Add to ORKGWe use RHESSI hard X-ray observations to constrain acceleration of solar flare electrons, generally considered to be a primary recipient of the released energ
Context: Solar flares release a large fraction of their energy into non-thermal electrons, but it is...
Combining in situ measurements of energetic electrons and remote sensing observations of hard X‐rays...
High-energy X-rays and γ-rays from solar flares were discovered just over fifty years ago. Since tha...
Observations with RHESSI have enabled the detailed study of the structure of dense hard X-ray corona...
Knowledge of the energy distribution of electrons accelerated in solar flares is important for const...
Solar flares are huge explosions on the Sun that release a tremendous amount of energy from the coro...
Context: Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
A popular scenario for electron acceleration in solar flares is transit-time damping of low-frequenc...
Solar flares are known to accelerate electrons to high energies, resulting in the movement of these ...
The imaging spectroscopy capabilities of the Reuven Ramaty high energy solar spectroscopic imager (R...
Aims. We aim to constrain the acceleration, injection, and transport processes of flare-accelerated ...
Context. Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
Observations with RHESSI have enabled the detailed study of the structure of dense hard X-ray corona...
Context.Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
Solar flares are known to accelerate electrons to high energies, resulting in the movement of these ...
Context: Solar flares release a large fraction of their energy into non-thermal electrons, but it is...
Combining in situ measurements of energetic electrons and remote sensing observations of hard X‐rays...
High-energy X-rays and γ-rays from solar flares were discovered just over fifty years ago. Since tha...
Observations with RHESSI have enabled the detailed study of the structure of dense hard X-ray corona...
Knowledge of the energy distribution of electrons accelerated in solar flares is important for const...
Solar flares are huge explosions on the Sun that release a tremendous amount of energy from the coro...
Context: Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
A popular scenario for electron acceleration in solar flares is transit-time damping of low-frequenc...
Solar flares are known to accelerate electrons to high energies, resulting in the movement of these ...
The imaging spectroscopy capabilities of the Reuven Ramaty high energy solar spectroscopic imager (R...
Aims. We aim to constrain the acceleration, injection, and transport processes of flare-accelerated ...
Context. Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
Observations with RHESSI have enabled the detailed study of the structure of dense hard X-ray corona...
Context.Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
Solar flares are known to accelerate electrons to high energies, resulting in the movement of these ...
Context: Solar flares release a large fraction of their energy into non-thermal electrons, but it is...
Combining in situ measurements of energetic electrons and remote sensing observations of hard X‐rays...
High-energy X-rays and γ-rays from solar flares were discovered just over fifty years ago. Since tha...