45 μm. The instrument will be used mainly in the study of the Martian atmosphere. The principal goals are the m...

    V. Formisano, V. Moroz, E. Amata, P. Baldetti, G. Bellucci in Il Nuovo Cimento C (1993)

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    An imaging spectrometer for planetary studies

    VNIR, a Visible Near-Infrared Map** Spectrometer, was developed at IFSI-CNR and it is the visible channel of an experiment, named OMEGA, to be flown on the Russian Mars 94 mission, that will provide detailed...

    G. Bellucci, F. Mastracci, V. Formisano, A. Adriani, F. Capaccioni in Il Nuovo Cimento C (1993)

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    Shapes of asteroids compared with fragments from hypervelocity impact experiments

    Light-curve observations have shown that most asteroids are non-axially symmetrical in shape, probably as a result of fragmentation undergone by objects with negligible gravitational binding1. Some earlier labora...

    F. Capaccioni, P. Cerroni, M. Coradini, P. Farinella, E. Flamini, G. Martelli in Nature (1984)

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    Radiofrequency emissions observed during macroscopic hypervelocity impact experiments

    Banded low-frequency radiofrequency (r.f.) signals, very low frequency propagation and light emission have been recorded to precede, accompany and follow some large earthquakes1–3, and mechanisms to account for t...

    R. Bianchi, F. Capaccioni, P. Cerroni, M. Coradini, E. Flamini, P. Hurren in Nature (1984)

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