DocumentCode :
126517
Title :
Generation of unusually low frequency plasmaspheric hiss
Author :
Lunjin Chen ; Thorne, R.M. ; Bortnik, Jacob ; Wen Li ; Horne, Richard B.
Author_Institution :
Dept. of Phys., Univ. of Texas at Dallas, Richardson, TX, USA
fYear :
2014
fDate :
16-23 Aug. 2014
Firstpage :
1
Lastpage :
4
Abstract :
Plasmaspheric hiss is an incoherent, broadband electromagnetic whistler-mode emission, preferentially and steadily observed inside high-density plasmasphere and storm-time plasmaspheric plume [1-2]. The frequency of plasmaspheric hiss typically ranges between ~200 Hz and 2 kHz, with peak wave power in a few 100s Hz. It has been recently proposed [3] that the dominant source of this emission is coherent chorus waves generated outside the plasmasphere. Subsequent ray tracing simulations [4] by tracing million rays of chorus waves reproduced a realistically spatial and spectral distribution of plasmaspheric hiss [Figure 1], showing the spatial confinement of plasmaspheric hiss emission within the plasmapause, and the typical frequency range from 200 Hz and 2 kHz with peak intensity around 500-700 Hz. It is worth pointing out that there is little hiss emission below 200 Hz in the simulation, indicating the chorus-as-embryonic-source mechanism does not work for such low frequency because chorus waves at those frequencies cannot propagate inward into the plasmasphere without substantial attenuations.
Keywords :
magnetospheric electromagnetic wave propagation; radiowave propagation; ray tracing; chorus-as-embryonic-source mechanism; coherent chorus wave emission; high-density plasmasphere; incoherent broadband electromagnetic whistler-mode emission; plasmapause; ray tracing; spatial confinement; spatial distribution; spectral distribution; storm-time plasmaspheric plume; unusually low frequency plasmaspheric hiss generation; Electronic mail; Gain; Magnetic fields; Plasma density; Probes; Ray tracing; Time-frequency analysis;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
General Assembly and Scientific Symposium (URSI GASS), 2014 XXXIth URSI
Conference_Location :
Beijing
Type :
conf
DOI :
10.1109/URSIGASS.2014.6929883
Filename :
6929883
Link To Document :
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