Resonant cyclotron scattering
WebApr 20, 2024 · Spectral modification of energetic magnetar flares by resonant cyclotron scattering (RCS) is considered. During energetic flares, photons emitted from the magnetically-trapped fireball near the stellar surface should resonantly interact with …
Resonant cyclotron scattering
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WebA typical time resolution is Thomson scattering diagnostic finally succeeded in producing 35 µs and it is observed that the electron density is pumped the preliminary results by increasing ... Jeon Y.M. et al 2012 Phys. Rev. Lett. 109 035004 Cyclotron Emission and Electron Cyclotron Resonance [17] Park J .K., Boozer A.H. and Menard ... WebApr 12, 2024 · Abstract When assessing the scattering of radiation belt electrons by fast magnetosonic ... It is found that the kinetic effects lead to a lower minimum resonant energy around 100 eV and a broader resonant pitch angle range. ... Ω σ is the cyclotron frequency with the sign of charge, ...
WebApr 10, 2024 · Abstract Averaged equations and 3D particle-in-cell modeling are used to examine the frequency multiplication regime in a high-current relativistic gyrotron operating in the 0.1 THz band of frequencies. It is shown that the ratio of the 3rd harmonic power output and the fundamental cyclotron resonance power can be as high as 0.4–0.8%, … WebApr 12, 2024 · Cyclotron resonance can result in the absorption of R-mode photons at a low altitude region of the magnetosphere, and an FRB should then be emitted from a high-altitude region if the waves have ...
WebJan 20, 2024 · We find that scattering by ion cyclotron waves is crucially important to relativistic electron losses in Saturn's radiation belt. 2 Methodology ... This is because the cyclotron-resonant energy of radiation belt electrons due to L-mode waves decreases … WebThe resonant cyclotron scattering (RCS) may well be a plausible process that can help to explain the observed spectra of energetic magnetar flares. Magnetars emit mostly in the X-ray band so that close to their surface, the cyclotron frequency well exceeds the radiation …
WebOct 21, 2008 · The scattering efficiency is quantified by the resonant optical depth, tau_{res}, which is related to the electron density (assumed to be constant through the scattering slab). The RCS model is based on a simplified, 1D semi-analytical treatment of resonant …
WebWang, J. C. L., Lamb, D. Q., Loredo, T. J., Wasserman, I. M., Salpeter, E. E., Fenimore, E. E., … Kondo, I. (1989). Cyclotron resonant scattering in the spectra ... i\u0027m writing you or to youWebApr 5, 2006 · Resonant cyclotron scattering and Comptonization in neutron star magnetospheres 1 INTRODUCTION. The magnetospheres of neutron stars are filled with plasma, with the minimum magnetospheric plasma... 2 RESONANT SCATTER IN THE … network auctions ukWebApr 14, 2024 · Abstract Precipitation into the Earth's atmosphere due to pitch angle scattering by plasma waves has been recognized as one ... Whistler mode waves are right-hand polarized electromagnetic waves with frequencies below electron cyclotron frequency ... Resonant harmonic numbers from −10 to 10 and magnetic latitudes within 50° are ... i\u0027m writing to you becauseWebCyclotron line formation by resonant Compton-cyclotron scattering in Hercules X-1. Calculations are presented which show that a spectrum similar to the one observed for Hercules X-1 can be generated. It is shown that there is no straightforward way to explain … network audit checklistWebCyclotron Resonance Scattering Features (hereafter called CRSFs or simply “cyclotron lines”), first discovered in the s pec-trumofHer X-1 (Tru¨mper et al., 1977; Tru¨mper et al., 1978), are observed as absorption lines in the spectra of highly magnetized accreting X … i\u0027m writing to you in regards toWebSep 23, 2024 · Electromagnetic ion cyclotron waves are expected to pitch-angle scatter and cause atmospheric precipitation of relativistic (> 1 MeV) electrons under typical conditions in Earth’s radiation belts.However, it has been a long-standing mystery how relativistic … i\\u0027m writing to inquireWebCyclotron resonant scattering features (short: cyclotron lines) are sensitive tracers of the physics of the accretion columns and mounds of X-ray pulsars. They form by interaction of X-ray photons with magnetically quantized electrons in the accreted plasma close to the … i\u0027m writing to you to ask