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Volumn 13, Issue 6, 2006, Pages

Modeling of the turbulent magnetohydrodynamic residual-energy equation using a statistical theory

Author keywords

[No Author keywords available]

Indexed keywords

FLUID DYNAMICS; MAGNETIC FIELDS; SHEAR FLOW; SOLAR RADIATION; STATISTICAL METHODS; TURBULENCE;

EID: 33745725476     PISSN: 1070664X     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.2209232     Document Type: Article
Times cited : (21)

References (42)
  • 24
    • 0005494952 scopus 로고
    • edited by J.-P. Zahn and J. Zinn-Justin (Elsevier Science, Amsterdam, The Netherlands)
    • P. H. Roberts, in Astrophysical Fluid Dynamics, edited by J.-P. Zahn and J. Zinn-Justin (Elsevier Science, Amsterdam, The Netherlands, 1980), p. 229.
    • (1980) Astrophysical Fluid Dynamics , pp. 229
    • Roberts, P.H.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.