| Issue |
E3S Web Conf.
Volume 62, 2018
IX International Conference “Solar-Terrestrial Relations and Physics of Earthquake Precursors”
|
|
|---|---|---|
| Article Number | 02004 | |
| Number of page(s) | 13 | |
| Section | Geophysical Fields and their Interactions | |
| DOI | https://doi.org/10.1051/e3sconf/20186202004 | |
| Published online | 07 November 2018 | |
Analysis of Whistlers Registration Data Obtained by Ssan System on Subauroral Station in Yakutsk
1 Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy of SB RAS, 677980, Republic of Sakha (Yakutia), Yakutsk, 31, Lenin ave., Russian Federation
2 Institute of Cosmophysical Research and Radio Wave Propagation of FEB RAS, 684034, Kamchatka region, Elizovskiy district, Paratunka, 7, Mirnaya str., Russian Federation
Since from November 2017 to August 2018, synchronous registration of atmospherics and whistlers at the radiophysical station “Oibenkyol”, began in the operational mode within the network SSAN/VLF (“Sensor signal analysis network/Very low frequency”). The classification and the characteristics of the registered whistlers are carried out. The correlation analysis of the number of the whistlers registered by the SSAN/VLF with the number of lightning registered by the WWLLN is used to determine the location of lightning sources of whistlers in the opposite hemisphere in the magnetoconjugate point at South of Australia. Thus, the SSAN/VLF make possible the distance monitoring of the dynamics of the various geophysical processes changes. The large number of registered nose whistlers allow performing the statistical analysis of processes occurring in the magnetosphere’ plasma.
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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