It appears you don't have support to open PDFs in this web browser. To view this file, Open with your PDF reader
Abstract
The equatorial Congo has been recognized as the most active lightning chimney region in the Globe. Although the perturbation of tropospheric thunderstorms on the lower ionosphere has been noticed in the middle latitudes through their transient lightning electric fields or convective gravity waves, the effects on equatorial ionosphere and the horizontal extent of this perturbation remains a mystery because of the difficulties in extracting the effects due to the sporadic nature of the equatorial ionosphere. Here we present observational results showing solid evidence of deviations in ionospheric total electron content (TEC) and its direction of propagation associated with thunderstorms using the method of polynomial filtering, by utilizing the TEC measured from equatorial Global Positioning System (GPS) Receiver stations along the West African region-Congo Basin. The TEC deviations due to the thunderstorms were found to be mostly propagated in a specific direction from the point of the event, with the highest absolute peak TEC at ~±1.5 TECUs. The internal dynamics of the equatorial ionosphere have been found to be suppressed by large thunderstorm effects during the daytime, with negligible impact at night.
You have requested "on-the-fly" machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Show full disclaimer
Neither ProQuest nor its licensors make any representations or warranties with respect to the translations. The translations are automatically generated "AS IS" and "AS AVAILABLE" and are not retained in our systems. PROQUEST AND ITS LICENSORS SPECIFICALLY DISCLAIM ANY AND ALL EXPRESS OR IMPLIED WARRANTIES, INCLUDING WITHOUT LIMITATION, ANY WARRANTIES FOR AVAILABILITY, ACCURACY, TIMELINESS, COMPLETENESS, NON-INFRINGMENT, MERCHANTABILITY OR FITNESS FOR A PARTICULAR PURPOSE. Your use of the translations is subject to all use restrictions contained in your Electronic Products License Agreement and by using the translation functionality you agree to forgo any and all claims against ProQuest or its licensors for your use of the translation functionality and any output derived there from. Hide full disclaimer
Details


1 Institute of Atmospheric Physics (IAP), Chinese Academy of Science, Key Laboratory for middle Atmosphere and Global Environment Observation (LAGEO), Beijing, China (GRID:grid.424023.3) (ISNI:0000 0004 0644 4737); Federal University of Technology, Department of Physics, Akure, Nigeria (GRID:grid.411257.4) (ISNI:0000 0000 9518 4324)
2 Institute of Atmospheric Physics (IAP), Chinese Academy of Science, Key Laboratory for middle Atmosphere and Global Environment Observation (LAGEO), Beijing, China (GRID:grid.424023.3) (ISNI:0000 0004 0644 4737)
3 Institute of Atmospheric Physics (IAP), Chinese Academy of Science, Key Laboratory for middle Atmosphere and Global Environment Observation (LAGEO), Beijing, China (GRID:grid.424023.3) (ISNI:0000 0004 0644 4737); University of Chinese Academy of Sciences, College of Earth and Planetary Sciences, Beijing, China (GRID:grid.410726.6) (ISNI:0000 0004 1797 8419)