2018
DOI: 10.1016/j.jastp.2017.06.009
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The influence of tidal winds in the formation of blanketing sporadic e-layer over equatorial Brazilian region

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Cited by 30 publications
(56 citation statements)
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“…We used the MIRE originally developed by Carrasco (2005) and Carrasco et al (2007), which was modified by Resende et al (2017aResende et al ( , 2017b. The extended version of MIRE included two major modifications: (1) Inclusion of a new wind model that correctly describes the wind dynamic over the Brazilian region; and (2) the seasonal variability of the metallic ions in the Es layer formation.…”
Section: Mire Modelmentioning
confidence: 99%
See 1 more Smart Citation
“…We used the MIRE originally developed by Carrasco (2005) and Carrasco et al (2007), which was modified by Resende et al (2017aResende et al ( , 2017b. The extended version of MIRE included two major modifications: (1) Inclusion of a new wind model that correctly describes the wind dynamic over the Brazilian region; and (2) the seasonal variability of the metallic ions in the Es layer formation.…”
Section: Mire Modelmentioning
confidence: 99%
“…However, we performed some modifications in MIRE to obtain a more realistic wind profile. In fact, Resende et al (2017aResende et al ( , 2017b) considered a constant wavelength in their simulations. Here, we adjust a wavelength tending to infinity above 120 km.…”
Section: Meteor Radar Wind Datamentioning
confidence: 99%
“…CO 2 mixing ratios are taken as constant with height until 87.5 km, and then decrease exponentially. Chemical heating due to recombination of O 2 and O (Riese et al, 1994), and heating due to extreme ultraviolet radiation, are added. This is described in more detail by Fröhlich et al (2003a).…”
Section: Muam Circulation Model Predictionsmentioning
confidence: 99%
“…Sporadic layers (Es) are electron density enhancements which appear in the lower ionospheric E region at heights between 90 and 130 km with a typical thickness of less than 5 km. The layers consist mainly of metallic ions (Fe + , Mg + , Ca + and Na + ) deposited by meteoric ablation (Whitehead, 1961;Layzer, 1972). The metallic ions have longer lifetimes than the nonmetallic ionized air constituents (O + , NO + , O 2 + ), which allow the formation of long-lasting sporadic E layers (Kopp, 1997).…”
Section: Introductionmentioning
confidence: 99%