Physics
Scientific paper
Sep 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..147..131z&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 147, no. 1, p. 131-136.
Physics
8
Coronal Loops, Plasma Currents, Plasma Temperature, Solar Flares, Beta Factor, Temperature Profiles
Scientific paper
The paper describes characteristics of plasma temperature variation during two-current-loop collisions for different initial conditions, such as plasma-beta, the type of two-current-loop collision and initial current strength. Enhancement of the plasma temperature is caused by adiabatic heating. Strong initial current strength leads to a strong flare and effective plasma heating. It is suggested that comparing these characteristics with observed time profiles of physical quantities makes it possible to guess the initial conditions of loop-loop interactions, such as Alfven transient time, loop-loop configuration, and current strength.
Chargeishvili Bidzina
Sakai Jun-Ichi
Zhao Jie
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