Drift-Type Waves in Rotating Tokamak Plasma

The concept of energy production through the fusion of two light nuclei has been studied since the 1950’s. One of the major problems that fusion scientists have encountered is the confinement of the hot ionised gas, i.e. the plasma, in which the fusion process takes place. The most common way to con...

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Bibliographic Details
Main Author: Asp, Elina
Format: Doctoral Thesis
Language:English
Published: Uppsala universitet, Institutionen för astronomi och rymdfysik 2003
Subjects:
ITG
TE
Online Access:http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-3400
http://nbn-resolving.de/urn:isbn:91-554-5625-1
id ndltd-UPSALLA1-oai-DiVA.org-uu-3400
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spelling ndltd-UPSALLA1-oai-DiVA.org-uu-34002013-01-08T13:03:47ZDrift-Type Waves in Rotating Tokamak PlasmaengAsp, ElinaUppsala universitet, Institutionen för astronomi och rymdfysikUppsala : Institutionen för astronomi och rymdfysik2003Space and plasma physicsfusionplasmatokamakrotationdriftshipITGTELandauTe/Tihot-electronconfinementstiffnessWeilandRymd- och plasmafysikSpace physicsRymdfysikThe concept of energy production through the fusion of two light nuclei has been studied since the 1950’s. One of the major problems that fusion scientists have encountered is the confinement of the hot ionised gas, i.e. the plasma, in which the fusion process takes place. The most common way to contain the plasma is by using at magnetic field configuration, in which the plasma takes a doughnut-like shape. Experimental devices of this kind are referred to as tokamaks. For the fusion process to proceed at an adequate rate, the temperature of the plasma must exceed 100,000,000C. Such a high temperature forces the plasma out of thermodynamical equilibrium which plasma tries to regain by exciting a number of turbulent processes. After successfully quenching the lager scale magnetohydrodynamic turbulence that may instantly disrupt the plasma, a smaller scale turbulence revealed itself. As this smaller scale turbulence behaved contrary to the common theory at the time, it was referred to as anomalous. This kind of turbulence does not directly threaten existents of the plasma, but it allows for a leakage of heat and particles which inhibits the fusion reactions. It is thus essential to understand the origin of anomalous turbulence, the transport it generates and most importantly, how to reduce it. Today it is believed that anomalous transport is due to drift-type waves driven by temperature and density inhomogeneities and the theoretical treatment of these waves is the topic of this thesis. The first part of the thesis contains a rigorous analytical two-fluid treatment of drift waves driven solely by density inhomogeneities. Effects of the toroidal magnetic field configuration, the Landau resonance, a peaked diamagnetic frequency and a sheared rotation of the plasma have been taken into account. These effects either stabilise or destabilise the drift waves and to determine the net result on the drift waves requires careful analysis. To this end, dispersion relations have been obtained in various limits to determine when to expect the different effects to be dominant. The main result of this part is that with a large enough rotational shear, the drift waves will be quenched. In the second part we focus on temperature effects and thus treat reactive drift waves, specifically ion temperature gradient and trapped electron modes. In fusion plasmas the α-particles, created as a by-product of the fusion process, transfer the better part of their energy to the electrons and hence the electron temperature is expected to exceed the ion temperature. In most experiments until today, the ion temperature is greater than the electron temperature and this have been proven to improve the plasma confinement. To predict the performance of future fusion plasmas, where the fusion process is ongoing, a comprehensive study of hot-electron plasmas and external heating effects have been carried out. Especially the stiffness (heat flux vs. inverse temperature length scale) of the plasma has been examined. This work was performed by simulations done with the JETTO code utilising the Weiland model. The outcome of these simulations shows that the plasma response to strong heating is very stiff and that the plasma energy confinement time seems to vary little in the hot-electron mode. Doctoral thesis, comprehensive summaryinfo:eu-repo/semantics/doctoralThesistexthttp://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-3400urn:isbn:91-554-5625-1Comprehensive Summaries of Uppsala Dissertations from the Faculty of Science and Technology, 1104-232X ; 837application/pdfinfo:eu-repo/semantics/openAccess
