Astron. Astrophys. 337, 887-896 (1998)
LRC-circuit analog of current-carrying magnetic loop: diagnostics of electric parameters
V.V. Zaitsev 1,
A.V. Stepanov 2,
S. Urpo 3 and
S. Pohjolainen 3
1 Applied Physics Institute, N. Novgorod, Russia
2 Pulkovo observatory, St. Petersburg, Russia
3 Metsähovi Radio Research Station, Helsinki
University of Technology, Espoo, Finland
Received 6 October 1997 / Accepted 4 March 1998
Abstract
The equation for an equivalent LRC-circuit of current-carrying
magnetic loop is obtained. It is suggested that the electric current,
driven by the converging flows in the photosphere, flows trough the
coronal part of a loop from one footpoint to another, and closes deep
in the photosphere where plasma beta 1. In a
self-consistent approach both the capacitance and the resistance of a
LRC-circuit depend on the electric current along the loop. This opens
new possibilities for the diagnostics of electric currents in coronal
loops, by using data on high-quality modulation of microwave emission
during flares. Spectral analysis of the Metsähovi millimeter wave
solar data for 16 solar flares have revealed modulation periods
0.7-17 s which give currents
6 1010-1.4 1012 A.
For two of the events we could compare the total energy of the
electric current stored in the magnetic loop with the energy released
in the flare. Only 5% of the total energy of the electric circuit was
released in both flares, suggesting a very low influence of these
flares on the magnetic loop structure. In the studied events there was
a tendency to decrease the energy release with the increase of the
current. This tendency is interpreted in terms of plasma beta, which
is getting smaller as the current grows. Therefore the plasma
instabilities responsible for the flare process manifestate themselves
weakly with the increase of the current.
Key words: Sun:
corona
Sun: flares
Sun: radio radiation
Send offprint requests to: Silja.Pohjolainen@hut.fi
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© European Southern Observatory (ESO) 1998
Online publication: August 27, 1998
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