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A plasma 10 times as hot as the sun.


A plasma 10 times as hot as the sun

"Tokamak" is a word composed of thefirst syllables of the Russian words for "toroidal magnetic chamber." a Russian invention, the tokamak has been voted by many physicists most likely to succeed in achieving controlled thermonuclear ther·mo·nu·cle·ar  
adj.
1. Of, relating to, or derived from the fusion of atomic nuclei at high temperatures: thermonuclear reactions.

2.
 fusion. In the toroidal chamber, magnetic fields magnetic fields,
n.pl the spaces in which magnetic forces are detectable; created by magnetostrictive ultrasonic scalers to cause the tips of instruments such as ultrasonic scalers to vibrate.
 confine a plasma -- an

ionized i·on·ize  
tr. & intr.v. i·on·ized, i·on·iz·ing, i·on·iz·es
To convert or be converted totally or partially into ions.



i
 gas -- while its temperature and density are raised to the point where nuclei in it should fuse and produce energy. In experiments conducted during July, one of the world's biggest tokamaks achieved a plasma temperature of 200 million kelvin (200 MK).

This temperature, achieved by theTokamak Fusion Test Reactor (TFTR TFTR Tokamak Fusion Test Reactor
TFTR Toroidal Fusion Test Reactor
TFTR Thanks for the Report
TFTR Thanks for the Reminder
) at the Princeton (N.J.) Plasma Physics Laboratory, is the highest ever reached in a laboratory. It is 10 times the temperature in the center fo the sun, but more important, it is more than enough for breakeven, the point where fusions produce as much energy as has to be expended to ignite them.

Besides temperature, break-even requiresanother criterion: the product of plasma density and confinement time, usually called the LAwson criterion. In April, TFTR experiments at lower temperatures produced a Lawson criterion of 1.5 X 10.sup.14 seconds per cubic centimeter, which is close to the goal for a practical reactor and five to seven times what is needed for break-even. However, the 200-MK experiments had a Lawson criterion of 10.sup.13., two or three times too small for break-even.

The next step is to put the high valuestogether and get break-even. Donald Grove, TFTR project manager, says they expect to echieve that in 1987 using the hydrogen isotope deuterium deuterium (dtēr`ēəm), isotope of hydrogen with mass no. 2. The deuterium nucleus, called a deuteron, contains one proton and one neutron. , with which they have been working so far. Then they intend to introduce another hydrogen isotope, tritium tritium (trĭt`ēəm), radioactive isotope of hydrogen with mass number 3. The tritium nucleus, called a triton, contains one proton and two neutrons. It has a half-life of 12.5 years and decays by beta-particle emission. . Deuterium-tritium fusion, which most controlled fusion experiments today are trying to achieve, produces energetic neutrons, from which energy can easily be harvested and converted to useful things like steam or electric power. They hope for deuterium-tritium break-even in 1989.

One reason tokamaks are expected tosucceed is that they should help confine themselves by producing a "bootstrap See boot.

(operating system, compiler) bootstrap - To load and initialise the operating system on a computer. Normally abbreviated to "boot". From the curious expression "to pull oneself up by one's bootstraps", one of the legendary feats of Baron von Munchhausen.
 current," a current flowing through the plasma around the torus torus /to·rus/ (tor´us) pl. to´ri   [L.] a swelling or bulging projection.

to·rus
n. pl.
. This current will generate a magnetic field that will help the external magnets confine the plasma. In these experiments, Grove says, a current not due to external driving seemed to arise in the plasma. The physicists concluded that this was probbably the bootstrap current, Grove says, although supporting evidence for that conclusion so far is nil.
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Copyright 1986, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

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Title Annotation:research at Tokamak Fusion Test Reactor
Author:Thomsen, Dietrick E.
Publication:Science News
Date:Aug 16, 1986
Words:409
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