Ionospheric Response to the Space Weather Events of 4-10 September 2017: First Chilean Observations
Manuel Bravo1, *, Carlos Villalobos2, Rodrigo Leiva3, Luis Tamblay4, Pedro Vega-Jorquera4, Elías Ovalle5, Alberto Foppiano5
Identifiers and Pagination:Year: 2019
First Page: 1
Last Page: 12
Publisher Id: TOASCJ-13-1
Article History:Received Date: 30/06/2019
Revision Received Date: 24/04/2019
Acceptance Date: 26/05/2019
Electronic publication date: 30/06/2019
open-access license: This is an open access article distributed under the terms of the Creative Commons Attribution 4.0 International Public License (CC-BY 4.0), a copy of which is available at: https://creativecommons.org/licenses/by/4.0/legalcode. This license permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
The diurnal variations of several ionospheric characteristics during the Space Weather Events of 4-10 September 2017, for Chilean latitudes, will be reported.
Materials and Methods:
Observations were made using a recently installed ionosonde at the Universidad de La Serena field station (29°52'S; 71°15’W). Also, reported is the total electron content determined using the upgraded Chilean network of dual-frequency Global Navigation Satellite Systems (GNSS) receivers.
Sudden ionospheric disturbances are described in terms of the minimum reflection frequency determined from ionosonde records. An attempt to derive the extent of the effect on high frequency propagation paths in the region is made using simultaneous ionosonde observations at other locations.
The geomagnetic storm ionospheric effects are discussed in detail using the observed diurnal variation of maximum electron concentration (NmF2), virtual height of the F-region (h’F/F2) and Total Electron Content (TEC). These are complemented with the time-latitude variation of TEC for the 70°W meridian.
It is found that large increases of NmF2, h’F/F2 and TEC observed during 8 September 2017 storm are well described in terms of the evolution of the Equatorial Ionospheric Anomaly (EIA) over the same time interval. Known physical mechanisms are suggested to explain most of the observations.