collection NDLTD
language English
format Doctoral Thesis
sources NDLTD
topic Space and plasma physics
fusion
plasma
tokamak
rotation
drift
ship
ITG
TE
Landau
Te/Ti
hot-electron
confinement
stiffness
Weiland
Rymd- och plasmafysik
Space physics
Rymdfysik
spellingShingle Space and plasma physics
fusion
plasma
tokamak
rotation
drift
ship
ITG
TE
Landau
Te/Ti
hot-electron
confinement
stiffness
Weiland
Rymd- och plasmafysik
Space physics
Rymdfysik
Asp, Elina
Drift-Type Waves in Rotating Tokamak Plasma
description The concept of energy production through the fusion of two light nuclei has been studied since the 1950’s. One of the major problems that fusion scientists have encountered is the confinement of the hot ionised gas, i.e. the plasma, in which the fusion process takes place. The most common way to contain the plasma is by using at magnetic field configuration, in which the plasma takes a doughnut-like shape. Experimental devices of this kind are referred to as tokamaks. For the fusion process to proceed at an adequate rate, the temperature of the plasma must exceed 100,000,000C. Such a high temperature forces the plasma out of thermodynamical equilibrium which plasma tries to regain by exciting a number of turbulent processes. After successfully quenching the lager scale magnetohydrodynamic turbulence that may instantly disrupt the plasma, a smaller scale turbulence revealed itself. As this smaller scale turbulence behaved contrary to the common theory at the time, it was referred to as anomalous. This kind of turbulence does not directly threaten existents of the plasma, but it allows for a leakage of heat and particles which inhibits the fusion reactions. It is thus essential to understand the origin of anomalous turbulence, the transport it generates and most importantly, how to reduce it. Today it is believed that anomalous transport is due to drift-type waves driven by temperature and density inhomogeneities and the theoretical treatment of these waves is the topic of this thesis. The first part of the thesis contains a rigorous analytical two-fluid treatment of drift waves driven solely by density inhomogeneities. Effects of the toroidal magnetic field configuration, the Landau resonance, a peaked diamagnetic frequency and a sheared rotation of the plasma have been taken into account. These effects either stabilise or destabilise the drift waves and to determine the net result on the drift waves requires careful analysis. To this end, dispersion relations have been obtained in various limits to determine when to expect the different effects to be dominant. The main result of this part is that with a large enough rotational shear, the drift waves will be quenched. In the second part we focus on temperature effects and thus treat reactive drift waves, specifically ion temperature gradient and trapped electron modes. In fusion plasmas the α-particles, created as a by-product of the fusion process, transfer the better part of their energy to the electrons and hence the electron temperature is expected to exceed the ion temperature. In most experiments until today, the ion temperature is greater than the electron temperature and this have been proven to improve the plasma confinement. To predict the performance of future fusion plasmas, where the fusion process is ongoing, a comprehensive study of hot-electron plasmas and external heating effects have been carried out. Especially the stiffness (heat flux vs. inverse temperature length scale) of the plasma has been examined. This work was performed by simulations done with the JETTO code utilising the Weiland model. The outcome of these simulations shows that the plasma response to strong heating is very stiff and that the plasma energy confinement time seems to vary little in the hot-electron mode.
author Asp, Elina
author_facet Asp, Elina
author_sort Asp, Elina
title Drift-Type Waves in Rotating Tokamak Plasma
title_short Drift-Type Waves in Rotating Tokamak Plasma
title_full Drift-Type Waves in Rotating Tokamak Plasma
title_fullStr Drift-Type Waves in Rotating Tokamak Plasma
title_full_unstemmed Drift-Type Waves in Rotating Tokamak Plasma
title_sort drift-type waves in rotating tokamak plasma
publisher Uppsala universitet, Institutionen för astronomi och rymdfysik
publishDate 2003
url http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-3400
http://nbn-resolving.de/urn:isbn:91-554-5625-1
work_keys_str_mv AT aspelina drifttypewavesinrotatingtokamakplasma
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