Can One Predict Coronal Mass Ejection Arrival Times With Thirty‐Minute Accuracy? by Gábor Tóth, Bart van derHolst, Ward Manchester IV

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Erratum: “Solar Wind Driven from GONG Magnetograms in the Last Solar Cycle” (2024, ApJ, 965, 1) by Zhenguang Huang, Gábor Tóth, Nishtha Sachdeva, Bart van der Holst

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Solar Wind Driven from GONG Magnetograms in the Last Solar Cycle by Zhenguang Huang, Gábor Tóth, Nishtha Sachdeva, Bart van der Holst

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Consequences of Hot Electrons for the Structure of the Outer Heliosphere by Ethan Schuyler Bair, Merav Opher, Marc Zachary Kornbleuth, Bertalan Zieger, Gabor Toth, Bart van der Holst

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Modeling the Solar Wind during Different Phases of the Last Solar Cycle by Zhenguang Huang, Gábor Tóth, Nishtha Sachdeva, Lulu Zhao, Bart van der Holst, Igor Sokolov, Ward B. Manchester, Tamas I. Gombosi

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Erratum: “Modeling the Solar Wind during Different Phases of the Last Solar Cycle” (2023, ApJL, 946, L47) by Zhenguang Huang, Gábor Tóth, Nishtha Sachdeva, Lulu Zhao, Bart van der Holst, Igor Sokolov, Ward B. Manchester, Tamas I. Gombosi

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Decent Estimate of CME Arrival Time From a Data‐Assimilated Ensemble in the Alfvén Wave Solar Atmosphere Model (DECADE‐AWSoM) by Hongfan Chen, Nishtha Sachdeva, Zhenguang Huang, Bart van derHolst, Ward Manchester IV, Aniket Jivani, Shasha Zou, Yang Chen, Xun Huan, Gabor Toth

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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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