Equatorial Counter Electrojet Longitudinal and Seasonal Variability in the American Sector. Issue 11 (28th November 2018)

• Record Type: Journal Article
• Authors: Soares, Gabriel; Yamazaki, Yosuke; Matzka, Jürgen; Pinheiro, Katia; Morschhauser, Achim; Stolle, Claudia; Alken, Patrick
• Is Part Of: Journal of geophysical research. Volume 123:Issue 11(2018)
• Page Start: 9906
• Page End: 9920
• Publication Date: 2018-11-28
• Subjects: ground‐based geomagnetic data -- counter electrojet climatology -- atmospheric tides; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1029/2018JA025968
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: The equatorial electrojet occasionally reverses during morning and afternoon hours, leading to periods of westward current in the ionospheric E region that are known as counter electrojet (CEJ) events. We present the first analysis of CEJ climatology and CEJ dependence on solar flux and lunar phase for the Brazilian sector, based on an extensive ground‐based data set for the years 2008 to 2017 from the geomagnetic observatory Tatuoca (1.2°S, 48.5°W), and we compare it to the results found for Huancayo (12.0°S, 75.3°W) observatory in the Peruvian sector. We found a predominance of morning CEJ events for both sectors. The afternoon CEJ occurrence rate in the Brazilian sector is twice as high as in the Peruvian sector. The afternoon CEJ occurrence rate strongly depends on season, with maximum rates occurring during the northern‐hemisphere summer for the Brazilian sector and during the northern‐hemisphere winter for the Peruvian sector. Significant discrepancies between the two sectors are also found for morning CEJ rates during the northern‐hemisphere summer. These longitudinal differences are in agreement with a CEJ climatology derived from contemporary Swarm satellite data and can be attributed in part to the well‐known longitudinal wave‐4 structure in the background equatorial electrojet strength that results from nonmigrating solar tides and stationary planetary waves. Simulations with the Thermosphere‐Ionosphere‐Electrodynamics General Circulation Model show that the remaining longitudinal variability in CEJ during northern summer can be explained by the effect of migrating tides in the presence of the varying geomagnetic field in the South Atlantic Anomaly. Key Points: A 10‐year ground‐based data set was used to investigate counter electrojet climatology in the Brazilian sector for the first time A comparison with the Peruvian sector counter electrojet climatology reveals a longitudinal variability around the June solstice Besides the known wave‐4 structure, migrating tides play a role for the counter electrojet longitudinal dependence in South America