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Volumn 318, Issue 5848, 2007, Pages 237-240

Io's atmospheric response to eclipse: UV aurorae observations

Author keywords

[No Author keywords available]

Indexed keywords

AURORA; ELECTRODYNAMICS; IMAGING METHOD; JUPITER; MAGNETOSPHERE; SUBLIMATION; ULTRAVIOLET RADIATION; VOLCANO;

EID: 35348928119     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1147594     Document Type: Article
Times cited : (40)

References (31)
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    • The angular size of Io varies with spacecraft distance but is smaller than the Alice slit width for these data. The spectral resolution varies between 0.3 nm and ∼0.9 nm for emissions known to be located near the satellite disk 22, see, e.g, Fig. 2
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    • We thank the New Horizons mission and science teams. New Horizons is funded by NASA. Support for this work was also provided by NASA though grant number GO-10871 from the Space Telescope Science Institute STScI, which is operated by the Association of Universities for Research in Astronomy, Inc, under NASA contract NAS5-26555
    • We thank the New Horizons mission and science teams. New Horizons is funded by NASA. Support for this work was also provided by NASA though grant number GO-10871 from the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.