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Volumn 318, Issue 5856, 2007, Pages 1582-1585

Fine thermal structure of a coronal active region

Author keywords

[No Author keywords available]

Indexed keywords

CORONA; HEATING; SIGNAL-TO-NOISE RATIO; SOLAR ACTIVITY; THERMAL STRUCTURE;

EID: 36849071401     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1146590     Document Type: Article
Times cited : (33)

References (13)
  • 9
    • 34848836404 scopus 로고    scopus 로고
    • L. Golub et al., Solar Phys. 243, 63 (2007).
    • (2007) Solar Phys , vol.243 , pp. 63
    • Golub, L.1
  • 13
    • 36849044574 scopus 로고    scopus 로고
    • Hinode is a Japanese mission developed and launched by the Institute of Space and Astronautical Science/Japan Aerospace Exploration Agency, with the National Astronomical Observatory of Japan as domestic partner and NASA and Science and Technology Facilities Council (UK) as international partners. It is operated by these agencies in cooperation with the European Space Agency (ESA) and the Norwegian Space Centre (Norway, F.R, G.P, and M.B. acknowledge support from Italian Ministero dell'Università e Ricerca and Agenzia Spaziale Italiana (ASI, under contracts I/035/05/0 and I/015/07/0. U. S. members of the XRT team are supported by NASA contract NNM07AA02C to the Smithsonian Astrophysical Observatory, S.P. acknowledges support from the Belgian Federal Science Policy Office through the ESA-Programme de Développement d'Experiences scientifiques program. This work was partially supported by the International Space Science Institute in the framework of an international wo
    • Hinode is a Japanese mission developed and launched by the Institute of Space and Astronautical Science/Japan Aerospace Exploration Agency, with the National Astronomical Observatory of Japan as domestic partner and NASA and Science and Technology Facilities Council (UK) as international partners. It is operated by these agencies in cooperation with the European Space Agency (ESA) and the Norwegian Space Centre (Norway). F.R., G.P., and M.B. acknowledge support from Italian Ministero dell'Università e Ricerca and Agenzia Spaziale Italiana (ASI), under contracts I/035/05/0 and I/015/07/0. U. S. members of the XRT team are supported by NASA contract NNM07AA02C (to the Smithsonian Astrophysical Observatory). S.P. acknowledges support from the Belgian Federal Science Policy Office through the ESA-Programme de Développement d'Experiences scientifiques program. This work was partially supported by the International Space Science Institute in the framework of an international working team.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.