No CrossRef data available.
Article contents
Particle Acceleration in Spherical Wave Fields
Published online by Cambridge University Press: 27 September 2017
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
A magnet rotating in vacuo with its vector of angular velocity ω perpendicular to its vector of magnetic dipole moment μ is able to act as a particle accelerator. The dynamic features involved may be relevant for the understanding of rotating magnetized neutron stars as cosmic accelerators (Thielheim 1989) and may be useful for the designing of new mechanisms for accelerating devices.
- Type
- Part III Magnetospheric models
- Information
- Copyright
- Copyright © United States Naval Observatory 1992
You have
Access