Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Introduction to the Diagnosis of Magnetically Confined Thermonuclear Plasma Magnetics J. Arturo Alonso Laboratorio Nacional de Fusión EURATOM-CIEMAT E6 P2.10 arturo.alonso@ciemat.es version 0.1 (September 24, 2011) Magnetics, A. Alonso, copyleft 2010 1 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Outline Preliminaries 1 2 The magnetic coil Global magnitudes 3 4 Plasma position and shape Magnetics, A. Alonso, copyleft 2010 2 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Outline Preliminaries 1 2 The magnetic coil Global magnitudes 3 4 Plasma position and shape Magnetics, A. Alonso, copyleft 2010 3 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary MHD equilibrium The MHD equilibrium equation reads j × B = ∇ p ⇒ B · ∇ p = 0 , j · ∇ p = 0 . Magnetics, A. Alonso, copyleft 2010 4 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Maxwell Equations (I) The physical basis of nearly all the magnetic measurements ∇ · E = ρ (1a) ǫ 0 ∇ · B = 0 (1b) ∇ × E = − ∂ B (1c) ∂ t ∂ E ∇ × B = µ 0 j + µ 0 ǫ 0 (1d) ∂ t The last term in equation (1d) is the displacement current important for EM wave phenomena ( c = ( µ 0 ǫ 0 ) − 1 / 2 ). The dynamics we are interested here have typical frequencies ω and wavelengths k such that ω/ k ≪ c so that the displacement current can be ignored. Magnetics, A. Alonso, copyleft 2010 5 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Maxwell Equations (I) The physical basis of nearly all the magnetic measurements ∇ · E = ρ (1a) ǫ 0 ∇ · B = 0 (1b) ∇ × E = − ∂ B (1c) ∂ t ∂ E ∇ × B = µ 0 j + µ 0 ǫ 0 (1d) ∂ t The last term in equation (1d) is the displacement current important for EM wave phenomena ( c = ( µ 0 ǫ 0 ) − 1 / 2 ). The dynamics we are interested here have typical frequencies ω and wavelengths k such that ω/ k ≪ c so that the displacement current can be ignored. Magnetics, A. Alonso, copyleft 2010 5 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Maxwell Equations (II) By using the integral theorems (see [Jackson(1999)]) we can write equations (1) in their integral form � E · d S = 1 � ρ dV ǫ 0 ∂ V V � B · d S = 0 ∂ V � E · d l = − ∂ � B · d S ∂ t ∂ S S � � B · d l = µ 0 j · d S ∂ S S Magnetics, A. Alonso, copyleft 2010 6 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Outline Preliminaries 1 2 The magnetic coil Global magnitudes 3 4 Plasma position and shape Magnetics, A. Alonso, copyleft 2010 7 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary The magnetic coil The simplest measuring device used to measure magnetic fields is a simple coil. From the MEs we can compute the electromotive force E (Volts): E · d l = ∂ � � B · d S ≡ d E ≡ − dt Φ B ∂ t ∂ S S where Φ B is magnetic flux through the sur- face encircled by the circuit. There is an electric current running on the circuit (or a potential difference for an open circuit) whenever there exist a time variation of the magnetic flux through the circuit-limited surface. Magnetics, A. Alonso, copyleft 2010 8 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary The magnetic coil The simplest measuring device used to measure magnetic fields is a simple coil. From the MEs we can compute the electromotive force E (Volts): E · d l = ∂ � � B · d S ≡ d E ≡ − dt Φ B ∂ t ∂ S S Assume B ( x , t ) ≈ B ( t ) in the surface of the coil. Then E = ˙ BA . Increase the effective area with N windings so that E = ˙ BNA . We can recover B ( t ) from the time integral of ˙ B ( t ) (electronics). Magnetics, A. Alonso, copyleft 2010 8 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Hall effect detectors Measure static magnetic fields by use of the solid-state Hall effect : A current flowing along a slab of a semiconductor material in the presence of a magnetic field creates a potential difference accross the slab n carriers/m 3 and charge q , in equilibrium, the electric field caused by the charge separation balances the j × B force so that jB + nqE = 0 V H = jBL I nq = nqdB Caveats: affected by