Postshock turbulence and diffusive shock acceleration in young supernova remnants

Astronomy and Astrophysics

Volumn 515, Issue 11, 2010, Pages

  Marcowith, A ^a   Casse, F ^b  

^a UNIVERSITÉ MONTPELLIER II   (France)

^b UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

Acceleration of particles; ISM: supernova remnants; Magnetohydrodynamics (MHD); Shock waves

Indexed keywords

ACCELERATION; AMPLIFICATION; ASTRONOMY; COSMOLOGY; DAMPING; DIFFERENTIAL EQUATIONS; DIFFERENTIATION (CALCULUS); FILAMENTS (LAMP); MAGNETIC FIELDS; MAGNETIC MATERIALS; MAGNETOHYDRODYNAMICS; PARTICLE ACCELERATOR ACCESSORIES; PARTICLE ACCELERATORS; RELAXATION PROCESSES; SHOCK WAVES; STOCHASTIC MODELS; STOCHASTIC SYSTEMS; TURBULENCE; WAVES; X RAYS;

ACCELERATION OF PARTICLES; BLAST WAVES; DIFFUSIVE SHOCK ACCELERATIONS; FERMI ACCELERATION; INVERSE COMPTON; ISM: SUPERNOVA REMNANTS; KOLMOGOROV; MAGNETIC FIELD AMPLITUDES; MAGNETIC FLUCTUATION; MAGNETO-HYDRODYNAMICS SIMULATIONS; MAGNETOHYDRODYNAMICS (MHD); MAGNETOSONIC MODE; MULTIWAVELENGTH; NON-LINEAR; NONRESONANT; NUMERICAL CALCULATION; OBSERVATIONAL DATA; PARTICLE ACCELERATION; POWER LAW INDEX; RADIATIVE LOSS; RADIATIVE SIGNATURE; RE-ACCELERATION; RELAXATION LENGTH; RELAXATION MODELS; RESONANT MODE; SECOND ORDERS; SHOCK FRONTS; SHOCK REGION; SPECTRAL INDICES; STOCHASTIC DIFFERENTIAL EQUATIONS; SUPERNOVA REMNANTS; TEST PARTICLES; UPPER LIMITS; X-RAY FILAMENTS;

MAGNETIC BUBBLES;

EID: 77953642419     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913022     Document Type: Article

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