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Volumn 285, Issue 5429, 1999, Pages 862-864

Trace observation of damped coronal loop oscillations: Implications for coronal heating

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; HEAT; OSCILLATION; PRIORITY JOURNAL; SPACE FLIGHT; SUN;

EID: 0033529530     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.285.5429.862     Document Type: Article
Times cited : (1004)

References (30)
  • 1
    • 0344141357 scopus 로고    scopus 로고
    • note
    • XV), and between 1200 and 7000 Å. Focal plane filters allow TRACE to select ultraviolet passbands around Lyman-α (1216 Å), C IV (1550 Å), the ultraviolet continuum at 1600 A and 1700 A, and the visible continuum up to 7000 A wavelengths (26). Additional detail on the TRACE spacecraft can be found in Handy et al. (27) and at http://vestige.Imsal.com/TRACE/. First results from the TRACE mission are reported by Schrijver et al. (28) and by Golub et al. (29).
  • 3
    • 0001684909 scopus 로고
    • _, Astrophys. J. 279, 857 (1984).
    • (1984) Astrophys. J. , vol.279 , pp. 857
  • 12
    • 0344572814 scopus 로고    scopus 로고
    • A movie made from these Images Is available as supplementary material
    • A movie made from these Images Is available as supplementary material at www.sciencemag.org/feature/ data/1040166.shl.
  • 26
    • 0344572809 scopus 로고    scopus 로고
    • note
    • The optics contains an active secondary mirror with image motion compensation. Pointing is internally stabilized to 0.1 arc sec against spacecraft jitters. A 1024 by 1024 charge-coupled device (CCD) detector collects images over an 8.5 arc min by 8.5 arc min field-of-view. A powerful data handling computer enables flexible use of the CCD array including adaptive target selection, data compression, and fast operation for a limited field-of-view.
  • 30
    • 0344141348 scopus 로고    scopus 로고
    • note
    • We thank the TRACE team. LO. acknowledges support by the NASA Solar Physics Supporting Research and Technology program, the NASA Space Physics Theory Program, and the NASA High-Performance Computing and Communications program. E.E.D. was supported by contract MASS-38099 with NASA Goddard Space Flight Center. V.M.N. and B.R. acknowledge Particle Physics and Astronomy Research Council support.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.