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- Fermi_acceleration abstract "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. 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. There are two types of Fermi acceleration: first-order Fermi acceleration (in shocks) and second-order Fermi acceleration (in the environment of moving magnetized gas clouds). In both cases the environment has to be collisionless in order for the mechanism to be effective. This is because Fermi acceleration only applies to particles with energies exceeding the thermal energies, and frequent collisions with surrounding particles will cause severe energy loss and as a result no acceleration will occur.".
- Fermi_acceleration wikiPageExternalLink 0610141.
- Fermi_acceleration wikiPageExternalLink books?id=tNDgb-U9PLMC&printsec=frontcover.
- Fermi_acceleration wikiPageExternalLink Fermi_acceleration.html.
- Fermi_acceleration wikiPageID "3035156".
- Fermi_acceleration wikiPageRevisionID "602293630".
- Fermi_acceleration hasPhotoCollection Fermi_acceleration.
- Fermi_acceleration subject Category:Acceleration.
- Fermi_acceleration subject Category:Cosmic_rays.
- Fermi_acceleration subject Category:Dynamics.
- Fermi_acceleration subject Category:Enrico_Fermi.
- Fermi_acceleration subject Category:Fusion_power.
- Fermi_acceleration subject Category:Physical_quantities.
- Fermi_acceleration type Abstraction100002137.
- Fermi_acceleration type Measure100033615.
- Fermi_acceleration type PhysicalQuantities.
- Fermi_acceleration comment "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. 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.".
- Fermi_acceleration label "Accélération de Fermi".
- Fermi_acceleration label "Fermi acceleration".
- Fermi_acceleration label "Przyspieszenie Fermiego".
- Fermi_acceleration sameAs Accélération_de_Fermi.
- Fermi_acceleration sameAs Przyspieszenie_Fermiego.
- Fermi_acceleration sameAs m.08m426.
- Fermi_acceleration sameAs Q2822925.
- Fermi_acceleration sameAs Q2822925.
- Fermi_acceleration sameAs Fermi_acceleration.
- Fermi_acceleration wasDerivedFrom Fermi_acceleration?oldid=602293630.
- Fermi_acceleration isPrimaryTopicOf Fermi_acceleration.