| dc.contributor.author | Schmitz, H | |
| dc.contributor.author | Tsiklauri, D | |
| dc.date.accessioned | 2013-07-15T11:03:50Z | |
| dc.date.available | 2013-07-15T11:03:50Z | |
| dc.date.issued | 2013-05-26 | |
| dc.identifier.citation | The effect of initial conditions on the electromagnetic radiation generation in type III solar radio bursts. H. Schmitz and D. Tsiklauri, Physics of Plasmas 20, 062903 (2013), DOI:10.1063/1.4812453 | |
| dc.identifier.issn | 1070-664X | |
| dc.identifier.issn | 1089-7674 | |
| dc.identifier.uri | http://qmro.qmul.ac.uk/xmlui/handle/123456789/4141 | |
| dc.description | Copyright 2013 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. This article appeared in Physics of Plasmas 20, 062903 (2013) and may be found at <http://pop.aip.org/resource/1/phpaen/v20/i6/p062903_s1>. | |
| dc.description.abstract | Extensive particle-in-cell simulations of fast electron beams injected in a background magnetised plasma with a decreasing density profile were carried out. These simulations were intended to further shed light on a newly proposed mechanism for the generation of electromagnetic waves in type III solar radio bursts [D. Tsiklauri, Phys. Plasmas, 18, 052903 (2011)]. The numerical simulations were carried out using different density profiles and fast electron distribution functions. It is shown that electromagnetic L and R modes are excited by the transverse current, initially imposed on the system. In the course of the simulations no further interaction of the electron beam with the background plasma could be observed. | |
| dc.title | The effect of initial conditions on the electromagnetic radiation generation in type III solar radio bursts | |
| dc.type | Journal Article | |
| dc.identifier.doi | 10.1063/1.4812453 | |
| dc.relation.isPartOf | Physics of Plasmas 20, 062903 (2013) | |
| pubs.author-url | http://arxiv.org/abs/1305.6038v1 | |
