Numerical simulation of astrophysical cyclotron-maser emission
Speirs, D. C. and McConville, S. L. and Gillespie, K. M. and Phelps, A.D.R. and Cross, A. W. and Ronald, K.; (2013) Numerical simulation of astrophysical cyclotron-maser emission. In: 2013 38th International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz, Mainz, Germany, 2013. IEEE, DEU. ISBN 9781467347174 (https://doi.org/10.1109/IRMMW-THz.2013.6665679)
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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.
ORCID iDs
Speirs, D. C. ORCID: https://orcid.org/0000-0001-5705-6126, McConville, S. L., Gillespie, K. M., Phelps, A.D.R. ORCID: https://orcid.org/0000-0002-1100-1012, Cross, A. W. ORCID: https://orcid.org/0000-0001-7672-1283 and Ronald, K. ORCID: https://orcid.org/0000-0002-8585-0746;-
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Item type: Book Section ID code: 71675 Dates: DateEvent11 December 2013PublishedNotes: © 2013 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting /republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works. Subjects: Science > Physics
Technology > Electrical engineering. Electronics Nuclear engineeringDepartment: Faculty of Science > Physics Depositing user: Pure Administrator Date deposited: 04 Mar 2020 14:25 Last modified: 11 Nov 2024 15:15 Related URLs: URI: https://strathprints.strath.ac.uk/id/eprint/71675