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Volumn 418, Issue 6900, 2002, Pages 853-856

A wind origin for Titan’s haze structure

Author keywords

[No Author keywords available]

Indexed keywords

ATMOSPHERIC MOVEMENTS; COMPUTER SIMULATION; MOON; NITROGEN; PRECIPITATION (METEOROLOGY);

EID: 0037158716     PISSN: 00280836     EISSN: None     Source Type: Journal    
DOI: 10.1038/nature00961     Document Type: Article
Times cited : (106)

References (28)
  • 1
    • 0001065603 scopus 로고
    • Titan's atmosphere and hypothesis ocean: A re-analysis of the Voyager 1 radio-occultation and IRIS 7.7-μm data
    • (1989) Icarus , vol.79 , pp. 328-349
    • Lellouch, E.1
  • 2
    • 0000409082 scopus 로고
    • Implication of Titan's north-south brightness asymmetry
    • (1981) Nature , vol.292 , pp. 698-702
    • Sromovsky, L.A.1
  • 3
    • 0029381384 scopus 로고
    • Numerical simulation of the general circulation of the atmosphere of Titan
    • (1995) Icarus , vol.117 , pp. 358-374
    • Hourdin, F.1
  • 8
    • 0035735465 scopus 로고    scopus 로고
    • Images of Titan at 1.3 and 1.6 micron with adaptative optics at the CFHT
    • (2002) Icarus , vol.154 , pp. 501-515
    • Coustenis, A.1
  • 12
    • 0001801381 scopus 로고
    • Titan's atmosphere from Voyager infrared observations: IV. Latitudinal variations of temperature and composition
    • (1995) Icarus , vol.115 , pp. 126-140
    • Coustenis, A.1    Bézard, B.2
  • 15
    • 0001654021 scopus 로고
    • Optical constants of organic tholins produced in a simulated Titanian atmosphere: From soft X-ray to microwave frequencies
    • (1984) Icarus , vol.60 , pp. 127-137
    • Khare, B.N.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.