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pdf file - Plasma Science and Fusion Center - MIT
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1942 Phys. <strong>Plasma</strong>s, Vol. 8, No. 5, May 2001 Egedal et al.<br />
FIG. 11. Color Contours measured current densities<br />
for the same conditions as in Fig 10. The dashed lines<br />
represent contours of constant poloidal magnetic flux.<br />
VI. MEASUREMENTS OF CURRENT SHEETS<br />
In magnetic configurations where the toroidal magnetic<br />
field is much stronger than the cusp field, the majority of the<br />
particles are no longer trapped. In such configurations we do<br />
indeed find a current sheet. In Figs. 10 <strong>and</strong> 11 snap shots in<br />
time of the plasma density <strong>and</strong> current density at the beginning<br />
of the formation of the current layers are shown. These<br />
correspond to the formation of current sheets for three different<br />
values of the ratio of toroidal field <strong>and</strong> cusp field: l 0<br />
B /B cusp 23, 17, 12 m note that the pro<strong>file</strong>s of all<br />
the previous figures are obtained with l 0 1m. In Fig. 12<br />
*E / j max is the ratio of the electric field <strong>and</strong> the current<br />
density at the center of the current sheet. Here E <br />
(R,Z)<br />
(d/dt)/R, where (R,Z) R0,Z0 RB dl is the<br />
poloidal flux variable, R is the major radius, Z describes the<br />
vertical position, <strong>and</strong> the subscript denotes the poloidal<br />
plane. is calculated on the basis of the currents applied in<br />
the poloidal field coils <strong>and</strong> the plasma current pro<strong>file</strong>s<br />
j (R,Z). The pro<strong>file</strong>s of j (R,Z) are obtained through a<br />
singular fit to the measured magnetic field pro<strong>file</strong>s.<br />
The Spitzer resistivity s is calculated using an electron<br />
temperature of 20 eV. It is seen that the constant Spitzer<br />
resistivity is insufficient to account for the low values of the<br />
current observed. Using an approach similar to that of Ref.<br />
15, the discrete particle enhanced inertial resistivity pei was<br />
introduced in Ref. 16 to describe the inertial resistivity based<br />
upon the time each individual particle spends in the region of<br />
the X line in a linear magnetic cusp. Although the values of<br />
pei are too low by a factor of about 6 to describe the<br />
measured values of * it is seen that pei accurately reproduces<br />
the scaling of * as a function of l 0 . It should be<br />
noted that pei was obtained on the basis of heuristic arguments<br />
for a linear cusp geometry. Using the measured geometry<br />
of the magnetic field a more accurate value of pei can<br />
be obtained which may fully account for the observed values<br />
of *. This work is currently underway. The current sheets<br />
shown in Fig. 11 evolve very differently in time. For the case<br />
where l 0 23 m, the X point evolves into an O point <strong>and</strong> the<br />
total plasma current increases from 1 kA to 10 kA. In the<br />
other two cases the X points are maintained throughout the<br />
pulses <strong>and</strong> the total plasma currents do not increase.<br />
VII. CONCLUSION<br />
Collisionless magnetic reconnection is routinely observed<br />
in the Versatile Toroidal Facility. In the cases where<br />
the strength of the cusp magnetic field is in the order of or<br />
larger than the strength of the toroidal magnetic field (l 0<br />
1 m the following experimental observations have been<br />
made<br />
1 Fast collisionless magnetic reconnection occurs without<br />
the formation of a macroscopic current sheet.<br />
FIG. 12. Inferred resistivities. A circles; *E / j ; diamonds, pei ;<br />
triangles, s ; B diamonds, */ pei ; triangles, */ s .<br />
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