277 citations as recorded by crossref.

1. Coronal Mass Ejections from the Same Active Region Cluster: Two Different Perspectives H. Cremades et al. 10.1007/s11207-015-0717-9
2. Empirical model of the transit time of interplanetary coronal mass ejections A. Mahrous et al. 10.1134/S0038094609020051
3. Studying the properties of interplanetary counterpart of halo-CMEs and their influences on Dst index A. Goswami 10.1016/j.asr.2019.03.015
4. Predicting the Geoeffectiveness of CMEs Using Machine Learning A. Pricopi et al. 10.3847/1538-4357/ac7962
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
7. Is the Asymmetric Cone Model for Halo Coronal Mass Ejections Correct? G. Michalek 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. 10.3847/1538-4357/ab2889
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
12. Coronal dimmings as indicators of the direction of early coronal mass ejection propagation S. Jain et al. 10.1051/0004-6361/202347927
13. A probabilistic approach to the drag-based model G. Napoletano et al. 10.1051/swsc/2018003
14. Probabilistic hazard assessment: Application to geomagnetic activity G. Richardson & A. Thomson 10.1051/swsc/2022001
15. From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection M. Bisi et al. 10.1007/s11207-010-9602-8
16. Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005 J. Zhang et al. 10.1029/2007JA012321
17. 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. 10.1007/s11207-018-1278-5
18. On the Expansion Speed of Coronal Mass Ejections: Implications for Self-Similar Evolution L. Balmaceda et al. 10.1007/s11207-020-01672-6
19. Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test A. Bemporad et al. 10.1051/0004-6361/201833058
20. 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
21. VARIATIONS OF THE MUON FLUX AT SEA LEVEL ASSOCIATED WITH INTERPLANETARY ICMEs AND COROTATING INTERACTION REGIONS C. Augusto et al. 10.1088/0004-637X/759/2/143
22. Comparison of geoeffectiveness of coronal mass ejections and corotating interaction regions G. Verbanac et al. 10.1051/0004-6361/201220417
23. Empirical modeling of the storm time geomagnetic indices: a comparison between the local K and global Kp indices J. Uwamahoro & J. Habarulema 10.1186/1880-5981-66-95
24. Causes responsible for intense and severe storms during the declining phase of Solar Cycle 24 K. Patel et al. 10.1007/s12036-018-9569-7
25. Expansion Speed of Coronal Mass Ejections G. Michalek et al. 10.1007/s11207-009-9464-0
26. Interplanetary coronal mass ejections that are undetected by solar coronagraphs T. Howard & G. Simnett 10.1029/2007JA012920
27. Numeric and analytic study of interplanetary coronal mass ejection and shock evolution: Driving, decoupling, and decaying P. Corona-Romero & J. Gonzalez-Esparza 10.1029/2010JA016008
28. Predicting the Time of Arrival of Coronal Mass Ejections at Earth From Heliospheric Imaging Observations C. Braga et al. 10.1029/2020JA027885
29. Correspondence of a global isolated substorm to the McPherron statistical model V. Parhomov et al. 10.12737/stp-82202206
30. Commission 10: Solar Activity D. Melrose et al. 10.1017/S1743921306004388
31. 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
32. 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
33. CME Arrival Time Prediction via Fusion of Physical Parameters and Image Features Y. Zhong et al. 10.3847/1538-4365/ad1f5d
34. 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. 10.1016/j.asr.2024.03.011
35. 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
36. Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure V. Parkhomov et al. 10.12737/szf-73202102
37. East‐west asymmetry in coronal mass ejection geoeffectiveness G. Siscoe et al. 10.1029/2006SW000286
38. Formation of Coronal Mass Ejections in the Solar Corona and Propagation of the Resulting Plasma Streams in the Heliosphere V. Slemzin et al. 10.1134/S1063780X19100076
39. Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection R. Márquez Rodríguez et al. 10.1007/s11207-023-02146-1
40. Investigations of the sensitivity of a coronal mass ejection model (ENLIL) to solar input parameters T. Falkenberg et al. 10.1029/2009SW000555
