Download An Assessment of the Department of Energy's Office of Fusion by Fusion Science Assessment Committee, Plasma Science PDF

By Fusion Science Assessment Committee, Plasma Science Committee, Board on Physics and Astronomy, National Research Council

The goal of this review of the fusion strength sciences application of the dept of Energy's (DOE's) workplace of technology is to guage the standard of the study application and to supply advice for the longer term application process aimed toward strengthening the examine section of this system. The committee centred its evaluate of the fusion software on magnetic confinement, or magnetic fusion strength (MFE), and touched merely in short on inertial fusion strength (IFE), simply because MFE-relevant examine debts for approximately ninety five percentage of the investment within the workplace of Science's fusion application. except in a different way famous, all references to fusion during this record might be assumed to consult magnetic fusion.

Fusion study conducted within the usa lower than the sponsorship of the place of work of Fusion power Sciences (OFES) has made outstanding strides through the years and lately handed a number of very important milestones. for instance, weakly burning plasmas with temperatures drastically exceeding these at the floor of the solar were created and clinically determined. major development has been made in knowing and controlling instabilities and turbulence in plasma fusion experiments, thereby facilitating superior plasma confinement-remotely controlling turbulence in a 100-million-degree medium is a most advantageous clinical success by means of any degree. idea and modeling at the moment are capable of offer worthwhile insights into instabilities and to steer experiments. Experiments and linked diagnostics at the moment are capable of extract adequate information regarding the techniques taking place in high-temperature plasmas to lead additional advancements in idea and modeling. the various significant experimental and theoretical instruments which have been built are actually converging to supply a qualitative swap within the program's method of clinical discovery.

The U.S. software has characteristically been an enormous resource of innovation and discovery for the overseas fusion power attempt. The target of realizing at a primary point the actual methods governing saw plasma habit has been a distinguishing function of this system.

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Extra info for An Assessment of the Department of Energy's Office of Fusion Energy Sciences Program (Compass Series)

Example text

Because of its broad importance for fusion and also in astrophysical plasmas (solar flares, magnetic storms in Earth’s magnetosphere, and stellar accretion disks), magnetic reconnection was widely studied by fusion scientists, especially in the early days of the program. The theory of the “tearing mode,” which is the manifestation of reconnection when the amplitude of the magnetic perturbations is small, was developed for a resistive plasma. Later theories demonstrated that kinetic effects could also facilitate reconnection and that the fluid drifts of electrons and ions could significantly modify stability due to the relatively feeble growth rates of the instabilities in high-temperature plasmas.

It was at that time that reconnection research shifted to the National Aeronautics and Space Administration (NASA) and the NSF-funded space science program. The recent construction of a dedicated magnetic reconnection experiment and its exploration in some of the emerging new experiments signals a rebirth of scientific interest in this area in the fusion program. Although magnetic reconnection and resistive instabilities have historically emphasized the plasma current and its associated magnetic field as the source of free energy, there is increasing observational and theoretical evidence that the plasma pressure gradient can also drive magnetic islands and reconnection.

At very high powers, the distribution often deviates significantly from Maxwellian, and direct solution of the velocityspace diffusion equation is necessary to produce the resultant particle distribution functions and to calculate the associated heating and current drive. Finite difference and Monte Carlo techniques are reasonably well established for these purposes. All of the above theories or models are computationally feasible only with idealizations and approximations, and determining or demonstrating the range of validity for a particular model is quite a challenge.

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