stray pickups, non-linear for large B and T ( � 140 ◦ C). Magnetics, A. Alonso, copyleft 2010 9 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Outline Preliminaries 1 2 The magnetic coil Global magnitudes 3 4 Plasma position and shape Magnetics, A. Alonso, copyleft 2010 10 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary The Rogowski coil Rogowski coils are used to measure the current flowing in a conducting medium by sensing the induced magnetic field. The magnetic flux through a Rogowski coil is N � � Φ B = B · d S i . S i i = 1 with d S i = dA u i . � z Assume windings are densely packed � N i → a ndl . Then � z � z � � Φ B = ndl B · u i dA = nA B · d l = nA µ j · d S = nA µ I . a S i a S Therefore E = d Φ B / dt = n µ A ˙ I . Magnetics, A. Alonso, copyleft 2010 11 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary The Rogowski coil From the Torpex tokamak in EPL-CRPP , Laussane, Switzerland. Magnetics, A. Alonso, copyleft 2010 12 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary The Voltage loop The Voltage loop measures the inductive electric potential V φ that drives the plasma current in a tokamak. Magnetics, A. Alonso, copyleft 2010 13 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Ohmic power and plasma resistance The heating (Ohmic) power P and plasma resistance R p can be calculated by the combination of a Rogowski coil ( I φ ) and a Voltage loop ( V φ ). Poynting’s theorem state the conservation of EM energy (see notes) ∂ u ∂ t + ∇ · S = − j · E , For the case of interest in a tokamak discharge this simplyfies to (see notes) I φ V φ = P + ∂ � 1 � 2 LI 2 φ ∂ t In stationary state P = I φ V φ = I 2 φ R p . Magnetics, A. Alonso, copyleft 2010 14 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Ohmic power and plasma resistance The heating (Ohmic) power P and plasma resistance R p can be calculated by the combination of a Rogowski coil ( I φ ) and a Voltage loop ( V φ ). Poynting’s theorem state the conservation of EM energy (see notes) ∂ u ∂ t + ∇ · S = − j · E , For the case of interest in a tokamak discharge this simplyfies to (see notes) I φ V φ = P + ∂ � 1 � 2 LI 2 φ ∂ t In stationary state P = I φ V φ = I 2 φ R p . Magnetics, A. Alonso, copyleft 2010 14 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Ohmic power and plasma resistance The heating (Ohmic) power P and plasma resistance R p can be calculated by the combination of a Rogowski coil ( I φ ) and a Voltage loop ( V φ ). Poynting’s theorem state the conservation of EM energy (see notes) ∂ u ∂ t + ∇ · S = − j · E , For the case of interest in a tokamak discharge this simplyfies to (see notes) I φ V φ = P + ∂ � 1 � 2 LI 2 φ ∂ t In stationary state P = I φ V φ = I 2 φ R p . Magnetics, A. Alonso, copyleft 2010 14 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Diamagnetic loop (I) It should now be evident that a diamagnetic loop like the one in the figure gives a measure of the cross -section-averaged toroidal B -field: V θ = d � B φ dS ≡ d dt � B φ � A dt S In what follows we will show how to relate this measurement to the plasma pressure profile. For ilustration we will work in cylindrical geometry. In this approximation � a � � V θ = d ≡ d dt � B z � π a 2 , 2 π B z ( r ) rdr dt 0 where z stands for the axial ( ∼ φ toroidal) direction. Magnetics, A. Alonso, copyleft 2010 15 / 26
Preliminaries The magnetic coil Global magnitudes Plasma position and shape Summary Diamagnetic loop (I) It should now be evident that a diamagnetic loop like the one in the figure gives a measure of the cross -section-averaged toroidal B -field: V θ = d � B φ dS ≡ d dt � B φ � A dt S In what follows we will show how to relate this measurement to the plasma pressure profile. For ilustration we will work in cylindrical geometry. In this approximation � a � � V θ = d ≡ d dt � B z � π a 2 , 2 π B z ( r ) rdr dt 0 where z stands for the axial ( ∼ φ toroidal) direction. Magnetics, A. Alonso, copyleft 2010 15 / 26
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