309 citations as recorded by crossref.

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3. Studying the properties of interplanetary counterpart of halo-CMEs and their influences on Dst index A. Goswami https://doi.org/10.1016/j.asr.2019.03.015
4. Predicting the Geoeffectiveness of CMEs Using Machine Learning A. Pricopi et al. https://doi.org/10.3847/1538-4357/ac7962
5. A New Tool for CME Arrival Time Prediction using Machine Learning Algorithms: CAT-PUMA J. Liu et al. https://doi.org/10.3847/1538-4357/aaae69
6. CME Propagation Characteristics from Radio Observations S. Pohjolainen et al. https://doi.org/10.1007/s11207-007-9006-6
7. Is the Asymmetric Cone Model for Halo Coronal Mass Ejections Correct? G. Michalek https://doi.org/10.1007/s11207-009-9472-0
8. Theory of the Formation of Forbush Decrease in a Magnetic Cloud: Dependence of Forbush Decrease Characteristics on Magnetic Cloud Parameters A. Petukhova et al. https://doi.org/10.3847/1538-4357/ab2889
9. A New Prediction Method for the Arrival Time of Interplanetary Shocks X. Feng & X. Zhao https://doi.org/10.1007/s11207-006-0185-3
10. Coronal Mass Ejection Arrival Forecasting with the Drag-based Assimilation of Satellite Observations Z. Abu-Shaar et al. https://doi.org/10.3847/1538-4365/ae0d8a
11. ElEvoHI: A NOVEL CME PREDICTION TOOL FOR HELIOSPHERIC IMAGING COMBINING AN ELLIPTICAL FRONT WITH DRAG-BASED MODEL FITTING T. Rollett et al. https://doi.org/10.3847/0004-637X/824/2/131
12. 4π Models of CMEs and ICMEs (Invited Review) J. Kleimann https://doi.org/10.1007/s11207-012-9994-8
13. Coronal dimmings as indicators of the direction of early coronal mass ejection propagation S. Jain et al. https://doi.org/10.1051/0004-6361/202347927
14. Statistical Study of Intense Geomagnetic Storms and Their Solar Origins over the Period 1996 – 2025 A. Augustine D’Awarave & V. Panditi https://doi.org/10.1007/s11207-026-02666-6
15. Estimating the lateral speed of a fast shock driven by a coronal mass ejection at the location of solar radio emissions S. Normo et al. https://doi.org/10.1051/0004-6361/202449277
16. A probabilistic approach to the drag-based model G. Napoletano et al. https://doi.org/10.1051/swsc/2018003
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18. From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection M. Bisi et al. https://doi.org/10.1007/s11207-010-9602-8
19. Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005 J. Zhang et al. https://doi.org/10.1029/2007JA012321
20. Statistical Analysis of Solar Events Associated with Storm Sudden Commencements over One Year of Solar Maximum During Cycle 23: Propagation from the Sun to the Earth and Effects K. Bocchialini et al. https://doi.org/10.1007/s11207-018-1278-5
21. On the Expansion Speed of Coronal Mass Ejections: Implications for Self-Similar Evolution L. Balmaceda et al. https://doi.org/10.1007/s11207-020-01672-6
22. Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test A. Bemporad et al. https://doi.org/10.1051/0004-6361/201833058
23. Analysis and study of the in situ observation of the June 1st 2008 CME by STEREO T. Nieves-Chinchilla et al. https://doi.org/10.1016/j.jastp.2010.09.026
24. VARIATIONS OF THE MUON FLUX AT SEA LEVEL ASSOCIATED WITH INTERPLANETARY ICMEs AND COROTATING INTERACTION REGIONS C. Augusto et al. https://doi.org/10.1088/0004-637X/759/2/143
25. Comparison of geoeffectiveness of coronal mass ejections and corotating interaction regions G. Verbanac et al. https://doi.org/10.1051/0004-6361/201220417
26. Empirical modeling of the storm time geomagnetic indices: a comparison between the local K and global Kp indices J. Uwamahoro & J. Habarulema https://doi.org/10.1186/1880-5981-66-95
27. Causes responsible for intense and severe storms during the declining phase of Solar Cycle 24 K. Patel et al. https://doi.org/10.1007/s12036-018-9569-7
28. Expansion Speed of Coronal Mass Ejections G. Michalek et al. https://doi.org/10.1007/s11207-009-9464-0
29. Interplanetary coronal mass ejections that are undetected by solar coronagraphs T. Howard & G. Simnett https://doi.org/10.1029/2007JA012920
30. Numeric and analytic study of interplanetary coronal mass ejection and shock evolution: Driving, decoupling, and decaying P. Corona-Romero & J. Gonzalez-Esparza https://doi.org/10.1029/2010JA016008
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33. Commission 10: Solar Activity D. Melrose et al. https://doi.org/10.1017/S1743921306004388
