메뉴 건너뛰기




Volumn 319, Issue 5859, 2008, Pages 79-81

Temperature and composition of Saturn's polar hot spots and hexagon

Author keywords

[No Author keywords available]

Indexed keywords

PHOSPHINE;

EID: 37849001831     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1149514     Document Type: Article
Times cited : (119)

References (25)
  • 5
    • 34447257917 scopus 로고    scopus 로고
    • L. N. Fletcher et al., Icarus 189, 457 (2007).
    • (2007) Icarus , vol.189 , pp. 457
    • Fletcher, L.N.1
  • 8
    • 37849048326 scopus 로고    scopus 로고
    • Materials and methods are available as supporting material on Science Online.
    • Materials and methods are available as supporting material on Science Online.
  • 12
  • 13
    • 7444253401 scopus 로고    scopus 로고
    • P. G. J. Irwin et al., Icarus 172, 37 (2004).
    • (2004) Icarus , vol.172 , pp. 37
    • Irwin, P.G.J.1
  • 17
    • 0040186657 scopus 로고
    • B. A. Smith et al., Science 215, 504 (1982).
    • (1982) Science , vol.215 , pp. 504
    • Smith, B.A.1
  • 20
    • 34247488340 scopus 로고    scopus 로고
    • D. A. Gurnett et al., Science 316, 442 (2007).
    • (2007) Science , vol.316 , pp. 442
    • Gurnett, D.A.1
  • 25
    • 37849015656 scopus 로고    scopus 로고
    • This work was carried out at the Atmospheric, Oceanic, and Planetary Physics Department at the University of Oxford. The UK authors acknowledge the support of the Science and Technology Facilities Council. We acknowledge the members of the Cassini and CIRS investigation teams involved in the building, testing, and calibration of the instrument, along with the design of imaging sequences, instrument commands, and other vital operational tasks. The authors also thank K. Baines, M. Roos-Serote, A. Aguiar, Y. H. Yamazaki, and R. Wordsworth for their helpful comments and suggestions
    • This work was carried out at the Atmospheric, Oceanic, and Planetary Physics Department at the University of Oxford. The UK authors acknowledge the support of the Science and Technology Facilities Council. We acknowledge the members of the Cassini and CIRS investigation teams involved in the building, testing, and calibration of the instrument, along with the design of imaging sequences, instrument commands, and other vital operational tasks. The authors also thank K. Baines, M. Roos-Serote, A. Aguiar, Y. H. Yamazaki, and R. Wordsworth for their helpful comments and suggestions.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.