Add to ORKGAcceleration of electrons by Langmuir plasma turbulence and by the Fermi mechanism are suggested to explain the two-stage acceleration processes observed in hard X-rays from solar flares. A model for particle acceleration in flares is presented
Combining in situ measurements of energetic electrons and remote sensing observations of hard X‐rays...
Context. Theoretical models and spacecraft observations of solar flares highlight the role of wave-p...
Solar flares are among the most energetic and interesting phenomena in the Solar system, releasing u...
Solar flares often accelerate ions and electrons to relativistic energies. The details of the accele...
It is proposed that particles during the second phase of solar flares are accelerated by stochastic ...
The electric field acceleration of electrons out of a thermal plasma and the simultaneous Joule heat...
We present a model for the acceleration of electrons from thermal to ultrarelativistic energies duri...
One of the outstanding problems in solar flare theory is how to explain the 10-20 keV and greater ha...
The acceleration of a huge number of electrons and ions to relativistic energies over timescales ran...
We present a model for high-energy solar flares to explain prompt proton and electron acceleration, ...
Energetic solar flare particles, both electrons and protons, must survive the turbulent environment ...
One-dimensional, electrostatic, particle-in-cell simulations are used to explore two mechanisms prop...
The most direct signatures of particle acceleration in flares are energetic particles detected in in...
We use RHESSI hard X-ray observations to constrain acceleration of solar flare electrons, generally ...
Two-dimensional (three velocity) electrostatic particle simulations are used to investigate the part...
Combining in situ measurements of energetic electrons and remote sensing observations of hard X‐rays...
Context. Theoretical models and spacecraft observations of solar flares highlight the role of wave-p...
Solar flares are among the most energetic and interesting phenomena in the Solar system, releasing u...
Solar flares often accelerate ions and electrons to relativistic energies. The details of the accele...
It is proposed that particles during the second phase of solar flares are accelerated by stochastic ...
The electric field acceleration of electrons out of a thermal plasma and the simultaneous Joule heat...
We present a model for the acceleration of electrons from thermal to ultrarelativistic energies duri...
One of the outstanding problems in solar flare theory is how to explain the 10-20 keV and greater ha...
The acceleration of a huge number of electrons and ions to relativistic energies over timescales ran...
We present a model for high-energy solar flares to explain prompt proton and electron acceleration, ...
Energetic solar flare particles, both electrons and protons, must survive the turbulent environment ...
One-dimensional, electrostatic, particle-in-cell simulations are used to explore two mechanisms prop...
The most direct signatures of particle acceleration in flares are energetic particles detected in in...
We use RHESSI hard X-ray observations to constrain acceleration of solar flare electrons, generally ...
Two-dimensional (three velocity) electrostatic particle simulations are used to investigate the part...
Combining in situ measurements of energetic electrons and remote sensing observations of hard X‐rays...
Context. Theoretical models and spacecraft observations of solar flares highlight the role of wave-p...
Solar flares are among the most energetic and interesting phenomena in the Solar system, releasing u...