Add to ORKGHard X-ray and microwave modelling that takes into account the temporal evolution of the electron spectrum as well as the inhomogeneity of the magnetic field and the ambient medium in the radio source is presented. This method is illustrated for the June 29 1980 10:41 UT event. The implication on the process of acceleration/injection is discussed
Knowledge of the energy distribution of electrons accelerated in solar flares is important for const...
Aims. We aim to constrain the acceleration, injection, and transport processes of flare-accelerated ...
A large fraction of the energy released during solar flares is carried by accelerated electrons and ...
The evolution of accelerated particle distributions in a magnetized plasma and the resulting radiati...
The joint study of hard x ray and microwave observations of solar flares is extremely important beca...
Recently, in a few case studies we demonstrated that gyrosynchrotron microwave emission can be detec...
The work supported by the grant consisted of two projects. The first project involved making detaile...
The electric field acceleration of electrons out of a thermal plasma and the simultaneous Joule heat...
Context. Microwave (MW) and hard X-ray (HXR) data are thought to be powerful means of investigating ...
Relativistic electrons in large solar flares produce gamma ray continuum by bremsstrahlung and micro...
Extending previous studies of nonthermal electron transport in solar flares, which include the effec...
A new analysis was made of a thermal flare model proposed by Brown, Melrose, and Spicer (1979) and S...
We use RHESSI hard X-ray observations to constrain acceleration of solar flare electrons, generally ...
The origin of hard X-rays and gamma-rays emitted from the solar atmosphere during occulted solar fla...
Context: Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
Knowledge of the energy distribution of electrons accelerated in solar flares is important for const...
Aims. We aim to constrain the acceleration, injection, and transport processes of flare-accelerated ...
A large fraction of the energy released during solar flares is carried by accelerated electrons and ...
The evolution of accelerated particle distributions in a magnetized plasma and the resulting radiati...
The joint study of hard x ray and microwave observations of solar flares is extremely important beca...
Recently, in a few case studies we demonstrated that gyrosynchrotron microwave emission can be detec...
The work supported by the grant consisted of two projects. The first project involved making detaile...
The electric field acceleration of electrons out of a thermal plasma and the simultaneous Joule heat...
Context. Microwave (MW) and hard X-ray (HXR) data are thought to be powerful means of investigating ...
Relativistic electrons in large solar flares produce gamma ray continuum by bremsstrahlung and micro...
Extending previous studies of nonthermal electron transport in solar flares, which include the effec...
A new analysis was made of a thermal flare model proposed by Brown, Melrose, and Spicer (1979) and S...
We use RHESSI hard X-ray observations to constrain acceleration of solar flare electrons, generally ...
The origin of hard X-rays and gamma-rays emitted from the solar atmosphere during occulted solar fla...
Context: Stochastic acceleration is thought to be a key mechanism in the energization of solar flare...
Knowledge of the energy distribution of electrons accelerated in solar flares is important for const...
Aims. We aim to constrain the acceleration, injection, and transport processes of flare-accelerated ...
A large fraction of the energy released during solar flares is carried by accelerated electrons and ...