Comparing numerical methods for isothermal magnetized supersonic turbulence

Astrophysical Journal

Volumn 737, Issue 1, 2011, Pages

  Kritsuk, Alexei G ^a,b   Nordlund, Åke ^b,c   Collins, David ^a,b,d   Padoan, Paolo ^b,e   Norman, Michael L ^a,f   Abel, Tom ^b,g   Banerjee, Robi ^b,c,i   Federrath, Christoph ^h,i,j   Flock, Mario ^j,k   Lee, Dongwook ^l   Shing Li, Pak ^b,m   Müller, Wolf Christian ⁿ   Teyssier, Romain ^b,o,p   Ustyugov, Sergey D ^q   Vogel, Christian ⁿ   Xu, Hao ^a,c  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF COPENHAGEN   (Denmark)

^d LOS ALAMOS NATIONAL LABORATORY   (United States)

^e UNIVERSITY OF BARCELONA   (Spain)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g STANFORD UNIVERSITY   (United States)

^h UNIVERSITY OF HEIDELBERG   (Germany)

ⁱ UNIVERSITY OF HAMBURG   (Germany)

^j MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^k CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^l University of Chicago   (United States)

^m UNIVERSITY OF CALIFORNIA   (United States)

ⁿ MAX PLANCK INSTITUT FÜR PLASMAPHYSIK   (Germany)

^o CEA SACLAY   (France)

^p UNIVERSITY OF ZURICH   (Switzerland)

^q KELDYSH INSTITUTE OF APPLIED MATHEMATICS   (Russian Federation)

more..

Author keywords

ISM: structure; magnetohydrodamics (MHD); methods: numerical; turbulence

Indexed keywords

EID: 80052049287     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/737/1/13     Document Type: Article

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