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35. Determining CME parameters by fitting heliospheric observations: Numerical investigation of the accuracy of the methods N. Lugaz et al. https://doi.org/10.1016/j.asr.2011.03.015
36. CME Arrival Time Prediction via Fusion of Physical Parameters and Image Features Y. Zhong et al. https://doi.org/10.3847/1538-4365/ad1f5d
37. Quasi-planar ICME sheath: A cause of the first two-step extreme geomagnetic storm of the 25th solar cycle observed on 23 April 2023 K. Ghag et al. https://doi.org/10.1016/j.asr.2024.03.011
38. Magnetic Flux Emergence, Activity, Eruptions and Magnetic Clouds: Following Magnetic Field from the Sun to the Heliosphere L. van Driel-Gesztelyi & J. Culhane https://doi.org/10.1007/s11214-008-9461-x
39. Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure V. Parkhomov et al. https://doi.org/10.12737/szf-73202102
40. Coronal Mass Ejection Transit Time Prediction Based on Spatiotemporal Modeling Using 3D Convolutional Neural Networks W. Zhou et al. https://doi.org/10.3847/1538-4357/ae3c79
41. East‐west asymmetry in coronal mass ejection geoeffectiveness G. Siscoe et al. https://doi.org/10.1029/2006SW000286
42. Formation of Coronal Mass Ejections in the Solar Corona and Propagation of the Resulting Plasma Streams in the Heliosphere V. Slemzin et al. https://doi.org/10.1134/S1063780X19100076
43. Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection R. Márquez Rodríguez et al. https://doi.org/10.1007/s11207-023-02146-1
44. Distribution and recovery phase of geomagnetic storms during solar cycles 23 and 24 W. Mishra et al. https://doi.org/10.1093/mnras/stae1045
45. Investigations of the sensitivity of a coronal mass ejection model (ENLIL) to solar input parameters T. Falkenberg et al. https://doi.org/10.1029/2009SW000555
46. Solar energetic particles propagation during solar events at the beginning of the 25th solar cycle T. Khumlumlert et al. https://doi.org/10.1088/1742-6596/2653/1/012021
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48. Relationship between the geomagnetic Dst(min) and the interplanetary Bz(min) during cycle 23 R. Kane https://doi.org/10.1016/j.pss.2009.11.005
49. Expansion-induced Three-part Morphology of the 2021 December 4 Coronal Mass Ejection L. Yang et al. https://doi.org/10.3847/1538-4357/adb313
50. Forecasting the Structure and Orientation of Earthbound Coronal Mass Ejections E. Kilpua et al. https://doi.org/10.1029/2018SW001944
51. Interplanetary Magnetic Flux Rope Observed at Ground Level by HAWC S. Akiyama et al. https://doi.org/10.3847/1538-4357/abc344
52. Near-Earth Interplanetary Coronal Mass Ejections and Their Association with DH Type II Radio Bursts During Solar Cycles 23 and 24 B. Patel et al. https://doi.org/10.1007/s11207-022-02073-7
53. Forbush decreases and turbulence levels at coronal mass ejection fronts P. Subramanian et al. https://doi.org/10.1051/0004-6361:200809551
54. The role of aerodynamic drag in propagation of interplanetary coronal mass ejections B. Vršnak et al. https://doi.org/10.1051/0004-6361/200913482
55. Correcting Projection Effects in CMEs Using GCS‐Based Large Statistics of Multi‐Viewpoint Observations H. Gandhi et al. https://doi.org/10.1029/2023SW003805
56. Predicting Arrival Times of the CCMC CME/Shock Events Based on the SPM3 Model Y. Liang 梁 et al. https://doi.org/10.3847/1538-4357/ad84f0
57. 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. https://doi.org/10.1051/swsc/2016038
58. Effects of ICMEs on High Energetic Particles as Observed by the Global Muon Detector Network (GMDN) A. Dal Lago et al. https://doi.org/10.1017/S1743921318000066
59. CME Disturbance Forecasting G. Siscoe & R. Schwenn https://doi.org/10.1007/s11214-006-9024-y
60. Impacts of CMEs on Earth Based on Logistic Regression and Recommendation Algorithm Y. Shi et al. https://doi.org/10.34133/2022/9852185
61. Source region of the 18 November 2003 coronal mass ejection that led to the strongest magnetic storm of cycle 23 N. Srivastava et al. https://doi.org/10.1029/2008JA013845
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63. A Statistical Study of Solar Filament Eruptions that Form High-speed Coronal Mass Ejections P. Zou et al. https://doi.org/10.3847/1538-4357/ab4355
64. Estimation of Transit Time of CMEs from the Sun to Earth A. Pattnaik et al. https://doi.org/10.3847/1538-4357/adb84b
65. Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure V. Parhomov et al. https://doi.org/10.12737/stp-73202102
66. CORONAL MASS EJECTION DYNAMICS REGARDING RADIAL AND EXPANSION SPEEDS N. Rigozo et al. https://doi.org/10.1088/0004-637X/738/1/107
