IPSE: The Italian package for scientific experiments on Mars

Autor: Angrilli, F., Debei, S., Rossi, F., De Marchi, E., Ferrario, R. ^*, Prendin, W., Terribile, A., Espinasse, S., Flaminis, E.

Publikováno v: In Planetary and Space Science 2004 52(1):41-45

The international package for scientific experiments (IPSE) for Mars surveyor program

Autor: Coradini, A., Angrilli, F., Bellucci, G., Bianchi, R., Capaccioni, F., Colangeli, L., Debei, S., De Sanctis, M.C., Di Lellis, A.M., Espinasse, S., Federico, C., Magni, G., Mahnes, G., Philippe, J.M.

Publikováno v: In Advances in Space Research 2001 28(8):1209-1218

MARS-IRMA: in-situ infrared microscope analysis of Martian soil and rock samples.

Autor: Capaccioni, F., Bellucci, G., Orosei, R., Amici, S., Bianchi, R., Blecka, M, Capria, M.T., Coradini, A., Erard, S., Fonti, S., Formisano, V., Forni, O., Mustard, J., Piccioni, G., Pieters, C., Poscolieri, M., Battistelli, E., Romoli, A., DiGiampietro, M., Espinasse, S., Magnani, M., Pasqui, C

Publikováno v: In Advances in Space Research 2001 28(8):1219-1224

A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express

Autor: Drossart, P, Piccioni, G, Gérard, JC, Lopez-Valverde, MA, Sanchez-Lavega, A, Zasova, L, Hueso, R, Taylor, FW, Bézard, B, Adriani, A, Angrilli, F, Arnold, G, Baines, KH, Bellucci, G, Benkhoff, J, Bibring, JP, Blanco, A, Blecka, MI, Carlson, RW, Coradini, A, Di Lellis, A, Encrenaz, T, Erard, S, Fonti, S, Formisano, V, Fouchet, T, Garcia, R, Haus, R, Helbert, J, Ignatiev, NI, Irwin, P, Langevin, Y, Lebonnois, S, Luz, D, Marinangeli, L, Orofino, V, Rodin, AV, Roos-Serote, MC, Saggin, B, Stam, DM, Titov, D, Visconti, G, Zambelli, M, Tsang, C, Ammannito, E, Barbis, A, Berlin, R, Bettanini, C, Boccaccini, A, Bonnello, G, Bouyé, M, Capaccioni, F, Cardesin, A, Carraro, F, Cherubini, G, Cosi, M, Dami, M, De Nino, M, Del Vento, D, Di Giampietro, M, Donati, A, Dupuis, O, Espinasse, S, Fabbri, A, Fave, A, Veltroni, IF, Filacchione, G, Garceran, K, Ghomchi, Y, Giustizi, M, Gondet, B, Hello, Y, Henry, F, Hofer, S, Huntzinger, G, Kachlicki, J, Knoll, R, Kouach, D, Mazzoni, A, Melchiorri, R, Mondello, G, Monti, F, Neumann, C, Nuccilli, F, Parisot, J, Pasqui, C, Perferi, S, Peter, G, Piacentino, A, Pompei, C, Réess, JM, Rivet, JP, Romano, A, Russ, N, Santoni, M, Scarpelli, A, Sémery, A, Soufflot, A, Stefanovitch, D, Suetta, E, Tarchi, F, Tonetti, N, Tosi, F, Ulmer, B

Publikováno v: Nature
Nature, Nature Publishing Group, 2007, 450, pp.641-645. ⟨10.1038/nature06140⟩
Nature, 2007, 450, pp.641-645. ⟨10.1038/nature06140⟩

The upper atmosphere of a planet is a transition region in which energy is transferred between the deeper atmosphere and outer space. Molecular emissions from the upper atmosphere (90-120 km altitude) of Venus can be used to investigate the energetic

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::283ef7d2baadcb9e7766add77da39785
http://ora.ox.ac.uk/objects/uuid:06a509aa-015c-4093-840c-ffe481c6f544

An assessment study for a NEO mission

Autor: Barucci A., Kofman W., Rocard F., Moura D., Brucato J., Dotto E., Ulamec S., Ball A., Harris A. W., Engrand C., Chazalnoel P., Valsecchi G. B., Espinasse S., Coradini A., Biel J., Mottola S., Green S., Morbidelli A., Gasnault O., Nathues A., Goesmann F., Demarchi E., Rossi A., Barriot J., Manhés G.

Publikováno v: European Geophysical Union General Assembly 2006, Vienna, Austria, 02-07/04/2006
info:cnr-pdr/source/autori:Barucci A., Kofman W., Rocard F., Moura D., Brucato J., Dotto E., Ulamec S., Ball A., Harris A. W., Engrand C., Chazalnoel P., Valsecchi G. B., Espinasse S., Coradini A., Biel J., Mottola S., Green S., Morbidelli A., Gasnault O., Nathues A., Goesmann F., Demarchi E., Rossi A., Barriot J., Manhés G./congresso_nome:European Geophysical Union General Assembly 2006/congresso_luogo:Vienna, Austria/congresso_data:02-07%2F04%2F2006/anno:2006/pagina_da:/pagina_a:/intervallo_pagine

The NEOs are representative of the population of asteroids and dead comets thought to be similar to the ancient planetesimal swarms that accreted to form the planets. The chemical investigation of NEOs having primitive characteristics is thus essenti

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::eeeecfd083988f27d355ffbf6ceaed8d
https://publications.cnr.it/doc/120311