41. Solar energetic particles propagation during solar events at the beginning of the 25th solar cycle T. Khumlumlert et al. 10.1088/1742-6596/2653/1/012021
42. Relationship between the geomagnetic Dst(min) and the interplanetary Bz(min) during cycle 23 R. Kane 10.1016/j.pss.2009.11.005
43. Forecasting the Structure and Orientation of Earthbound Coronal Mass Ejections E. Kilpua et al. 10.1029/2018SW001944
44. Interplanetary Magnetic Flux Rope Observed at Ground Level by HAWC S. Akiyama et al. 10.3847/1538-4357/abc344
45. 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. 10.1007/s11207-022-02073-7
46. Forbush decreases and turbulence levels at coronal mass ejection fronts P. Subramanian et al. 10.1051/0004-6361:200809551
47. The role of aerodynamic drag in propagation of interplanetary coronal mass ejections B. Vršnak et al. 10.1051/0004-6361/200913482
48. Correcting Projection Effects in CMEs Using GCS‐Based Large Statistics of Multi‐Viewpoint Observations H. Gandhi et al. 10.1029/2023SW003805
49. 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
50. Effects of ICMEs on High Energetic Particles as Observed by the Global Muon Detector Network (GMDN) A. Dal Lago et al. 10.1017/S1743921318000066
51. CME Disturbance Forecasting G. Siscoe & R. Schwenn 10.1007/s11214-006-9024-y
52. Impacts of CMEs on Earth Based on Logistic Regression and Recommendation Algorithm Y. Shi et al. 10.34133/2022/9852185
53. 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
54. 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
55. A Statistical Study of Solar Filament Eruptions that Form High-speed Coronal Mass Ejections P. Zou et al. 10.3847/1538-4357/ab4355
56. Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure V. Parhomov et al. 10.12737/stp-73202102
57. CORONAL MASS EJECTION DYNAMICS REGARDING RADIAL AND EXPANSION SPEEDS N. Rigozo et al. 10.1088/0004-637X/738/1/107
58. 3D Reconstruction of the Leading Edge of the 20 May 2007 Partial Halo CME N. Srivastava et al. 10.1007/s11207-009-9423-9
59. The Effect of the Heliospheric Current Sheet on Interplanetary Shocks Y. Xie et al. 10.1007/s11207-006-0227-x
60. Transit time of CME/shock associated with four major geo-effective CMEs in solar cycle 24 M. Syed Ibrahim et al. 10.1016/j.asr.2014.09.031
61. A kinematically distorted flux rope model for magnetic clouds M. Owens et al. 10.1029/2005JA011460
62. Investigation of geo-effective properties of halo coronal mass ejections S. Bhardwaj et al. 10.2205/2018ES000620
63. Estimating the geoeffectiveness of halo CMEs from associated solar and IP parameters using neural networks J. Uwamahoro et al. 10.5194/angeo-30-963-2012
64. 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
65. Pursuing Forecasts of the Behavior and Arrival of Coronal Mass Ejections through Modeling and Observations H. Cremades 10.1017/S1743921317010882
66. Assessing the Nature of Collisions of Coronal Mass Ejections in the Inner Heliosphere W. Mishra et al. 10.3847/1538-4365/aa8139
67. Multipoint Study of Successive Coronal Mass Ejections Driving Moderate Disturbances at 1 au E. Palmerio et al. 10.3847/1538-4357/ab1850
68. CME Projection Effects Studied with STEREO/COR and SOHO/LASCO M. Temmer et al. 10.1007/s11207-009-9336-7
69. Prediction of the shock arrival time with SEP observations G. Qin et al. 10.1029/2009JA014332
70. Coronal mass ejections and their sheath regions in interplanetary space E. Kilpua et al. 10.1007/s41116-017-0009-6
71. Cosmic rays as an indicator of the geoeffectiveness of magnetic clouds A. Petukhova et al. 10.1051/e3sconf/201912702007
72. On the Variation in the Volumetric Evolution of CMEs from the Inner to Outer Corona S. Majumdar et al. 10.3847/1538-4357/ac5909
73. CME dynamics using coronagraph and interplanetary ejecta data A. Dal Lago et al. 10.1016/j.asr.2012.11.023
74. Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model B. Vršnak et al. 10.1007/s11207-012-0035-4
75. 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
76. Some properties of the development of the perturbed zone and shock preceding a coronal mass ejection M. Eselevich & V. Eselevich 10.1134/S1063772911110023
