An empirical model of the ionospheric sporadic E layer based on GNSS radio occultation data

B Yu, X Xue, CJ Scott, X Yue, X Dou - Space weather, 2022 - Wiley Online Library
The intense plasma irregularities within the ionospheric sporadic E (Es) layers at 90–130 km
altitude have a significant impact on radio communications and navigation systems. As a …

Estimation model of global ionospheric irregularities: an artificial intelligence approach

P Tian, B Yu, H Ye, X Xue, J Wu, T Chen - Space weather, 2022 - Wiley Online Library
The ionospheric sporadic E layer, the ionospheric irregularities of enhanced electron
density, appears in the Earth's ionosphere at altitudes between 90 and 120 km, which …

Tianwen-1 and MAVEN Observations of the Response of Mars to an Interplanetary Coronal Mass Ejection

B Yu, Y Chi, M Owens, CJ Scott, C Shen… - The Astrophysical …, 2023 - iopscience.iop.org
Interplanetary coronal mass ejections (ICMEs) are solar transients that have significant
effects on the upper atmosphere and ionosphere of Mars. The simultaneous spacecraft …

Ionospheric oscillation with periods of 6–30 days at middle latitudes: A response to solar radiative, geomagnetic, and lower atmospheric forcing

Z Yang, SY Gu, Y Qin, CKM Teng, Y Wei, X Dou - Remote Sensing, 2022 - mdpi.com
This research studies the medium timescale (6–30 days) ionospheric response over the
Wuhan area to solar radiative, recurrent geomagnetic, and lower atmospheric forcing. The …

Worldwide study of the Sporadic E (Es) layer development during a space weather event

LCA Resende, Y Zhu, CM Denardini, J Moro… - Journal of Atmospheric …, 2022 - Elsevier
This work analyzes the worldwide development of Sporadic E (Es) layers in different regions
during a High-Speed Solar Wind Stream (HSS) event on March 18, 2018. We used …

Predictive Capabilities of Corotating Interaction Regions Using STEREO and Wind In‐Situ Observations

Y Chi, C Shen, C Scott, M Xu, M Owens… - Space …, 2022 - Wiley Online Library
Solar wind stream interaction regions (SIRs) and corotating interaction regions (CIRs) can
cause geomagnetic storms and change energetic particle environment, ionospheric …

Intensity of 27-day variations in solar emission and ionospheric electron content

A Setov, K Ratovsky, L Kashapova - Advances in Space Research, 2024 - Elsevier
The rotation of the Sun modulates solar emission with 27-day variations. Large-scale
structures in the solar atmosphere, like sunspots and plages, rotate with the Sun and emit at …

The characteristics and simulation of sporadic E layers in ascending and descending phases of the solar cycle at mid‐latitude stations

Y Zhang, H Peng, R Jin, H Li, Y Hu… - Journal of …, 2025 - Wiley Online Library
Most of the attention was paid to the correlation between Sporadic E (Es) layers and solar
activity, and conflicting conclusions were obtained in previous research. For the first time, we …

Prediction interval of interface regions: Machine learning nowcasting approach

K Alielden, E Camporeale, MB Korsós… - Space …, 2023 - Wiley Online Library
Stream interaction region (SIR) is one of the space weather phenomena that accelerates the
upstream particles of the interface region in interplanetary space and causes geomagnetic …

Prediction for Arrival Time and Parameters of Corotation Interaction Regions using Earth–Mars Correlated Events from Tianwen-1, MAVEN, and Wind Observations

Z Zhong, C Shen, Y Chi, D Mao, B Miao… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract Using the Stream Interaction Regions list from the Tianwen-1/Mars Orbiter
Magnetometer (MOMAG) data between 2021 November and 2021 December and from …