Physical Review Letters · 1974 · 42 citations · 10 references
EngineeringNuclear PhysicsLaser-plasma InteractionRelativistic PlasmaPlasma SciencePlasma PhysicsEmitted Line RadiationPlasma TheoryPlasma SimulationMagnetohydrodynamicsIonized Helium PlasmaPlasma ConfinementPhysicsApplied Plasma PhysicAtomic PhysicsTotal Energy DepositionNatural SciencesApplied PhysicsRelativistic Electron Beams
A partially ionized helium plasma (${n}_{e}=5\ifmmode\times\else\texttimes\fi{}{10}^{13}$ ${\mathrm{cm}}^{\ensuremath{-}3}$) was heated by an intense ($\frac{\ensuremath{\nu}}{\ensuremath{\gamma}}\ensuremath{\simeq}1$) relativistic electron beam (600 keV, 25-60 kA). Observations of the emitted line radiation and Thomson-scattered light indicate noncollisional electron heating rates consistent with electron-ion instability predictions, and total energy deposition consistent with electron-electron- instability saturation levels.
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Rate of Collisional Excitation in Stellar Atmospheres.
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