Comparative case study of delayed ionospheric response to a superposed 27-day solar rotation signal

IF 2.8 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Advances in Space Research Pub Date : 2025-02-01 DOI:10.1016/j.asr.2024.12.004
Hanna Dühnen , Rajesh Vaishnav , Christoph Jacobi , Erik Schmölter , Jens Berdermann
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Abstract

Major ionization processes in the upper atmosphere are driven by the solar extreme ultraviolet (EUV) radiation causing corresponding responses in ionospheric observables. The response to the 27-day solar rotation period is of particular interest, as this variation occurs with a delay, which depends on the level of solar and geomagnetic activity as well as atmospheric processes. The 27-day signature is also frequently superimposed with long-term variations, which further impact the length of the delay. For a better understanding of these interactions, the present study investigates the delayed response of ionospheric total electron content (TEC) and the concentrations of major neutral and ionized species. Using high-resolution simulations from the Thermosphere-Ionosphere-Electrodynamics General Circulation Model (TIE-GCM) and the Coupled Thermosphere Ionosphere Plasmasphere Electrodynamics (CTIPe) model, two distinct 27-day solar rotation periods from the high solar activity year of 2014 are analyzed. This comparison allows us to examine the effects of an ideal 27-day solar activity cycle alongside one characterized by increasing solar activity, while also comparing model results with observed IGS data. Our detailed analysis, based on TIE-GCM simulations, presents the ionospheric response for various ionized and neutral species across different altitudes and latitudes. Notably, we find that the accumulation of ionized species, such as O+ and O2+, in the lower ionosphere, particularly at approximately 230 km, where ionized oxygen density peaks—is significantly influenced by the long-term increase in solar activity. However, the 27-day solar rotation period predominantly governs ionization processes at altitudes above 230 km in both, ideal and complex model runs. Thus, our results are in good agreement with previous studies and extend the understanding of the delayed ionospheric response to more complex cases.
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延迟电离层响应叠加27天太阳旋转信号的比较案例研究
高层大气中的主要电离过程是由太阳极紫外线(EUV)辐射驱动的,在电离层观测中引起相应的响应。对27天太阳自转周期的响应是特别有趣的,因为这种变化是有延迟的,这取决于太阳和地磁活动的水平以及大气过程。27天的签名也经常与长期变化叠加,这进一步影响了延迟的长度。为了更好地理解这些相互作用,本研究研究了电离层总电子含量(TEC)和主要中性和电离物质浓度的延迟响应。利用热层-电离层-电动力学综合环流模型(TIE-GCM)和耦合热层-电离层-等离子体电动力学模型(CTIPe)的高分辨率模拟,分析了2014年太阳高活动年两个不同的27天太阳自转周期。这种比较使我们能够检查理想的27天太阳活动周期和以太阳活动增加为特征的太阳活动周期的影响,同时还将模型结果与观测到的IGS数据进行比较。在TIE-GCM模拟的基础上,我们详细分析了不同海拔和纬度的电离层对各种电离和中性物质的响应。值得注意的是,我们发现,在较低的电离层,特别是在大约230公里处,电离氧密度达到峰值的地方,电离物质(如O+和O2+)的积累受到太阳活动长期增加的显著影响。然而,在理想和复杂模型运行中,27天的太阳自转周期主要控制海拔230公里以上的电离过程。因此,我们的结果与先前的研究结果很好地一致,并将对延迟电离层响应的理解扩展到更复杂的情况。
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来源期刊
Advances in Space Research
Advances in Space Research 地学天文-地球科学综合
CiteScore
5.20
自引率
11.50%
发文量
800
审稿时长
5.8 months
期刊介绍: The COSPAR publication Advances in Space Research (ASR) is an open journal covering all areas of space research including: space studies of the Earth''s surface, meteorology, climate, the Earth-Moon system, planets and small bodies of the solar system, upper atmospheres, ionospheres and magnetospheres of the Earth and planets including reference atmospheres, space plasmas in the solar system, astrophysics from space, materials sciences in space, fundamental physics in space, space debris, space weather, Earth observations of space phenomena, etc. NB: Please note that manuscripts related to life sciences as related to space are no more accepted for submission to Advances in Space Research. Such manuscripts should now be submitted to the new COSPAR Journal Life Sciences in Space Research (LSSR). All submissions are reviewed by two scientists in the field. COSPAR is an interdisciplinary scientific organization concerned with the progress of space research on an international scale. Operating under the rules of ICSU, COSPAR ignores political considerations and considers all questions solely from the scientific viewpoint.
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