TY - JOUR A1 - Soares, Gabriel A1 - Yamazaki, Yosuke A1 - Matzka, Jürgen A1 - Pinheiro, Katia A1 - Morschhauser, Achim A1 - Stolle, Claudia A1 - Alken, Patrick T1 - Equatorial counter electrojet longitudinal and seasonal variablity in the American sector JF - Journal of geophysical research : Space physics N2 - 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 degrees S, 48.5 degrees W), and we compare it to the results found for Huancayo (12.0 degrees S, 75.3 degrees 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. Y1 - 2018 U6 - https://doi.org/10.1029/2018JA025968 SN - 2169-9380 SN - 2169-9402 VL - 123 IS - 11 SP - 9906 EP - 9920 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Soares, Gabriel Brando A1 - Yamazaki, Yosuke A1 - Cnossen, Ingrid A1 - Matzka, Jürgen A1 - Pinheiro, Katia J. A1 - Morschhauser, Achim A1 - Alken, Patrick A1 - Stolle, Claudia T1 - Evolution of the geomagnetic daily variation at Tatuoca, Brazil, From 1957 to 2019 BT - a transition from Sq to EEJ JF - Journal of geophysical research : Space physics N2 - The magnetic equator in the Brazilian region has moved over 1,100 km northward since 1957, passing the geomagnetic observatory Tatuoca (TTB), in northern Brazil, around 2013. We recovered and processed TTB hourly mean values of the geomagnetic field horizontal (H) component from 1957 until 2019, allowing the investigation of long-term changes in the daily variation due to the influence of secular variation, solar activity, season, and lunar phase. The H day-to-day variability and the occurrence of the counter electrojet at TTB were also investigated. Until the 1990s, ionospheric solar quiet currents dominated the quiet-time daily variation at TTB. After 2000, the magnitude of the daily variation became appreciably greater due to the equatorial electrojet (EEJ) contribution. The H seasonal and day-to-day variability increased as the magnetic equator approached, but their amplitudes normalized to the average daily variation remained at similar levels. Meanwhile, the amplitude of the lunar variation, normalized in the same way, increased from 5% to 12%. Within the EEJ region, the occurrence rate of the morning counter electrojet (MCEJ) increased with proximity to the magnetic equator, while the afternoon counter electrojet (ACEJ) did not. EEJ currents derived from CHAMP and Swarm satellite data revealed that the MCEJ rate varies with magnetic latitude within the EEJ region while the ACEJ rate is largely constant. Simulations with the Thermosphere-Ionosphere-Electrodynamics General Circulation Model based on different geomagnetic main field configurations suggest that long-term changes in the geomagnetic daily variation at TTB can be attributed to the main field secular variation. Y1 - 2020 U6 - https://doi.org/10.1029/2020JA028109 SN - 2169-9380 SN - 2169-9402 VL - 125 IS - 9 PB - American Geophysical Union CY - Washington ER - TY - JOUR A1 - Soares, Gabriel A1 - Yamazaki, Yosuke A1 - Matzka, Jürgen A1 - Pinheiro, Katia A1 - Stolle, Claudia A1 - Alken, Patrick A1 - Yoshikawa, Akimasa A1 - Uozumi, Teiji A1 - Fujimoto, Akiko A1 - Kulkarni, Atul T1 - Longitudinal variability of the equatorial counter electrojet during the solar cycle 24 JF - Studia geophysica et geodaetica N2 - Ground and space-based geomagnetic data were used in the investigation of the longitudinal, seasonal and lunar phase dependence of the equatorial counter electrojet (CEJ) occurrence in the Peruvian, Brazilian, African, Indian and Philippine sectors during geomagnetically quiet days from the solar cycle 24 (2008 to 2018). We found that CEJ events occur more frequently during the morning (MCEJ) than in the afternoon (ACEJ). The highest MCEJ and ACEJ occurrence rates were observed for the Brazilian sector. Distinct seasonal dependence was found for each longitudinal sector under investigation. The lunar phase dependence was determined for the first time for the Philippine sector (longitude 125 degrees E), and it was shown to be less pronounced than in the Peruvian, Brazilian and African sectors. We demonstrate that differences in CEJ rates derived from ground-based and satellite data can arise from the longitudinal separation between low-latitude and equatorial stations that are used to determine the signal and its consequent time delay in their sunrise/sunset times at ionospheric heights. KW - geomagnetism KW - equatorial ionosphere KW - geomagnetic observatories KW - satellite data Y1 - 2019 U6 - https://doi.org/10.1007/s11200-018-0286-0 SN - 0039-3169 SN - 1573-1626 VL - 63 IS - 2 SP - 304 EP - 319 PB - Springer CY - New York ER - TY - JOUR A1 - Ruszkiewicz, Joanna A. A1 - de Macedo, Gabriel Teixeira A1 - Miranda-Vizuete, Antonio A1 - Bowman, Aaron B. A1 - Bornhorst, Julia A1 - Schwerdtle, Tanja A1 - Antunes Soares, Felix A. A1 - Aschner, Michael T1 - Sex-Specific response of caenorhabditis elegans to Methylmercury Toxicity JF - Neurotoxicity Research N2 - Methylmercury (MeHg), an abundant environmental pollutant, has long been known to adversely affect neurodevelopment in both animals and humans. Several reports from epidemiological studies, as well as experimental data indicate sex-specific susceptibility to this neurotoxicant; however, the molecular bases of this process are still not clear. In the present study, we used Caenorhabditis elegans (C. elegans), to investigate sex differences in response to MeHg toxicity during development. Worms at different developmental stage (L1, L4, and adult) were treated with MeHg for 1h. Lethality assays revealed that male worms exhibited significantly higher resistance to MeHg than hermaphrodites, when at L4 stage or adults. However, the number of worms with degenerated neurons was unaffected by MeHg, both in males and hermaphrodites. Lower susceptibility of males was not related to changes in mercury (Hg) accumulation, which was analogous for both wild-type (wt) and male-rich him-8 strain. Total glutathione (GSH) levels decreased upon MeHg in him-8, but not in wt. Moreover, the sex-dependent response of the cytoplasmic thioredoxin system was observedmales exhibited significantly higher expression of thioredoxin TRX-1, and thioredoxin reductase TRXR-1 expression was downregulated upon MeHg treatment only in hermaphrodites. These outcomes indicate that the redox status is an important contributor to sex-specific sensitivity to MeHg in C. elegans. KW - Methylmercury KW - Sex KW - Male KW - C KW - elegans KW - Antioxidant KW - Thioredoxin Y1 - 2019 U6 - https://doi.org/10.1007/s12640-018-9949-4 SN - 1029-8428 SN - 1476-3524 VL - 35 IS - 1 SP - 208 EP - 216 PB - Springer CY - New York ER -