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High-gradient two-beam electron accelerator
The main goal for this project was to design, build, and evaluate a detuned-cavity, collinear, two-beam accelerator structure. Testing was to be at the Yale University Beam Physics Laboratory, under terms of a sub-grant from Omega-P to Yale. Facilities available at Yale for this project include a 6-MeV S-band RF gun and associated beam line for forming and transporting a ~1 A drive beam , a 300 kV beam source for use as a test beam, and a full panoply of laboratory infrastructure and test equipment. During the first year of this project, availability and functionality of the 6-MeV drive beam and 300 kV test beam were confirmed, and the beam line was restored to a layout to be used with the two-beam accelerator project. Major efforts during the first year were also focused on computational design and simulation of the accelerator structure itself, on beam dynamics, and on beam transport. Effort during the second year was focussed on building and preparing to test the structure, including extensive cold testing. Detailed results from work under this project have been published in twelve archival journal articles, listed in Section IV of the technical report.
Results of four one-day electron-accelerator irradiations of enriched Mo-100 targets for the production of Mo-99
A series of four one-day irradiations was conducted with 100 Mo-enriched disk targets. After irradiation, the enriched disks were removed from the target and dissolved. The resulting solution was processed using a NorthStar RadioGenix™ 99m Tc generator either at Argonne National Laboratory or at the NorthStar Medical Radioisotopes facility. Runs on the RadioGenix system produced inconsistent analytical results for 99m Tc in the Tc/Mo solution. These inconsistencies were attributed to the impurities in the solution or improper column packing. During the irradiations, the performance of the optic transitional radiation (OTR) and infrared cameras was tested in high radiation field. The OTR cameras survived all irradiations, while the IR cameras failed every time. The addition of X-ray and neutron shielding improved camera survivability and decreased the number of upsets.
Modeling Electron Acceleration and Transport in 3D Solar Flare Regions
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Next generation superconducting electron accelerators: a high efficiency and high power tool for radiation science and industrial application
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Magnetic Analyzers for X-pinch Accelerated Electron and Ion Beams
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Wave Generation and Wave-Particle Interaction Using Space-Based, RF, Linear Electron Accelerators
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The Efficiency of Electron Acceleration during the Impulsive Phase of a Solar Flare
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Solar wind conditions leading to efficient radiation belt electron acceleration: A superposed epoch analysis
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Evidence of Electron Acceleration via Nonlinear Resonant Interactions with Whistler-mode Waves at Foreshock Transients
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Energy limits of electron acceleration in the plasma sheet during substorms: A case study with the Magnetospheric Multiscale (MMS) mission
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Low‐altitude electron acceleration due to multiple flow bursts in the magnetotail
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Subpacket structure in strong VLF chorus rising tones: characteristics and consequences for relativistic electron acceleration
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Coalescence of Macroscopic Magnetic Islands and Electron Acceleration from STEREO Observation
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Single-cycle electron acceleration in focused laser fields.
The possibility of accelerating particles with a focused laser is considered. The particle is accelerated transversely by the electric field and redirected to the forward direction within a single half-cycle by the magnetic field of the radiation. The equations of motion of the particle are solved and discussed. Special attention is given to an intuitive understanding of the constraint imposed by the geometry of the focal region. Optimum conditions are examined.
Io-accelerated electrons and ions
A description is given of a model in which the Jupiter moon Io interacts with the Jovian magnetosphere through plasma sheaths in the vicinity of Io. Several recent results available from Pioneer 10 are used to revise a Io sheath model suggested by Gurnett (1972) and developed by Hubbard et al. (1974). The revised model is used to suggest an explanation for a number of observations. Attention is also given to other phenomena which might be detectable with the aid of future experiments.
The 10-100 keV electron acceleration and emission from solar flares
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Generation and propagation of an electromagnetic pulse in the Trigger experiment and its possible role in electron acceleration
Instruments onboard the Trigger payload detected a large-amplitude, low-frequency, electric field pulse which was observed with a time delay consistent only with an electromagnetic wave. A model for this perturbation is constructed, and the associated field-aligned current is calculated as a function of altitude. This experiment may simulate the acceleration mechanism which results in the formation of auroral arcs, and possibly even other events in cosmic plasmas.