Heating in Toroidal Plasmas 1981
DOI: 10.1016/b978-1-4832-8373-9.50110-5
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Heating Experiments in the Heliotron E

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1986
1986
1986
1986

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“…After the occurrence of a strong MHD instability, the plasma energy (diamagnetic beta) decreases fast with a time constant of 2 to 3 ms and then decreases slowly with a longer time constant of 10 to 15 ms. The fast decrease in plasma energy is, possibly, the result of the rapid energy loss ( -3W p /9t = -200 kW) by an interchange instability, where bolometric measurements detect the same amount of heat pulse (200 kW) at the wall, after a fast decay of beta [29][30]. The subsequent slow decrease of the plasma energy is the result of impurity accumulation due to the increase of impurity sources at the plasma boundary in the presence of a strong MHD instability.…”
Section: Diamagnetic Average Beta and Magnetic Fluctuationsmentioning
confidence: 99%
“…After the occurrence of a strong MHD instability, the plasma energy (diamagnetic beta) decreases fast with a time constant of 2 to 3 ms and then decreases slowly with a longer time constant of 10 to 15 ms. The fast decrease in plasma energy is, possibly, the result of the rapid energy loss ( -3W p /9t = -200 kW) by an interchange instability, where bolometric measurements detect the same amount of heat pulse (200 kW) at the wall, after a fast decay of beta [29][30]. The subsequent slow decrease of the plasma energy is the result of impurity accumulation due to the increase of impurity sources at the plasma boundary in the presence of a strong MHD instability.…”
Section: Diamagnetic Average Beta and Magnetic Fluctuationsmentioning
confidence: 99%