Marcio Muella, Ana P. M. Silva, Ângela M. dos Santos, V. Pillat, Laysa C. A. Resende, Vânia F. Andrioli, Paulo R. Fagundes
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Model simulations for SJC (October 2008) and PAL (April and June 2009) revealed distinct wind oscillations influencing IL dynamics at heights below 140 km. In SJC, meridional wind shears controlled IL descent, with possible zonal wind interactions weakening ILs. Conversely, in PAL during April 2009, both zonal and meridional winds contributed to IL formation and altitude descent. However, discrepancies between observed and modeled descent rates suggest the need for considering additional atmospheric wave interactions in future modeling studies. June 2009 over PAL presented unique IL behavior, exhibiting a lower observed decay rate and daily height oscillations potentially linked to local modulations. Meanwhile, MIRE indicated that meridional wind shearing predominantly controlled IL descent in the morning, with zonal wind becoming relevant post-midday. 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引用次数: 0
摘要
本研究通过观测和建模研究了巴西低纬度地区中间层(IL)的向下运动。对圣若泽多斯坎波斯(SJC)和帕尔马斯(PAL)的电离层探测仪数据进行了分析,以研究电离层参数的季节性变化,包括虚拟高度(h'IL)和顶部频率(ftIL)。IL 主要源于 F 层脱离后的向下运动,在 11 时前达到峰值,并在日落前消失。日高度变化范围在 130 至 190 千米之间,峰值频率约为 4-5 兆赫。利用流星雷达数据作为输入,电离层 E 区域模型模拟了昼夜潮汐和半昼夜潮汐,以分析中性风对 ILs 下降的影响。对上海合作组织(2008 年 10 月)和亚太地区(2009 年 4 月和 6 月)的模型模拟显示,在 140 公里以下的高度,影响电离层下降动力学的风振荡截然不同。在 SJC,经向风切变控制着 IL 的下降,可能的地带风相互作用削弱了 IL。相反,2009 年 4 月在 PAL,经向风和带风都对 IL 的形成和高度下降起了作用。然而,观测到的下降率与模拟的下降率之间的差异表明,在未来的模拟研究中需要考虑更多的大气波浪相互作用。2009 年 6 月,PAL 上空出现了独特的 IL 行为,观测到的衰减率较低,每日高度振荡可能与局部调制有关。同时,MIRE 显示,经向风切变在上午主要控制着 IL 的下降,而在中午以后则与带风有关。这些发现加深了我们对IL动力学及其大气驱动因素的理解。
Intermediate E-F layer dynamics study in the Brazilian low-latitude sector: observational data and simulations
This study investigates the downward motion of Intermediate E-F Layers (ILs) in the Brazilian low latitude sector through observation and modeling. Ionosonde data from São José dos Campos (SJC) and Palmas (PAL) were analyzed to investigate the seasonal variation of the IL parameters, including the virtual height (h'IL) and the top frequency (ftIL). The ILs primarily originated from F layer detachment followed by downward motion, peaking before 11 LT and disappearing well before sunset. Daily height variability ranged between 130 and 190 km, with peak frequencies around 4–5 MHz. Using meteor radar data as input, the Ionospheric E-region Model (MIRE) simulated diurnal and semidiurnal tides to analyze neutral wind effects on ILs descent. Model simulations for SJC (October 2008) and PAL (April and June 2009) revealed distinct wind oscillations influencing IL dynamics at heights below 140 km. In SJC, meridional wind shears controlled IL descent, with possible zonal wind interactions weakening ILs. Conversely, in PAL during April 2009, both zonal and meridional winds contributed to IL formation and altitude descent. However, discrepancies between observed and modeled descent rates suggest the need for considering additional atmospheric wave interactions in future modeling studies. June 2009 over PAL presented unique IL behavior, exhibiting a lower observed decay rate and daily height oscillations potentially linked to local modulations. Meanwhile, MIRE indicated that meridional wind shearing predominantly controlled IL descent in the morning, with zonal wind becoming relevant post-midday. These findings enhance our understanding of IL dynamics and their atmospheric drivers.