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Volumn 6, Issue 5 I, 1999, Pages 2217-2224

Magnetohydrodynamic modeling of the global solar corona

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0013233748     PISSN: 1070664X     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.873474     Document Type: Article
Times cited : (360)

References (53)
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    • edited by K. S. Balasubramaniam, S. L. Keil, and R. N. Smartt Astronomical Society of the Pacific, Conf. Series
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    • (1996) Solar Drivers of Interplanetary and Terrestrial Disturbances , vol.95 , pp. 208
    • Linker, J.A.1    Mikić, Z.2    Schnack, D.D.3
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    • 0009699097 scopus 로고    scopus 로고
    • edited by N. Crooker, J. Joselyn, and J. Feynman American Geophysical Union. Washington DC. Geophys. Monograph 99
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    • (1997) Coronal Mass Ejections , pp. 57
    • Mikić, Z.1    Linker, J.A.2
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    • 0041318707 scopus 로고    scopus 로고
    • edited by N. Crooker, J. Joselyn, and J. Feynman American Geophysical Union. Washington DC, Geophys. Monograph 99
    • J. A. Linker and Z. Mikić, Coronal Mass Ejections, edited by N. Crooker, J. Joselyn, and J. Feynman (American Geophysical Union. Washington DC, 1997), Geophys. Monograph 99, p. 269.
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    • edited by D. Winterhalter, J. T. Gosling, S. R. Habbal, W. S. Kurth, and M. Neugebauer American Institute of Physics, Woodbury, NY, Conf. Proc.
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    • A composite MHD model of an expanding corona and its application to the Whole Sun Month campaign
    • submitted
    • Y. V. Pisanko, "A composite MHD model of an expanding corona and its application to the Whole Sun Month campaign," J. Geophys. Res. (submitted).
    • J. Geophys. Res.
    • Pisanko, Y.V.1
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    • Ph.D. thesis, Gottingen University
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    • note
    • This simulation took 65 h of CPU time on a single processor of the Cray-T90 supercomputer. A real-time solution would take about 10 times longer. It may be possible to perform a real-time simulation once our code is ported to a massively parallel computer.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.