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Section Days abstract book 2010.indd - RUB Research School ...

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NSE_10<br />

EXPERIMENTAL SIMULATION OF SOLAR<br />

MAGNETIC FLUX TUBES<br />

Felix Mackel, P. Kempkes, H. Stein, J. Tenfelde and H. Soltwisch<br />

Institute for Experimental Physics V<br />

Workgroup Laser and Plasma Physics<br />

Ruhr-Universität Bochum, 44780 Bochum, Germany<br />

email: felix.mackel@ep5.rub.de<br />

A pulsed-power experiment has been designed to produce arc-shaped magnetic flux tubes<br />

similar to ascending solar flares. The tubes are filled with hydrogen plasma and expand with<br />

a velocity of about 2.5 cm/µs, while keeping their minor radius of about 1.5 cm constant<br />

during their lifetime of about 10 µs. In order to characterize the plasma regime and to<br />

investigate relevant magnetohydrodynamic phenomena, accurate data on parameters like<br />

electron density and mean energy are essential.<br />

For measuring the line integrated electron density a CO2 laser interferometer is set up at a<br />

fixed position. Time resolved measurements of the discharge arc’s passage across the<br />

laser beam allow for the measurement of the radial profile of the line-integrated electron<br />

density. Results are compared to measurements taken with an electrostatic probe at the<br />

same position.<br />

The magnetic field of the arc is investigated employing induction probes. From the currentgenerated<br />

magnetic field, information about the arc’s propagation and expansion is obtained.<br />

Furthermore, the derived plasma conditions indicate the possibility of magnetic flux being<br />

frozen into the plasma.

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