A model for cyclotron resonance scattering features

Strong magnetic fields of accreting neutron stars Modeling cyclotron resonance scattering features

Schönherr, Gabriele Strong magnetic fields of accreting neutron stars — Modeling cyclotron lines — Accreting neutron stars in X-ray binaries are unique astrophysical laboratories for studying the physics of matter under extreme conditions. Not only does their compact nature lead to an amount of gravity only topped by black hole systems; they can also possess extreme magnetic fields, exceeding t...

A Quasi-3d Model of Electron Cyclotron Resonance Ion Source*

FAR-TECH, Inc. is developing a hybrid, quasi-three dimensional (Quasi-3D) model to simulate charge breeding of a test 1+ or 2+ ion beam in an electron cyclotron resonance ion source (ECRIS). The model is a combination of three dimensional (3D) mapping of the plasma background calculated by a 1D Generalised ECRIS Model (GEM-1D) [1] and 3D tracking of the ion trajectories with Monte Carlo Charge ...

Cyclotron Resonance and Quasiparticles

This introductory paper contains personal perspectives about the importance of cyclotron resonance in forming our modern view of solids. The papers following this one will discuss the discovery, refinements, and some of the latest developments. Although I will touch on some of these subjects, I leave the details to the other authors and in the main focus on the conceptual impact of the work. I ...

Cyclotron resonance revisited

Optics for electron cyclotron resonance heating and collective Thomson scattering at the stellarator W7-X

W. Kasparek, V. Erckmann, H.P. Laqua, T. Stange, M. Weißgerber, C. Lechte, B. Plaum, D. Moseev, F. Leipold, M. Petelin, K.J. Brunner, H. Braune, S. Marsen, N. Schneider, R.C. Wolf, and the W7-X team Institute of Interfacial Process Engineering and Plasma Technology, U. Stuttgart, Germany, [email protected] Max-Planck Institute of Plasma Physics (IPP), Garching and Greifswald, Germa...