77. Investigating plasma motion of magnetic clouds at 1 AU through a velocity‐modified cylindrical force‐free flux rope model Y. Wang et al. 10.1002/2014JA020494
78. Influence of Convection Effects of Solar Wind Speed on CME Transit Time L. SUN 10.11728/cjss2016.06.828
79. Arrival time of solar eruptive CMEs associated with ICMEs of magnetic cloud and ejecta A. Shanmugaraju et al. 10.1007/s10509-015-2251-5
80. The Origin, Early Evolution and Predictability of Solar Eruptions L. Green et al. 10.1007/s11214-017-0462-5
81. Multifractal analysis of geomagnetic storm and solar flare indices and their class dependence Z. Yu et al. 10.1029/2008JA013854
82. Why are halo coronal mass ejections faster? Q. Zhang et al. 10.1088/1674-4527/10/5/006
83. The 17–22 October (1999) solar‐interplanetary‐geomagnetic event: Very intense geomagnetic storm associated with a pressure balance between interplanetary coronal mass ejection and a high‐speed stream A. Dal Lago et al. 10.1029/2005JA011394
84. Catalog of large-scale solar wind phenomena during 1976–2000 Y. Yermolaev et al. 10.1134/S0010952509020014
85. Geomagnetic storm's precursors observed from 2001 to 2007 with the Global Muon Detector Network (GMDN) M. Rockenbach et al. 10.1029/2011GL048556
86. 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
87. Plasma Diagnostics of Coronal Dimming Events K. Vanninathan et al. 10.3847/1538-4357/aab09a
88. Magnetic complexity in eruptive solar active regions and associated eruption parameters M. Georgoulis 10.1029/2007GL032040
89. 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
90. Numerical Heliospheric Simulations as Assisting Tool for Interpretation of Observations by STEREO Heliospheric Imagers D. Odstrcil & V. Pizzo 10.1007/s11207-009-9449-z
91. Solar and interplanetary precursors of geomagnetic storms in solar cycle 23 J. Uwamahoro & L. McKinnell 10.1016/j.asr.2012.09.034
92. Heliospheric tracking of enhanced density structures of the 6 October 2010 CME W. Mishra & N. Srivastava 10.1051/swsc/2015021
93. First Simultaneous Views of the Axial and Lateral Perspectives of a Coronal Mass Ejection I. Cabello et al. 10.1007/s11207-016-0941-y
94. Sun-to-earth propagation of the 2015 June 21 coronal mass ejection revealed by optical, EUV, and radio observations N. Gopalswamy et al. 10.1016/j.jastp.2018.07.013
95. Magnetic Structure and Propagation of Two Interacting CMEs From the Sun to Saturn E. Palmerio et al. 10.1029/2021JA029770
96. On the possible reason for the formation of impulsive coronal mass ejections D. Romanov et al. 10.1016/j.asr.2014.09.017
97. Interplanetary shocks unconnected with earthbound coronal mass ejections T. Howard & S. Tappin 10.1029/2005GL023056
98. 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
99. Sun to 1 AU propagation and evolution of a slow streamer‐blowout coronal mass ejection B. Lynch et al. 10.1029/2009JA015099
100. Arrival Time Estimates of Earth-Directed CME-Driven Shocks K. Suresh et al. 10.1007/s11207-021-01914-1
101. 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
102. 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
103. On the Evolution of Coronal Mass Ejections in the Interplanetary Medium T. Howard et al. 10.1086/519758
104. Prediction of the Transit Time of Coronal Mass Ejections with an Ensemble Machine-learning Method Y. Yang et al. 10.3847/1538-4365/acf218
105. Space Weather: Physics, Effects and Predictability A. Singh et al. 10.1007/s10712-010-9103-1
106. Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun–Earth connection M. Pick & N. Vilmer 10.1007/s00159-008-0013-x
107. Predicting the Arrival Time of an Interplanetary Shock Based on DSRT Spectrum Observations for the Corresponding Type II Radio Burst and a Blast Wave Theory R. Li 李 et al. 10.3847/1538-4357/ad150f
108. Speeds and Arrival Times of Solar Transients Approximated by Self-similar Expanding Circular Fronts C. Möstl & J. Davies 10.1007/s11207-012-9978-8
109. 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
110. Study of simultaneous presence of DD and PP electric fields during the geomagnetic storm of November 7–8, 2004 and resultant TEC variation over the Indian Region P. Galav et al. 10.1007/s10509-014-1792-3
