2D MHD AND 1D HD MODELS OF A SOLAR FLARE—A COMPREHENSIVE COMPARISON OF THE RESULTS

@article{Falewicz20152DMA,
  title={2D MHD AND 1D HD MODELS OF A SOLAR FLARE—A COMPREHENSIVE COMPARISON OF THE RESULTS},
  author={Robert Falewicz and Pawel Rudawy and Krzysztof Murawski and Anand K. Srivastava},
  journal={The Astrophysical Journal},
  year={2015},
  volume={813},
  pages={70}
}
  • Robert Falewicz, Pawel Rudawy, +1 author Anand K. Srivastava
  • Published 2015
  • Physics
  • The Astrophysical Journal
  • Without any doubt, solar flaring loops possess a multithread internal structure that is poorly resolved, and there are no means to observe heating episodes and thermodynamic evolution of the individual threads. These limitations cause fundamental problems in numerical modeling of flaring loops, such as selection of a structure and a number of threads, and an implementation of a proper model of the energy deposition process. A set of one-dimensional (1D) hydrodynamic and two-dimensional (2D… CONTINUE READING

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