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Magnetic nozzle studied at Princeton
Scientists at the DOE's Princeton Plasma Physics Laboratory (PPPL) are using a novel experimental apparatus to study basic plasma physics phenomena with potential applications in several fields, including the development of plasma thrusters for space propulsion. This research program is being performed in collaboration with many scientists, including several at NASA. The Magnetic Nozzle Experiment (MNX) studies the expansion of a plasma (hot ionized gas) through a constriction in magnetic field lines, called a magnetic nozzle. MNX utilizes a 30-cm long helium or argon plasma column, initially 2-cm in diameter, confined by a magnetic field. The field is compressed at one location along the column-the magnetic nozzle. The plasma is squeezed there and then expands as it flows through and out. During the expansion, the plasma cools and partially recombines into a neutral gas. This phase transition is of fundamental interest to scientists who hope to use the magnetic nozzle to accelerate plasma to supersonic speeds for space propulsion. The recombination phenomenon is also of interest in the fields of fusion research, materials processing, and lasers. PPPL Physicist Sam Cohen, who heads the MNX project, said this work builds on earlier studies of recombination at Princeton. That research was motivated by the need to cool the plasma exhaust in magnetic fusion energy devices. One of the exciting results was the generation of conditions in the plasma that might it useful as a source for a new type of laser. In a space propulsion system, it is essential for the plasma to detach itself from the magnetic field lines in the exhaust region of the nozzle. Otherwise, the exhausted plasma would return to the spacecraft, reducing the thrust. Detachment of supersonic plasma ions may be brought about by several processes, including both recombination and charge exchange of ions, or loss of magnetization. MNX is equipped with apparatus to measure the charged and neutral particle temperatures and velocities in the expansion region. Measurements of ultraviolet light and x-rays emitted by the plasma exhaust are enabling scientists to quantify the recombination processes that occur. Submitted by DOE's Princeton Plasma Physics Laboratory |
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