Fermi acceleration
Fermi acceleration, sometimes referred to as diffusive shock acceleration (a subclass of Fermi acceleration ), is the acceleration that charged particles undergo when being repeatedly reflected, usually by a magnetic mirror (see also Centrifugal mechanism of acceleration). This is thought to be the primary mechanism by which particles gain non thermal energies in astrophysical shock waves. It plays a very important role in many astrophysical models, mainly of shocks including solar flares and supernova remnants.
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Fermi acceleration
Fermi acceleration, sometimes referred to as diffusive shock acceleration (a subclass of Fermi acceleration ), is the acceleration that charged particles undergo when being repeatedly reflected, usually by a magnetic mirror (see also Centrifugal mechanism of acceleration). This is thought to be the primary mechanism by which particles gain non thermal energies in astrophysical shock waves. It plays a very important role in many astrophysical models, mainly of shocks including solar flares and supernova remnants.
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En physique, l'accélération de ...... t les rémanents de supernovae.
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Fermi acceleration, sometimes ...... lt no acceleration will occur.
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Przyspieszenie Fermiego – proc ...... tycznych promieni kosmicznych.
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En physique, l'accélération de ...... t les rémanents de supernovae.
@fr
Fermi acceleration, sometimes ...... flares and supernova remnants.
@en
Przyspieszenie Fermiego – proc ...... du oraz proces drugiego rzędu.
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Accélération de Fermi
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Fermi acceleration
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Przyspieszenie Fermiego
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