Hydrodynamics of flaring loops - SMM observations and numerical simulations

Details Hydrodynamics of flaring loops - SMM observations and numerical simulations Hydrodynamics of flaring loops - SMM observations and numerical simulations

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..147p&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Physics

2

Coronal Loops, Magnetohydrodynamics, Solar Flares, Solar Maximum Mission, Light Curve, Line Spectra, Numerical Flow Visualization, Solar Atmosphere, Velocity Distribution

Scientific paper

The hydrodynamic response of confined magnetic structures to strong heating perturbations is investigated by means of a time-dependent one-dimensional code which incorporates the energy, momentum and mass conservation equations. The entire atmospheric structure from the chromosphere to the corona is taken into account. The results of model calculations are compared with observations of flares obtained with the X-ray Polychromator experiment on the Solar Maximum Mission.

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