By Juan G. Roederer

ISBN-10: 3642415296

ISBN-13: 9783642415296

ISBN-10: 364241530X

ISBN-13: 9783642415302

This booklet is a brand new version of Roederer’s vintage *Dynamics of Geomagnetically Trapped Radiation*, up-to-date and significantly increased. the most aim is to explain the dynamic houses of magnetically trapped debris in planetary radiation belts and plasmas and clarify the actual strategies concerned from the theoretical perspective. The technique is to ascertain intimately the orbital and adiabatic movement of person debris in common configurations of magnetic and electrical fields within the magnetosphere and, from there, derive easy beneficial properties of the debris’ collective “macroscopic” habit typically planetary environments. Emphasis isn't at the “what*”* yet at the “why*”* of particle phenomena in near-earth house, delivering an excellent and transparent figuring out of the crucial uncomplicated actual mechanisms and dynamic procedures concerned. The publication also will function an creation to basic area plasma physics, with ample easy examples to demonstrate and clarify the actual starting place of other different types of plasma present structures and their self-organizing personality through the magnetic box. the final word goal is to assist either graduate scholars and scientists to effectively face the theoretical and experimental demanding situations mendacity forward in house physics in view of modern and upcoming satellite tv for pc missions and an anticipated wealth of information on radiation belts and plasmas.

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**Extra info for Dynamics of Magnetically Trapped Particles: Foundations of the Physics of Radiation Belts and Space Plasmas**

**Example text**

This leads to energy levels of the order of hundreds of keV to thousands of MeV, for electrons trapped in extreme magnetic environments. n C / m0 2 n D 0; 1; 2;. . Considerations of quantum spin of the original particle and relativistic effects complicate somewhat the picture, but are outside the scope of this book. 3 Zero-Order Drifts We now consider the case of a charged particle in a uniform static magnetic field under the action of an external non-magnetic, non-inertial, interaction force F which is constant in time and space.

Note that for a force field, zero order drifts are a function of position r only—a vector field. We cannot independently impart some arbitrary zero order drift to a particle as an initial condition. One can easily understand the physical reasons for the drift of a charged particle under the action of a constant external force, perpendicular to B. As sketched in Fig. ) and decelerated by the external force F — v? is not constant during one turn (see below). It should be clear that in this case the magnetic moment cannot be defined in the OFR.

Considerations of quantum spin of the original particle and relativistic effects complicate somewhat the picture, but are outside the scope of this book. 3 Zero-Order Drifts We now consider the case of a charged particle in a uniform static magnetic field under the action of an external non-magnetic, non-inertial, interaction force F which is constant in time and space. We divide the force into two components F k and F ? , parallel and perpendicular to B, respectively. 1) can be split into the following pair: d pk D Fk dt d p?

### Dynamics of Magnetically Trapped Particles: Foundations of the Physics of Radiation Belts and Space Plasmas by Juan G. Roederer

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