Výsledky vyhledávání - "Stefanovitch, D."

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