Physical conditions in the low corona and chromosphere of solar active regions according to spectral radar measurements

@article{Kaltman2013PhysicalCI,
  title={Physical conditions in the low corona and chromosphere of solar active regions according to spectral radar measurements},
  author={T. Kaltman and V. Bogod and A. Stupishin and L. Yasnov},
  journal={Geomagnetism and Aeronomy},
  year={2013},
  volume={53},
  pages={1030-1034}
}
The physical conditions in the low corona and chromosphere of solar active regions are studied. A diagnostics technique based on multiwave observations in the centimeter range, photospheric magnetic field extrapolation, and radioemission calculations has been applied. The calculated spatial and spectral structure of the radioemission has been compared with RATAN-600 spectral-polarization observations with a high spatial resolution. The effect of the plasma physical parameters on the emission… Expand

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