… accelerated particles, but how were they accelerated and why should they have a power
law spectrum? The advantage of the alternative microscopic derivation (Bell 1978a, see also …

… driven accelerating fronts … particle acceleration that are thought to operate at the Sun, and
in Sect. 4 we discuss the links and timings between remote sensing signatures of acceleration …

… -encounter energetic particle acceleration is compression at the shock. Particles are scattered
… Accordingly, shock acceleration is included in Equation (2) if we simply take V to change …

… the impulsive and gradual solar energetic particle (SEP) events. … However, we have no such
images of solar energetic particles (… Solar energetic particles (SEPs) come as bursts of high-…

… roles of stochastic acceleration by random electric field and plasma motion in the production
and transport of energetic particles in the heliosphere. Stochastic acceleration can occur in …

… -dependent transport of energetic particles accelerated at a … our previous work on particle
acceleration at shocks, allows … , particle anisotropies) of high-energy particles arriving at …

… This paper describes the instruments which make up the Energetic Particles: Acceleration, …
Particle collection power has been increased by factors up to 100, while the telemetry bit-…

… It is well established that energetic particles (energies `~ 1 MeV per nucleon) are
accelerated in association with … The accelerated energetic particles are seen in two …

… respect to the acceleration of energetic particles from the ambient solar wind by an
interplanetary shock. The time-intensity profiles are derived from the Helio 1 particle data base for …

… Magnitude fluctuations should be a continuous source of energy for accelerating energetic
particles because these fluctuatiohs are continuously regenerated. For example, Alfv6n …