High‐Speed Solar Wind Imprints on the Ionosphere During the Recovery Phase of the August 2018 Geomagnetic Storm by Dexin Ren, Jiuhou Lei, Su Zhou, Wenbo Li, Fuqing Huang, Xiaoli Luan, Tong Dang, Yu Liu

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Influences of Solar Wind Parameters on Energetic Electron Fluxes at Geosynchronous Orbit Revealed by the Deep SHAP Method by Jianhang Wang, Zheng Xiang, Binbin Ni, Deyu Guo, Yangxizi Liu, Junhu Dong, Jingle Hu, Haozhi Guo

“…Backpropagating the prediction results of this ANN model from 2011 to 2020, SHAP values for four solar wind parameters (interplanetary magnetic field (IMF) BZ, solar wind speed, solar wind dynamic pressure, and proton density) are calculated and comprehensively analyzed. …”
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Beyond Basic Drag in Interplanetary CME Modeling: Effects of Solar Wind Pileup and High‐Speed Streams by C. Kay, T. Nieves‐Chinchilla, S. J. Hofmeister, E. Palmerio

“…As a fast CME propagates through interplanetary space, it accumulates solar wind materials at its front. This pileup of materials, or CME‐driven sheath, can be important in determining the geoeffectiveness of a CME. …”
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Prediction of Solar Wind Speed Through Machine Learning From Extrapolated Solar Coronal Magnetic Field by Rong Lin, Zhekai Luo, Jiansen He, Lun Xie, Chuanpeng Hou, Shuwei Chen

Subjects: “…solar wind speed…”
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A Parametric Study of Performance of Two Solar Wind Velocity Forecasting Models During 2006–2011 by Sandeep Kumar, Nandita Srivastava

Subjects: “…solar wind…”
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Radial Evolution of Interplanetary Shock Properties with Heliospheric Distance: Observations from Parker Solar Probe by Oksana Kruparova, Adam Szabo, Lan K. Jian, František Němec, Jana Šafránková, Zdeněk Němeček, Jacob Pasanen, Ayris Narock, Vratislav Krupar

Subjects: “…Solar wind…”
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Analytical Verification of the Normal Vector Determination Methods for Planar Magnetic Structures by Wai-Leong Teh

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Linear analysis of bump on tail instability with non-Maxwellian distribution function by Noreen, N, Shiekh, A, Habumugisha, I, Zaheer, S, AShah, H

Subjects: “…solar wind, Instability, Growth rate…”
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Forecasting GOES 15 >2 MeV Electron Fluxes From Solar Wind Data and Geomagnetic Indices by C. Forsyth, C. E. J. Watt, M. K. Mooney, I. J. Rae, S. D. Walton, R. B. Horne

“…Forecasts from AL give the highest skill scores for forecasts of up to 6 days. AL, solar wind pressure, or SYM‐H give the highest skill scores over 7–10 days. …”
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Attention‐Based Machine Vision Models and Techniques for Solar Wind Speed Forecasting Using Solar EUV Images by Edward J. E. Brown, Filip Svoboda, Nigel P. Meredith, Nicholas Lane, Richard B. Horne

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Double Superposed Epoch Analysis of Geomagnetic Storms and Corresponding Solar Wind and IMF in Solar Cycles 23 and 24 by V. Manu, N. Balan, Qing‐He Zhang, Zan‐Yang Xing

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Worst‐Case Severe Environments for Surface Charging Observed at LANL Satellites as Dependent on Solar Wind and Geomagnetic Conditions by N. Yu Ganushkina, B. Swiger, S. Dubyagin, J.‐C. Matéo‐Vélez, M. W. Liemohn, A. Sicard, D. Payan

“…Appearances of severe environments for surface charging do not necessarily require high values of Kp (Planetarische Kennziffer) and no storm is needed for such an event to be detected. Among solar wind parameters, solar wind velocity Vsw is directly related to the highest risk of severe environments, dependent on the Vsw value; and number density Nsw is of no importance. …”
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Global Sensitivity Analysis and Uncertainty Quantification for Background Solar Wind Using the Alfvén Wave Solar Atmosphere Model by Aniket Jivani, Nishtha Sachdeva, Zhenguang Huang, Yang Chen, Bart van derHolst, Ward Manchester, Daniel Iong, Hongfan Chen, Shasha Zou, Xun Huan, Gabor Toth

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Solar Wind With Field Lines and Energetic Particles (SOFIE) Model: Application to Historical Solar Energetic Particle Events by Lulu Zhao, Igor Sokolov, Tamas Gombosi, David Lario, Kathryn Whitman, Zhenguang Huang, Gabor Toth, Ward Manchester, Bart van derHolst, Nishtha Sachdeva, Weihao Liu

“…Abstract In this paper, we demonstrate the applicability of the data‐driven solar energetic particle (SEP) model, SOlar‐wind with FIeld‐lines and Energetic‐particles (SOFIE), to simulate the acceleration and transport processes of SEPs and make forecast of the energetic proton flux at energies ≥10 MeV that will be observed near 1 AU. …”
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An Adaptive X‐Ray Dynamic Image Estimation Method Based on OMNI Solar Wind Parameters and SXI Simulated Observations by R. C. Wang, Anders M. Jorgensen, Dalin Li, Tianran Sun, Zhen Yang, Xiaodong Peng

“…Abstract Observations of the overall interactions between solar wind and the Earth's magnetosphere are crucial for space weather monitoring. …”
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Nighttime Geomagnetic Response to Jumps of Solar Wind Dynamic Pressure: A Possible Cause of Québec Blackout in March 1989 by T. Zhang, Y. Ebihara, T. Tanaka

“…Abstract By performing a global magnetohydrodynamic (MHD) simulation, we investigated magnetic disturbances on the ground at high‐latitudes in response to jumps in the solar wind dynamic pressure, namely a sudden commencement (SC). …”
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Positive-Sum Game-Based Capacity Configuration Planning Method of Solar-Wind-Battery System Designed for Black-Start by Hejun Yang, Zhibo Liu, Yinghao Ma

“…The participation of the solar-wind-battery renewable energy system (SWBS) in black-start can improve the resilience of the power grid. …”
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Quasi-parallel Antisunward-propagating Whistler Waves Associated with the Electron Deficit in the Near-Sun Solar Wind: Particle-in-cell Simulation by Alfredo Micera, Daniel Verscharen, Jesse T. Coburn, Maria Elena Innocenti

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Characteristics of the IBEX Ribbon and Their Implications for a Source Region Outside the Heliopause by Sung Jun Noh, Daniel B. Reisenfeld, Lauren J. Beesley, Yue Chen, Fan Guo, Herbert O. Funsten, Paul H. Janzen, Thomas K. Kim, Asher Merrill, Dave Osthus, Nehpreet K. Walia, Eric J. Zirnstein

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Assessing the Influence of Input Magnetic Maps on Global Modeling of the Solar Wind and CME‐Driven Shock in the 2013 April 11 Event by Meng Jin, Nariaki V. Nitta, Christina M. S. Cohen

“…Abstract In the past decade, significant efforts have been made in developing physics‐based solar wind and coronal mass ejection (CME) models, which have been or are being transferred to national centers (e.g., SWPC, Community Coordinated Modeling Center) to enable space weather predictive capability. …”
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