Numerical simulation of astrophysical cyclotron-maser emission

David C Speirs , Sandra L McConville , Karen Gillespie, Alan D R Phelps , Adrian W Cross , Kevin Ronald

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Numerical simulations have been conducted at the University of Strathclyde to study the spatial growth rate and emission topology of the cyclotron maser instability responsible for auroral magnetospheric radio emission from stars and planets and intense non-thermal radio emission in other astrophysical contexts. The results have significant bearing on the radiation propagation characteristics and highly debated question of escape from the source region.
Original languageEnglish
Title of host publication8th International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz
Number of pages2
Publication statusPublished - 2013
Externally publishedYes

Fingerprint

Dive into the research topics of 'Numerical simulation of astrophysical cyclotron-maser emission'. Together they form a unique fingerprint.

Cite this