메뉴 건너뛰기




Volumn 307, Issue 5713, 2005, Pages 1251-1255

Ultraviolet imaging spectroscopy shows an active Saturnian system

Author keywords

[No Author keywords available]

Indexed keywords

ATOMS; ICE; IMAGING TECHNIQUES; OXYGEN; SOLAR SYSTEM; ULTRAVIOLET SPECTROSCOPY; WATER;

EID: 20044389669     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1105606     Document Type: Article
Times cited : (104)

References (35)
  • 3
    • 0000552183 scopus 로고
    • B. Sandel et al., Science 215, 548 (1982).
    • (1982) Science , vol.215 , pp. 548
    • Sandel, B.1
  • 7
    • 14544290253 scopus 로고    scopus 로고
    • in preparation
    • D. E. Shemansky et al., in preparation.
    • Shemansky, D.E.1
  • 14
    • 18244391447 scopus 로고    scopus 로고
    • D. A. Gurnett et al., Nature 415, 985 (2002).
    • (2002) Nature , vol.415 , pp. 985
    • Gurnett, D.A.1
  • 15
    • 14544290719 scopus 로고    scopus 로고
    • in preparation
    • W. R. Pryor et al., in preparation.
    • Pryor, W.R.1
  • 16
    • 20044376077 scopus 로고    scopus 로고
    • D. T. Young et al., Science 307, 1262 (2005).
    • (2005) Science , vol.307 , pp. 1262
    • Young, D.T.1
  • 21
    • 14544286615 scopus 로고    scopus 로고
    • note
    • The gas detection threshold is based on a minimum 2σ detectable level of 10 counts above background, instrument sensitivity at 130.4 nm of 3.4 cts/kR-s, integration time of ∼0 hours, and solar-wind values for the electron density and temperature at Saturn.
  • 35
    • 14544282626 scopus 로고    scopus 로고
    • note
    • Thanks to H. Tollerud for assistance with data processing, L. Bloom for producing the manuscript, and J. Cuzzi and the anonymous reviewers for helpful comments. This work is one part of the Cassini UVIS investigation, supported by the NASA Jet Propulsion Laboratory Cassini mission.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.