67. 3D Reconstruction of the Leading Edge of the 20 May 2007 Partial Halo CME N. Srivastava et al. https://doi.org/10.1007/s11207-009-9423-9
68. The Effect of the Heliospheric Current Sheet on Interplanetary Shocks Y. Xie et al. https://doi.org/10.1007/s11207-006-0227-x
69. Transit time of CME/shock associated with four major geo-effective CMEs in solar cycle 24 M. Syed Ibrahim et al. https://doi.org/10.1016/j.asr.2014.09.031
70. A kinematically distorted flux rope model for magnetic clouds M. Owens et al. https://doi.org/10.1029/2005JA011460
71. Investigation of geo-effective properties of halo coronal mass ejections S. Bhardwaj et al. https://doi.org/10.2205/2018ES000620
72. Estimating the geoeffectiveness of halo CMEs from associated solar and IP parameters using neural networks J. Uwamahoro et al. https://doi.org/10.5194/angeo-30-963-2012
73. Relationships Between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Rising Phase of Solar Cycles 23 and 24 M. Lawrance et al. https://doi.org/10.1007/s11207-016-0911-4
74. Statistical geoeffectiveness of solar-interplanetary disturbance events of type II radio bursts and CMEs/shocks J. Yan & Q. Yu https://doi.org/10.3389/fspas.2024.1452513
75. Pursuing Forecasts of the Behavior and Arrival of Coronal Mass Ejections through Modeling and Observations H. Cremades https://doi.org/10.1017/S1743921317010882
76. Assessing the Nature of Collisions of Coronal Mass Ejections in the Inner Heliosphere W. Mishra et al. https://doi.org/10.3847/1538-4365/aa8139
77. Multipoint Study of Successive Coronal Mass Ejections Driving Moderate Disturbances at 1 au E. Palmerio et al. https://doi.org/10.3847/1538-4357/ab1850
78. Effects of Background Solar Wind and Drag Force on the Propagation of Coronal-mass-ejection-driven Shocks C. Wu et al. https://doi.org/10.3847/1538-4357/ad88ee
79. CME Projection Effects Studied with STEREO/COR and SOHO/LASCO M. Temmer et al. https://doi.org/10.1007/s11207-009-9336-7
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83. On the Variation in the Volumetric Evolution of CMEs from the Inner to Outer Corona S. Majumdar et al. https://doi.org/10.3847/1538-4357/ac5909
84. CME dynamics using coronagraph and interplanetary ejecta data A. Dal Lago et al. https://doi.org/10.1016/j.asr.2012.11.023
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86. Low-Frequency Type-II Radio Detections and Coronagraph Data Employed to Describe and Forecast the Propagation of 71 CMEs/Shocks H. Cremades et al. https://doi.org/10.1007/s11207-015-0776-y
87. Some properties of the development of the perturbed zone and shock preceding a coronal mass ejection M. Eselevich & V. Eselevich https://doi.org/10.1134/S1063772911110023
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104. Numerical Heliospheric Simulations as Assisting Tool for Interpretation of Observations by STEREO Heliospheric Imagers D. Odstrcil & V. Pizzo https://doi.org/10.1007/s11207-009-9449-z
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106. Heliospheric tracking of enhanced density structures of the 6 October 2010 CME W. Mishra & N. Srivastava https://doi.org/10.1051/swsc/2015021
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116. On the Fast Propagating Ultra-hot Disturbance Captured by SDO/AIA: An In-depth Insight into the Coronal Nonlinear Dynamics H. Li et al. https://doi.org/10.3847/2041-8213/aba128
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118. Prediction of the Transit Time of Coronal Mass Ejections with an Ensemble Machine-learning Method Y. Yang et al. https://doi.org/10.3847/1538-4365/acf218
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123. Speeds and Arrival Times of Solar Transients Approximated by Self-similar Expanding Circular Fronts C. Möstl & J. Davies https://doi.org/10.1007/s11207-012-9978-8
124. 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. https://doi.org/10.1029/2019JA027213
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136. Using soft X‐ray observations to help the prediction of flare related interplanetary shocks arrival times at the Earth H. Liu & G. Qin https://doi.org/10.1029/2011JA017220
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149. A COMPARISON OF RECONSTRUCTION METHODS FOR THE ESTIMATION OF CORONAL MASS EJECTIONS KINEMATICS BASED ON SECCHI/HI OBSERVATIONS W. Mishra et al. https://doi.org/10.1088/0004-637X/784/2/135
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