MHD simulations of the dynamics of sharp disturbances of the interplanetary medium and comparison with spacecraft observations

Cosmic Research

Volumn 41, Issue 6, 2003, Pages 529-538

  Barkhatov, N A ^a   Korolev, A V ^a   Zastenker, G N ^b   Ryazantseva, M O ^b,c   Dalin, P A ^b  

^a MININ NIZHNY NOVGOROD STATE PEDAGOGICAL UNIVERSITY   (Russian Federation)

^b Russian Academy of Sciences   (Russian Federation)

^c MOSCOW STATE UNIVERSITY   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

APPROXIMATION THEORY; COMPUTER PROGRAMMING; COMPUTER SIMULATION; EARTH ATMOSPHERE; ENTROPY; HEAT TRANSFER; INTERPLANETARY SPACECRAFT; KINETIC THEORY OF GASES; MAGNETIC FIELD EFFECTS; MATHEMATICAL MODELS; NUMERICAL ANALYSIS; PARAMETER ESTIMATION; PLASMA DENSITY; REYNOLDS NUMBER; SUN;

COMPUTER CODES; INTERPLANETARY MAGNETIC FIELDS (IMF); POLYTROPIC GAS; THERMAL PRESSURES;

MAGNETOHYDRODYNAMICS;

EID: 3543059985     PISSN: 00109525     EISSN: None     Source Type: Journal    
DOI: 10.1023/B:COSM.0000007951.49454.8a     Document Type: Article

References (10)

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