Structure function scaling in compressible super-alfvénic MHD turbulence

Physical Review Letters

Volumn 92, Issue 19, 2004, Pages

  Padoan, Paolo ^a   Jimenez, Raul ^b   Nordlund, Åke ^c   Boldyrev, Stanislav ^d  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF PENNSYLVANIA   (United States)

^c THEORETICAL ASTROPHYSICS CENTER   (Denmark)

^d UNIVERSITY OF CHICAGO   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; CLOUDS; COMPUTER SIMULATION; FUNCTIONS; GALAXIES; INCOMPRESSIBLE FLOW; MAGNETIZATION; MATHEMATICAL MODELS; SHOCK WAVES; SUPERSONIC FLOW; TURBULENCE;

DISSIPATIVE STRUCTURES; STAR FORMATION; STRUCTURE FUNCTION SCALING; SUPERSONIC TURBULENCE;

TURBULENT FLOW;

EID: 4644310941     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.92.191102     Document Type: Article

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