{"title":"漠河站和北京站 G 条件期间热层外层温度响应案例研究","authors":"Shaoyang Li, Zhipeng Ren, Tingting Yu, Biqiang Zhao, Libo Liu, Guozhu Li, Xinan Yue, Yong Wei, Lianhuan Hu","doi":"10.1029/2024JA032653","DOIUrl":null,"url":null,"abstract":"<p>The G-condition (NmF<sub>2</sub> ≤ NmF<sub>1</sub>) was observed by ground-based ionosondes at Mohe and Beijing during the geomagnetic storm occurred on 23 and 24 April 2023. We studied exospheric temperature (Tex) responses during the G-condition. Tex was derived from electron density (Ne) profiles (∼150–200 km) by the method proposed by Li et al. (2023, https://doi.org/10.1029/2022ja030988). The retrieved Tex showed obvious enhancements, with relative deviation of ∼10%–35% and ∼3%–20% at Mohe and Beijing, respectively. Additionally, chemical reaction rate increased by ∼15%–100% and ∼13%–30%, and O/N<sub>2</sub> decreased by ∼17%–35% and ∼23%–30% at Mohe and Beijing, respectively. Under photochemical equilibrium assumption, peak Ne is inversely proportional to chemical reaction rate and proportional to O/N<sub>2</sub>. Increased chemical reaction rate and decreased O/N<sub>2</sub> indicate a decrease in peak Ne. Compared to the increased Tex, the relative enhancement in Tex is more significantly associated with the G-condition, with relative deviation above ∼10% during the G-condition.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"129 10","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2024-10-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A Case Study of Thermospheric Exospheric Temperature Responses During the G-Condition at Mohe and Beijing Stations\",\"authors\":\"Shaoyang Li, Zhipeng Ren, Tingting Yu, Biqiang Zhao, Libo Liu, Guozhu Li, Xinan Yue, Yong Wei, Lianhuan Hu\",\"doi\":\"10.1029/2024JA032653\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The G-condition (NmF<sub>2</sub> ≤ NmF<sub>1</sub>) was observed by ground-based ionosondes at Mohe and Beijing during the geomagnetic storm occurred on 23 and 24 April 2023. We studied exospheric temperature (Tex) responses during the G-condition. Tex was derived from electron density (Ne) profiles (∼150–200 km) by the method proposed by Li et al. (2023, https://doi.org/10.1029/2022ja030988). The retrieved Tex showed obvious enhancements, with relative deviation of ∼10%–35% and ∼3%–20% at Mohe and Beijing, respectively. Additionally, chemical reaction rate increased by ∼15%–100% and ∼13%–30%, and O/N<sub>2</sub> decreased by ∼17%–35% and ∼23%–30% at Mohe and Beijing, respectively. Under photochemical equilibrium assumption, peak Ne is inversely proportional to chemical reaction rate and proportional to O/N<sub>2</sub>. Increased chemical reaction rate and decreased O/N<sub>2</sub> indicate a decrease in peak Ne. Compared to the increased Tex, the relative enhancement in Tex is more significantly associated with the G-condition, with relative deviation above ∼10% during the G-condition.</p>\",\"PeriodicalId\":15894,\"journal\":{\"name\":\"Journal of Geophysical Research: Space Physics\",\"volume\":\"129 10\",\"pages\":\"\"},\"PeriodicalIF\":2.6000,\"publicationDate\":\"2024-10-07\",\"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/10.1029/2024JA032653\",\"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}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA032653","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
在 2023 年 4 月 23 日和 24 日发生的地磁暴期间,漠河和北京的地基电离层探测仪观测到了 G 条件(NmF2 ≤ NmF1)。我们研究了地磁条件下大气层外温度(Tex)的响应。Tex是根据电子密度(Ne)剖面(∼150-200 km),按照Li等人(2023,https://doi.org/10.1029/2022ja030988)提出的方法得出的。获取的 Tex 值明显增强,在漠河和北京的相对偏差分别为 10%~35%和 3%~20%。此外,漠河和北京的化学反应速率分别增加了 15%~100%和 13%~30%,O/N2 分别减少了 17%~35%和 23%~30%。在光化学平衡假设下,峰值 Ne 与化学反应速率成反比,与 O/N2 成正比。化学反应速率的增加和 O/N2 的降低表明 Ne 峰值的降低。与 Tex 的增加相比,Tex 的相对增加与 G 条件的关系更为显著,在 G 条件下,Tex 的相对偏差超过 ∼10%。
A Case Study of Thermospheric Exospheric Temperature Responses During the G-Condition at Mohe and Beijing Stations
The G-condition (NmF2 ≤ NmF1) was observed by ground-based ionosondes at Mohe and Beijing during the geomagnetic storm occurred on 23 and 24 April 2023. We studied exospheric temperature (Tex) responses during the G-condition. Tex was derived from electron density (Ne) profiles (∼150–200 km) by the method proposed by Li et al. (2023, https://doi.org/10.1029/2022ja030988). The retrieved Tex showed obvious enhancements, with relative deviation of ∼10%–35% and ∼3%–20% at Mohe and Beijing, respectively. Additionally, chemical reaction rate increased by ∼15%–100% and ∼13%–30%, and O/N2 decreased by ∼17%–35% and ∼23%–30% at Mohe and Beijing, respectively. Under photochemical equilibrium assumption, peak Ne is inversely proportional to chemical reaction rate and proportional to O/N2. Increased chemical reaction rate and decreased O/N2 indicate a decrease in peak Ne. Compared to the increased Tex, the relative enhancement in Tex is more significantly associated with the G-condition, with relative deviation above ∼10% during the G-condition.