Solar energetic particles, or SEPs, from suprathermal (few keV) up to relativistic (∼∼ few
GeV) energies are accelerated near the Sun in at least two ways:(1) by magnetic …

Evidence for two different physical mechanisms for acceleration of solar energetic particles
(SEPs) arose 50 years ago with radio observations of type III bursts, produced by outward …

Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global
challenge in the field of heliophysics, in that such a study, if it were to be performed from first …

Nonlinear Collisionless Perpendicular Diffusion Of Charged Particles Page 1 Florida
Institute of Technology Scholarship Repository @ Florida Tech Aerospace, Physics, and …

It is argued here that the inner heliosphere is filled with a network of entangled magnetic flux
tubes and that the flux tubes are fossil structures that originate at the solar surface. 65,860 …

An overview is given of important properties of spatial and temporal intermittency, including
evidence of its appearance in fluids, magnetofluids and plasmas, and its implications for …

Abstract The Integrated Science Investigation of the Sun (ISIS) is a complete science
investigation on the Solar Probe Plus (SPP) mission, which flies to within nine solar radii of …

Using observations from the High Energy Telescopes (HETs) on the STEREO A and B
spacecraft and similar observations from near-Earth spacecraft, we summarize the …

Above a few tens of MeV per nucleon, large, gradual solar energetic particle (SEP) events
are highly variable in their spectral characteristics and elemental composition. The origin of …

Abstract Solar Energetic Particles (SEPs) are an important component of Space Weather,
including radiation hazard to humans and electronic equipment, and the ionisation of the …