{"title":"Day-To-Day Variability of Ionospheric Electron Temperature Revealed by High-Resolution SYISR Observations During April–May 2022","authors":"Zhongqiu Wang, Xinan Yue, Xu Zhou, Yihui Cai, Junyi Wang, Feng Ding, Jianhui He, Yonghui Wang, Ning Zhang, Junhao Luo, Mingyuan Li, Su Xu","doi":"10.1029/2024JA032863","DOIUrl":null,"url":null,"abstract":"<p>This study investigated the day-to-day variability of ionospheric electron temperature (<i>T</i><sub><i>e</i></sub>) over Sanya using the newly built Sanya Incoherent Scatter Radar (SYISR; 18.3°N, 109.6°E, dip latitude: 12.8°N). The 24 days of observations with transmitted beams encoded by the alternating code and directed toward the zenith provided <i>T</i><sub><i>e</i></sub> profiles during April–May 2022. The spatial-temporal resolution was as precise as 4.5 km and ∼120 s. The day-to-day variability of <i>T</i><sub><i>e</i></sub> over Sanya thus revealed, which was strong in the sunrise <i>T</i><sub><i>e</i></sub> peak region (above ∼260 km, duration increases from ∼0.5 to ∼3.5 hr with altitude) and the top of the 200–300 km <i>T</i><sub><i>e</i></sub> bulge (∼260 to ∼300 km, lasting from ∼09:00 LT to ∼18:30 LT). The day-to-day variability of <i>T</i><sub><i>e</i></sub> in the two regions could reach ∼26% and ∼16% of the average <i>T</i><sub><i>e</i></sub>, respectively. Although the day-to-day variability of <i>T</i><sub><i>e</i></sub> is negatively correlated with the variation of ionospheric electron densities (<i>N</i><sub><i>e</i></sub>) in general, a positive correlation still occurred during the daytime, especially at 400–480 km from ∼17:00 LT to ∼18:00 LT. Further Thermosphere Ionosphere Electrodynamics General Circulation Model simulations reproduced the positive correlation, which may result from the internal heat exchange between electrons, ions, and neutrals. The simulations suggested that the variation of solar radiation/geomagnetic activity contributes most to the daytime/sunrise day-to-day variability of <i>T</i><sub><i>e</i></sub> over Sanya.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 1","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2025-01-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA032863","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
本研究利用新建的三亚非相干散射雷达(SYISR;18.3°N,109.6°E,倾角纬度:12.8°N)研究了三亚上空电离层电子温度(Te)的日变化情况。在 2022 年 4 月至 5 月期间,利用交替码编码并指向天顶的发射波束进行了 24 天的观测,提供了 Te 剖面图。由此揭示了三亚上空 Te 的日变化,其中日出 Te 峰值区域变化强烈(在 ∼260 km 以上,持续时间从 ∼0.5 秒增加到 ∼3.5 秒)。5小时到∼3.5小时)和200-300千米Te凸起顶部(∼260到∼300千米,持续时间从∼09:00时到∼18:30时)。这两个区域的 Te 日变率分别达到平均 Te 的 26% 和 16%。虽然Te的日变化与电离层电子密度(Ne)的变化总体上呈负相关,但在白天仍呈正相关,特别是在400-480公里处,从17:00 LT到18:00 LT。进一步的热层电离层电动力学大气环流模式模拟再现了正相关,这可能是电子、离子和中子之间内部热交换的结果。模拟结果表明,太阳辐射/地磁活动的变化是造成三亚上空 Te 日间/日出日变化的主要原因。
Day-To-Day Variability of Ionospheric Electron Temperature Revealed by High-Resolution SYISR Observations During April–May 2022
This study investigated the day-to-day variability of ionospheric electron temperature (Te) over Sanya using the newly built Sanya Incoherent Scatter Radar (SYISR; 18.3°N, 109.6°E, dip latitude: 12.8°N). The 24 days of observations with transmitted beams encoded by the alternating code and directed toward the zenith provided Te profiles during April–May 2022. The spatial-temporal resolution was as precise as 4.5 km and ∼120 s. The day-to-day variability of Te over Sanya thus revealed, which was strong in the sunrise Te peak region (above ∼260 km, duration increases from ∼0.5 to ∼3.5 hr with altitude) and the top of the 200–300 km Te bulge (∼260 to ∼300 km, lasting from ∼09:00 LT to ∼18:30 LT). The day-to-day variability of Te in the two regions could reach ∼26% and ∼16% of the average Te, respectively. Although the day-to-day variability of Te is negatively correlated with the variation of ionospheric electron densities (Ne) in general, a positive correlation still occurred during the daytime, especially at 400–480 km from ∼17:00 LT to ∼18:00 LT. Further Thermosphere Ionosphere Electrodynamics General Circulation Model simulations reproduced the positive correlation, which may result from the internal heat exchange between electrons, ions, and neutrals. The simulations suggested that the variation of solar radiation/geomagnetic activity contributes most to the daytime/sunrise day-to-day variability of Te over Sanya.