Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...146...25n&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 146, no. 1, May 1985, p. 25-37.
Astronomy and Astrophysics
Astrophysics
3
Coronal Loops, Energy Transfer, Particle Acceleration, Plasma Heating, Solar Electrons, Solar Flares, Conductive Heat Transfer, Electron Bombardment, Electron Energy, Energy Distribution, Magnetohydrodynamic Waves, Plasma Acceleration, Plasma Dynamics, Radiative Transfer, Shock Heating, Spatial Distribution
Scientific paper
In the present investigation of the relation between the dynamical behavior of a flare plasma and the evolution of various energy terms, using an electron beam enhancement model in the impulsive phase of solar flares, the energy input or output rates integrated along the entire loop are evaluated and the distribution of the flare energy among various energy terms is demonstrated through the integration of those rates over time. A one-fluid, two-temperature model is adopted, and nonthermal electrons with power law spectra are assumed to be isotropically injected from the loop apex. The spatial distribution of thermal conduction shows that thermal energy is removed from the high temperature region and is primarily deposited in the thermal conduction front.
Jordan Cathy
Nagai F.
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