Search results for "Astrophysical plasmas"

showing 2 items of 2 documents

Efficient generation of energetic ions in multi-ion plasmas by radio-frequency heating

2017

We describe a new technique for the efficient generation of high-energy ions with electromagnetic ion cyclotron waves in multi-ion plasmas. The discussed ‘three-ion’ scenarios are especially suited for strong wave absorption by a very low number of resonant ions. To observe this effect, the plasma composition has to be properly adjusted, as prescribed by theory. We demonstrate the potential of the method on the world-largest plasma magnetic confinement device, JET (Joint European Torus, Culham, UK), and the high-magnetic-field tokamak Alcator C-Mod (Cambridge, USA). The obtained results demonstrate efficient acceleration of 3He ions to high energies in dedicated hydrogen–deuterium mixtures.…

Astrophysical plasmasTokamakradio-frequency heatingCyclotronJoint European TorusPlasma heatingGeneral Physics and AstronomyFREQUENCY114 Physical sciences01 natural sciences7. Clean energyMagnetically confined plasmas010305 fluids & plasmaslaw.inventionIonPHYSICSPhysics and Astronomy (all)FUSIONMODE CONVERSIONlawPhysics::Plasma Physics0103 physical sciencesDielectric heating010306 general physicsPhysics[PHYS]Physics [physics]ta114Solar flare:Física [Àrees temàtiques de la UPC]Plasma dynamicsmulti-ion plasmasSettore FIS/01 - Fisica SperimentaleMagnetic confinement fusionPlasmaHE-3-RICH SOLAR-FLARESTècniques de plasmaJETCYCLOTRON RANGETOKAMAKPhysics::Space PhysicsAtomic physicsHE-3-RICH SOLAR-FLARES; MODE CONVERSION; CYCLOTRON RANGE; FUSION; JET; FREQUENCY; TOKAMAK; PHYSICS
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The supernova remnant SN 1006 as a Galactic particle accelerator

2022

The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants are strong candidates to be the Galactic factory of cosmic rays, their blast waves being powerful particle accelerators. However, supernova remnants can power the observed flux of cosmic rays only if they transfer a significant fraction of their kinetic energy to the accelerated particles, but conclusive evidence for such efficient acceleration is still lacking. In this scenario, the shock energy channeled to cosmic rays should induce a higher post-shock density than that predicted by standard shock conditions. Here we show this effect, and probe its dependence on the orientation of the ambient…

High Energy Astrophysical Phenomena (astro-ph.HE)Astrophysical plasmasSHARPHorizon 2020MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomyshock wavesGeneral ChemistryGeneral Biochemistry Genetics and Molecular BiologyHigh-energy astrophysicsSettore FIS/05 - Astronomia E AstrofisicaEuropean Union (EU)Particle astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomenacosmic rayNature Communications
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