299 citations as recorded by crossref.

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5. A New Tool for CME Arrival Time Prediction using Machine Learning Algorithms: CAT-PUMA J. Liu et al. 10.3847/1538-4357/aaae69
6. CME Propagation Characteristics from Radio Observations S. Pohjolainen et al. 10.1007/s11207-007-9006-6
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9. A New Prediction Method for the Arrival Time of Interplanetary Shocks X. Feng & X. Zhao 10.1007/s11207-006-0185-3
10. ElEvoHI: A NOVEL CME PREDICTION TOOL FOR HELIOSPHERIC IMAGING COMBINING AN ELLIPTICAL FRONT WITH DRAG-BASED MODEL FITTING T. Rollett et al. 10.3847/0004-637X/824/2/131
11. 4π Models of CMEs and ICMEs (Invited Review) J. Kleimann 10.1007/s11207-012-9994-8
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19. On the Expansion Speed of Coronal Mass Ejections: Implications for Self-Similar Evolution L. Balmaceda et al. 10.1007/s11207-020-01672-6
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21. Analysis and study of the in situ observation of the June 1st 2008 CME by STEREO T. Nieves-Chinchilla et al. 10.1016/j.jastp.2010.09.026
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32. What Is the Nature of EUV Waves? First STEREO 3D Observations and Comparison with Theoretical Models S. Patsourakos et al. 10.1007/s11207-009-9386-x
33. Determining CME parameters by fitting heliospheric observations: Numerical investigation of the accuracy of the methods N. Lugaz et al. 10.1016/j.asr.2011.03.015
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36. Magnetic Flux Emergence, Activity, Eruptions and Magnetic Clouds: Following Magnetic Field from the Sun to the Heliosphere L. van Driel-Gesztelyi & J. Culhane 10.1007/s11214-008-9461-x
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41. Distribution and recovery phase of geomagnetic storms during solar cycles 23 and 24 W. Mishra et al. 10.1093/mnras/stae1045
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45. Expansion-induced Three-part Morphology of the 2021 December 4 Coronal Mass Ejection L. Yang et al. 10.3847/1538-4357/adb313
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52. Predicting Arrival Times of the CCMC CME/Shock Events Based on the SPM3 Model Y. Liang 梁 et al. 10.3847/1538-4357/ad84f0
53. Microwave radio emissions as a proxy for coronal mass ejection speed in arrival predictions of interplanetary coronal mass ejections at 1 AU C. Matamoros et al. 10.1051/swsc/2016038
54. Effects of ICMEs on High Energetic Particles as Observed by the Global Muon Detector Network (GMDN) A. Dal Lago et al. 10.1017/S1743921318000066
55. CME Disturbance Forecasting G. Siscoe & R. Schwenn 10.1007/s11214-006-9024-y
56. Impacts of CMEs on Earth Based on Logistic Regression and Recommendation Algorithm Y. Shi et al. 10.34133/2022/9852185
57. Source region of the 18 November 2003 coronal mass ejection that led to the strongest magnetic storm of cycle 23 N. Srivastava et al. 10.1029/2008JA013845
58. IMPULSIVE ACCELERATION OF CORONAL MASS EJECTIONS. I. STATISTICS AND CORONAL MASS EJECTION SOURCE REGION CHARACTERISTICS B. Bein et al. 10.1088/0004-637X/738/2/191
59. A Statistical Study of Solar Filament Eruptions that Form High-speed Coronal Mass Ejections P. Zou et al. 10.3847/1538-4357/ab4355
60. Estimation of Transit Time of CMEs from the Sun to Earth A. Pattnaik et al. 10.3847/1538-4357/adb84b
61. Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure V. Parhomov et al. 10.12737/stp-73202102
62. CORONAL MASS EJECTION DYNAMICS REGARDING RADIAL AND EXPANSION SPEEDS N. Rigozo et al. 10.1088/0004-637X/738/1/107
63. 3D Reconstruction of the Leading Edge of the 20 May 2007 Partial Halo CME N. Srivastava et al. 10.1007/s11207-009-9423-9
64. The Effect of the Heliospheric Current Sheet on Interplanetary Shocks Y. Xie et al. 10.1007/s11207-006-0227-x
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66. A kinematically distorted flux rope model for magnetic clouds M. Owens et al. 10.1029/2005JA011460
67. Investigation of geo-effective properties of halo coronal mass ejections S. Bhardwaj et al. 10.2205/2018ES000620
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69. Relationships Between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Rising Phase of Solar Cycles 23 and 24 M. Lawrance et al. 10.1007/s11207-016-0911-4
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72. Assessing the Nature of Collisions of Coronal Mass Ejections in the Inner Heliosphere W. Mishra et al. 10.3847/1538-4365/aa8139
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74. Effects of Background Solar Wind and Drag Force on the Propagation of Coronal-mass-ejection-driven Shocks C. Wu et al. 10.3847/1538-4357/ad88ee
