High Power Laser Science and Engineering, Volume. 7, Issue 1, 01000e17(2019)
Maser radiation from collisionless shocks: application to astrophysical jets
Fig. 1. Perpendicular and parallel components of electron momentum (normalized to the mean electron momentum
Fig. 2. Imaginary part of the refractive index as a function of frequency for a mean beam energy of 100 keV and a thermal spread of 1 keV, and a mean beam energy of 500 keV and a thermal spread of 5 keV. The magnetic field ratio is taken to be 20.
Fig. 3. Composite overview of 3D VSim PIC simulation results in an
Fig. 4. 3D VSim PIC simulation results showing (a) the spectrum of EM emission at
Fig. 5. Diagrammatic overview of the experimental setup showing the magnetic coil configuration, electron gun and the convergent axial magnetic field profile with peak-plateau region for cyclotron resonant energy transfer.
Fig. 6. Experimental measurements for the TE01 resonance, illustrating the spectrum of the output signal, displaying a strong resonance close to the electron-cyclotron frequency, 4.42 GHz.
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D. C. Speirs, K. Ronald, A. D. R. Phelps, M. E. Koepke, R. A. Cairns, A. Rigby, F. Cruz, R. M. G. M. Trines, R. Bamford, B. J. Kellett, B. Albertazzi, J. E. Cross, F. Fraschetti, P. Graham, P. M. Kozlowski, Y. Kuramitsu, F. Miniati, T. Morita, M. Oliver, B. Reville, Y. Sakawa, S. Sarkar, C. Spindloe, M. Koenig, L. O. Silva, D. Q. Lamb, P. Tzeferacos, S. Lebedev, G. Gregori, R. Bingham. Maser radiation from collisionless shocks: application to astrophysical jets[J]. High Power Laser Science and Engineering, 2019, 7(1): 01000e17
Special Issue: LABORATORY ASTROPHYSICS
Received: Aug. 30, 2018
Accepted: Jan. 21, 2019
Posted: Jan. 31, 2019
Published Online: Apr. 4, 2019
The Author Email: D. C. Speirs (david.c.speirs@strath.ac.uk)