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A year in orbit: ISS deployment tests radiation detectors for future space missions
The predawn darkness on a cool Florida night was shattered by the ignition of nine Merlin engines on a SpaceX Falcon 9 rocket. The thrust of the engines shook the ground miles away. From a distance, the rocket appeared to slowly rise above the horizon. For the cargo onboard, the launch was anything but gentle, as the ignition of liquid oxygen generated more than 1.5 million pounds of force. After the rocket had been out of sight for several minutes, the booster dramatically returned to Earth with several sonic booms in a captivating show of engineering designed to make space travel less expensive and more sustainable.
D. Hofmann
Nuclear Science and Engineering | Volume 147 | Number 3 | July 2004 | Pages 319-322
Technical Note | doi.org/10.13182/NSE04-A2436
Articles are hosted by Taylor and Francis Online.
A projectile penetrates with high velocity the lid of a gas receptacle, compresses and heats a statically precompressed volume of a gaseous deuterium-tritium mixture, and may possibly start fusion reactions by releasing and focusing a shock wave.A high amount of energy is delivered to a small volume in a very short time. The wall of the receptacle and the high density of projectile and receptacle material act as confinement. For the acceleration of projectile and receptacle, a series of interconnected (cascaded) and modified light gas guns is used.In the first part of this note, technical aspects are outlined. By a synchronized operation of the light gas guns, projectile and receptacle hit each other in the center of a reaction chamber. If fusion reactions can be started, a gas-cooled high-temperature moderator, containing breeding material for tritium, will surround the reaction chamber. In the second part the shock wave propagation and focusing is described in approximation. The results should encourage a precise theoretical treatment of the problem.