메뉴 건너뛰기




Volumn 318, Issue 5848, 2007, Pages 240-243

Io volcanism seen by new horizons: A major eruption of the Tvashtar Volcano

(17)  Spencer, J R a   Stern, S A b   Cheng, A F b   Weaver, H A c   Reuter, D C d   Retherford, K e   Lunsford, A d   Moore, J M f   Abramov, O a   Lopes, R M C g   Perry, J E h   Kamp, L g   Showalter, M i   Jessup, K L a   Marchis, F i   Schenk, P M j   Dumas, C k  


Author keywords

[No Author keywords available]

Indexed keywords

BRIGHTNESS TEMPERATURE; JUPITER; MAGMA; NEAR INFRARED; PLUME; SPACECRAFT; VOLCANISM;

EID: 35348877331     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1147621     Document Type: Article
Times cited : (113)

References (23)
  • 1
    • 2442689388 scopus 로고    scopus 로고
    • E. P. Turtle et al., Icarus 169, 3 (2004).
    • (2004) Icarus , vol.169 , pp. 3
    • Turtle, E.P.1
  • 4
    • 35248820349 scopus 로고    scopus 로고
    • R. M. C. Lopes, J. R. Spencer, Eds, Praxis, Chichester, UK
    • P. Geissler, D. Goldstein, in Io After Galileo, R. M. C. Lopes, J. R. Spencer, Eds. (Praxis, Chichester, UK, 2007), pp. 163-192.
    • (2007) Io After Galileo , pp. 163-192
    • Geissler, P.1    Goldstein, D.2
  • 5
    • 35348862736 scopus 로고    scopus 로고
    • Pele-type plumes are thought to result from direct ejection of gas from a volcanic vent, whereas the smaller Prometheus-type plumes may result from remobilization of surface volatiles by lava flows.
    • "Pele-type" plumes are thought to result from direct ejection of gas from a volcanic vent, whereas the smaller "Prometheus-type" plumes may result from remobilization of surface volatiles by lava flows.
  • 7
    • 35348896274 scopus 로고    scopus 로고
    • U.S. Geological Survey Astrogeology Research Program
    • U.S. Geological Survey Astrogeology Research Program, http://astrogeology.usgs.gov/Projects/JupiterSatellites/io.html.
  • 8
    • 4544345813 scopus 로고    scopus 로고
    • P. E. Geissler et al., Icarus 172, 127 (2004).
    • (2004) Icarus , vol.172 , pp. 127
    • Geissler, P.E.1
  • 11
    • 0036854814 scopus 로고    scopus 로고
    • F. Marchis et al., Icarus 160, 124 (2002).
    • (2002) Icarus , vol.160 , pp. 124
    • Marchis, F.1
  • 12
    • 27744577666 scopus 로고    scopus 로고
    • M. P. Milazzo et al., Icarus 179, 235 (2005).
    • (2005) Icarus , vol.179 , pp. 235
    • Milazzo, M.P.1
  • 13
    • 18844418239 scopus 로고    scopus 로고
    • F. Marchis et al., Icarus 176, 96 (2005).
    • (2005) Icarus , vol.176 , pp. 96
    • Marchis, F.1
  • 17
    • 0001471362 scopus 로고    scopus 로고
    • A. S. McEwen et al., Icarus 135, 181 (1998).
    • (1998) Icarus , vol.135 , pp. 181
    • McEwen, A.S.1
  • 18
    • 0011772888 scopus 로고
    • D. Morrison, Ed, Univ. of Arizona Press, Tucson, AZ
    • R. G. Strom, N. M. Schneider, in Satellites of Jupiter, D. Morrison, Ed. (Univ. of Arizona Press, Tucson, AZ, 1982), pp. 598-633.
    • (1982) Satellites of Jupiter , pp. 598-633
    • Strom, R.G.1    Schneider, N.M.2
  • 19
    • 11144291551 scopus 로고    scopus 로고
    • J. Zhang et al., Icarus 172, 479 (2004).
    • (2004) Icarus , vol.172 , pp. 479
    • Zhang, J.1
  • 22
    • 0344766744 scopus 로고    scopus 로고
    • A. S. McEwen et al., Science 281, 87 (1998).
    • (1998) Science , vol.281 , pp. 87
    • McEwen, A.S.1
  • 23
    • 35348819012 scopus 로고    scopus 로고
    • We thank the entire NH mission team, particularly D. Rose and E. Birath, and our colleagues on the NH science team. NH and the ancillary investigations described here are funded by NASA, whose financial support we gratefully acknowledge
    • We thank the entire NH mission team, particularly D. Rose and E. Birath, and our colleagues on the NH science team. NH and the ancillary investigations described here are funded by NASA, whose financial support we gratefully acknowledge.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.