75. CME Projection Effects Studied with STEREO/COR and SOHO/LASCO M. Temmer et al. 10.1007/s11207-009-9336-7
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78. Cosmic rays as an indicator of the geoeffectiveness of magnetic clouds A. Petukhova et al. 10.1051/e3sconf/201912702007
79. On the Variation in the Volumetric Evolution of CMEs from the Inner to Outer Corona S. Majumdar et al. 10.3847/1538-4357/ac5909
80. CME dynamics using coronagraph and interplanetary ejecta data A. Dal Lago et al. 10.1016/j.asr.2012.11.023
81. Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model B. Vršnak et al. 10.1007/s11207-012-0035-4
82. Low-Frequency Type-II Radio Detections and Coronagraph Data Employed to Describe and Forecast the Propagation of 71 CMEs/Shocks H. Cremades et al. 10.1007/s11207-015-0776-y
83. Some properties of the development of the perturbed zone and shock preceding a coronal mass ejection M. Eselevich & V. Eselevich 10.1134/S1063772911110023
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85. Influence of Convection Effects of Solar Wind Speed on CME Transit Time L. SUN 10.11728/cjss2016.06.828
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87. The Origin, Early Evolution and Predictability of Solar Eruptions L. Green et al. 10.1007/s11214-017-0462-5
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89. Why are halo coronal mass ejections faster? Q. Zhang et al. 10.1088/1674-4527/10/5/006
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93. On Earth’s habitability over the Sun’s main-sequence history: joint influence of space weather and Earth’s magnetic field evolution J. Varela et al. 10.1093/mnras/stad2519
94. Plasma Diagnostics of Coronal Dimming Events K. Vanninathan et al. 10.3847/1538-4357/aab09a
95. Magnetic complexity in eruptive solar active regions and associated eruption parameters M. Georgoulis 10.1029/2007GL032040
96. UV and Radio Observations of the Coronal Shock Associated with the 2002 July 23 Coronal Mass Ejection Event S. Mancuso & D. Avetta 10.1086/528839
97. A Coronal Mass Ejection Impacting Parker Solar Probe at 14 Solar Radii C. Braga et al. 10.3847/1538-4357/ad2b4e
98. Numerical Heliospheric Simulations as Assisting Tool for Interpretation of Observations by STEREO Heliospheric Imagers D. Odstrcil & V. Pizzo 10.1007/s11207-009-9449-z
99. Solar and interplanetary precursors of geomagnetic storms in solar cycle 23 J. Uwamahoro & L. McKinnell 10.1016/j.asr.2012.09.034
100. Heliospheric tracking of enhanced density structures of the 6 October 2010 CME W. Mishra & N. Srivastava 10.1051/swsc/2015021
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103. Magnetic Structure and Propagation of Two Interacting CMEs From the Sun to Saturn E. Palmerio et al. 10.1029/2021JA029770
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106. Relationships between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Declining Phase of Solar Cycles 23 and 24 M. Lawrance et al. 10.1007/s11207-020-01623-1
107. Sun to 1 AU propagation and evolution of a slow streamer‐blowout coronal mass ejection B. Lynch et al. 10.1029/2009JA015099
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109. The 04 – 10 September 2017 Sun–Earth Connection Events: Solar Flares, Coronal Mass Ejections/Magnetic Clouds, and Geomagnetic Storms C. Wu et al. 10.1007/s11207-019-1446-2
110. On the Fast Propagating Ultra-hot Disturbance Captured by SDO/AIA: An In-depth Insight into the Coronal Nonlinear Dynamics H. Li et al. 10.3847/2041-8213/aba128
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117. Speeds and Arrival Times of Solar Transients Approximated by Self-similar Expanding Circular Fronts C. Möstl & J. Davies 10.1007/s11207-012-9978-8
118. Evolution of a Long‐Duration Coronal Mass Ejection and Its Sheath Region Between Mercury and Earth on 9–14 July 2013 N. Lugaz et al. 10.1029/2019JA027213
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128. The Formation of Large-Scale Current Sheets within Magnetic Clouds M. Owens 10.1007/s11207-009-9442-6
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131. Influence of Convective Effect of Solar Winds on the CME Transit Time S. Lu-yuan 10.1016/j.chinastron.2017.11.004
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153. Interplanetary Coronal Mass Ejections Observed by Ulysses Through Its Three Solar Orbits D. Du et al. 10.1007/s11207-009-9505-8
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158. Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections P. Démoulin et al. 10.1007/s11207-008-9221-9
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