The cooling of post-flare plasmas is discussed and the formation of loop prominences is explained as due to a thermal instability. A one-dimensional model was developed for active loop prominences. Only the motion and heat fluxes parallel to the existing magnetic fields are considered. The relevant size scales and time scales are such that single-fluid MHD equations are valid. The effects of gravity, the geometry of the field and conduction losses to the chromosphere are included. A computer code was constructed to solve the model equations. Basically, the system is treated as an initial value problem (with certain boundary conditions at the chromosphere-corona transition region), and a two-step time differencing scheme is used
We present revised values of temperature and density for the flare loops of 29 July 1973 and compare...
Satellite observations with high spatial and temporal resolution have revealed the highly dynamic na...
Prominence condensation and support, the dynamics of coronal loops, and streamer structure and disco...
A simple model facilitates calculation of the influence of magnetic field configuration on the condu...
We examine the radiative cooling of coronal loops and demonstrate that the recently identified catas...
ABSTRACT---- We investigate a model for the decay of flare heated coronal loops in which rapid radia...
A one-dimensional loop model for the evaporative cooling of the coronal flare plasma was investigate...
Using the “enthalpy-based thermal evolution of loops” (EBTEL) model, we investigate the hydrodynamic...
We investigate the impact of turbulent suppression of parallel heat conduction on the cooling of pos...
The thermal equilibrium and evolution of coronal structure is studied in this thesis. A symmetric an...
Solar flare model atmospheres computed under the assumption of energetic equilibrium in the chromosp...
In the present work, we study the C8 flare that occurred on 2000 September 26 at 19:49 UT and observ...
It has become clear that the closed-field regions of the solar atmosphere are not static (as was onc...
Recent space observations of coronal lines broadening during a flare occurrence suggest that unresol...
The thermal disappearance of solar prominences under strong perturbations due to wave heating, Ohmic...
We present revised values of temperature and density for the flare loops of 29 July 1973 and compare...
Satellite observations with high spatial and temporal resolution have revealed the highly dynamic na...
Prominence condensation and support, the dynamics of coronal loops, and streamer structure and disco...
A simple model facilitates calculation of the influence of magnetic field configuration on the condu...
We examine the radiative cooling of coronal loops and demonstrate that the recently identified catas...
ABSTRACT---- We investigate a model for the decay of flare heated coronal loops in which rapid radia...
A one-dimensional loop model for the evaporative cooling of the coronal flare plasma was investigate...
Using the “enthalpy-based thermal evolution of loops” (EBTEL) model, we investigate the hydrodynamic...
We investigate the impact of turbulent suppression of parallel heat conduction on the cooling of pos...
The thermal equilibrium and evolution of coronal structure is studied in this thesis. A symmetric an...
Solar flare model atmospheres computed under the assumption of energetic equilibrium in the chromosp...
In the present work, we study the C8 flare that occurred on 2000 September 26 at 19:49 UT and observ...
It has become clear that the closed-field regions of the solar atmosphere are not static (as was onc...
Recent space observations of coronal lines broadening during a flare occurrence suggest that unresol...
The thermal disappearance of solar prominences under strong perturbations due to wave heating, Ohmic...
We present revised values of temperature and density for the flare loops of 29 July 1973 and compare...
Satellite observations with high spatial and temporal resolution have revealed the highly dynamic na...
Prominence condensation and support, the dynamics of coronal loops, and streamer structure and disco...