Non-linear amplification of a magnetic field driven by cosmic ray streaming

Non-linear amplification of a magnetic field driven by cosmic ray streaming

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Manylion Llyfryddiaeth
Prif Awduron:	Lucek, S, Bell, A
Fformat:	Conference item
Cyhoeddwyd:	2000

Eitemau Tebyg

Non-linear amplification of a magnetic field driven by cosmic ray streaming
gan: Lucek, S, et al.
Cyhoeddwyd: (2000)

Cosmic ray acceleration to very high energy through the non-linear amplification by cosmic rays of the seed magnetic field
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COSMIC-RAY ACCELERATION IN INHOMOGENEOUS MAGNETIC-FIELDS ABOUT RELATIVISTIC SHOCKS
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Magnetic field amplification by cosmic rays in supernova remnants
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Amplification of perpendicular and parallel magnetic fields by cosmic ray currents
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Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays
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Cosmic ray acceleration in pulsar-driven supernova remnants: The effect of scattering
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Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
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The nonlinear amplification of magnetic fields by cosmic rays at supernova remnant shocks
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A filamentation instability for streaming cosmic rays
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A filamentation instability for streaming cosmic rays
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The interaction of cosmic rays and magnetized plasma
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A three-phase amplification of the cosmic magnetic field in galaxies
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COSMIC-RAY ACCELERATION IN PULSAR-DRIVEN SUPERNOVA-REMNANTS
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Cosmic ray propagation in turbulent magnetic fields
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Interplanetary magnetic field fluctuations and the propagation of cosmic rays
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A Model for Cosmic Magnetic Field Amplification: Effects of Pressure Anisotropy Perturbations
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Cosmic ray acceleration
gan: Bell, A
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Towards extracting cosmic magnetic field structures from cosmic-ray arrival directions
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Evolution of magnetic fields and cosmic ray acceleration in supernova remnants
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Intercluster magnetic fields and ultra high energy cosmic rays
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Resistive Magnetic Field Generation at Cosmic Dawn
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Magnetic field amplification in strong shocks
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Cosmic Ray Diffusion in Magnetic Fields Amplified by Nonlinear Turbulent Dynamo
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The stability, during formation, of magnetohydrodynamic jets collimated by an azimuthal magnetic field
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Sidereal cosmic ray variation and its relation with the interplanetary magnetic field polarity.
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Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory
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Reacceleration of Galactic Cosmic Rays beyond the Knee at the Termination Shock of a Cosmic-Ray-driven Galactic Wind
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Confining the high-energy cosmic rays
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Confining the high-energy cosmic rays
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Precise mapping of the magnetic field in the CMS barrel yoke using cosmic rays
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Precise mapping of the magnetic field in the CMS barrel yoke using cosmic rays
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Precise mapping of the magnetic field in the CMS barrel yoke using cosmic rays
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Understanding Streaming Instabilities in the Limit of High Cosmic-Ray Current Density
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Ion alfvén velocity fluctuations and implications for the diffusion of streaming cosmic rays
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Implications of strong intergalactic magnetic fields for ultrahigh-energy cosmic-ray astronomy
gan: Batista, R, et al.
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ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .1.
gan: Bell, A
Cyhoeddwyd: (1978)

ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .2.
gan: Bell, A
Cyhoeddwyd: (1978)

Cosmic ray acceleration at oblique shocks
gan: Bell, A, et al.
Cyhoeddwyd: (2011)

Cosmic ray acceleration at oblique shocks
gan: Bell, A, et al.
Cyhoeddwyd: (2011)