111. PROPAGATION OF THE 2014 JANUARY 7 CME AND RESULTING GEOMAGNETIC NON-EVENT M. Mays et al. 10.1088/0004-637X/812/2/145
112. High-rigidity Forbush decreases: due to CMEs or shocks? K. Arunbabu et al. 10.1051/0004-6361/201220830
113. Geoeffective Analysis of CMEs Under Current Sheet Magnetic Coordinates X. Feng & X. Zhao 10.1007/s10509-006-9039-6
114. Propagation of an Earth-directed coronal mass ejection in three dimensions J. Byrne et al. 10.1038/ncomms1077
115. A geometrical description for interplanetary propagation of Earth-directed CMEs based on radiative proxies C. Salas-Matamoros & J. Sanchez-Guevara 10.1093/mnras/stab1232
116. Combining remote and in situ observations of coronal mass ejections to better constrain magnetic cloud reconstruction M. Owens 10.1029/2008JA013589
117. Predicting CME arrival time through data integration and ensemble learning K. Alobaid et al. 10.3389/fspas.2022.1013345
118. The Formation of Large-Scale Current Sheets within Magnetic Clouds M. Owens 10.1007/s11207-009-9442-6
119. Using soft X‐ray observations to help the prediction of flare related interplanetary shocks arrival times at the Earth H. Liu & G. Qin 10.1029/2011JA017220
120. EIT wave observations and modeling in the STEREO era A. Zhukov 10.1016/j.jastp.2010.11.030
121. Influence of Convective Effect of Solar Winds on the CME Transit Time S. Lu-yuan 10.1016/j.chinastron.2017.11.004
122. Halo coronal mass ejections during Solar Cycle 24: reconstruction of the global scenario and geoeffectiveness C. Scolini et al. 10.1051/swsc/2017046
123. On the Collision Nature of Two Coronal Mass Ejections: A Review F. Shen et al. 10.1007/s11207-017-1129-9
124. NEAR-SIMULTANEOUS OBSERVATIONS OF X-RAY PLASMA EJECTION, CORONAL MASS EJECTION, AND TYPE II RADIO BURST Y. Kim et al. 10.1088/0004-637X/705/2/1721
125. Improved methods for determining the kinematics of coronal mass ejections and coronal waves J. Byrne et al. 10.1051/0004-6361/201321223
126. Properties and drivers of fast interplanetary shocks near the orbit of the Earth (1995–2013) E. Kilpua et al. 10.1002/2015JA021138
127. Extraction of Halo Coronal Mass Ejection Asymmetry Information from LASCO Coronagraph Images A. Ling & D. Webb 10.1086/518956
128. Investigating Remote-Sensing Techniques to Reveal Stealth Coronal Mass Ejections E. Palmerio et al. 10.3389/fspas.2021.695966
129. Improved input to the empirical coronal mass ejection (CME) driven shock arrival model from CME cone models H. Xie et al. 10.1029/2006SW000227
130. Genesis and Impulsive Evolution of the 2017 September 10 Coronal Mass Ejection A. Veronig et al. 10.3847/1538-4357/aaeac5
131. Potential role of energetic particle observations in geomagnetic storm forecasting D. Ameri & E. Valtonen 10.1016/j.asr.2019.05.012
132. A COMPARISON OF RECONSTRUCTION METHODS FOR THE ESTIMATION OF CORONAL MASS EJECTIONS KINEMATICS BASED ON SECCHI/HI OBSERVATIONS W. Mishra et al. 10.1088/0004-637X/784/2/135
133. Estimating Travel Times of Coronal Mass Ejections to 1 AU Using Multi-spacecraft Coronagraph Data E. Kilpua et al. 10.1007/s11207-012-0005-x
134. Space Weather Monitor at the L5 Point: A Case Study of a CME Observed with STEREO B L. Rodriguez et al. 10.1029/2020SW002533
135. COMPREHENSIVE OBSERVATIONS OF A SOLAR MINIMUM CORONAL MASS EJECTION WITH THESOLAR TERRESTRIAL RELATIONS OBSERVATORY B. Wood et al. 10.1088/0004-637X/694/2/707
136. ESTIMATING THE ARRIVAL TIME OF EARTH-DIRECTED CORONAL MASS EJECTIONS AT IN SITU SPACECRAFT USING COR AND HI OBSERVATIONS FROMSTEREO W. Mishra & N. Srivastava 10.1088/0004-637X/772/1/70
137. Exploring the radial evolution of interplanetary coronal mass ejections using EUHFORIA C. Scolini et al. 10.1051/0004-6361/202040226
138. Three frontside full halo coronal mass ejections with a nontypical geomagnetic response L. Rodriguez et al. 10.1029/2008SW000453
139. Geoeffective Properties of Solar Transients and Stream Interaction Regions E. Kilpua et al. 10.1007/s11214-017-0411-3
140. Clustering of Fast Coronal Mass Ejections during Solar Cycles 23 and 24 and the Implications for CME–CME Interactions J. Rodríguez Gómez et al. 10.3847/1538-4357/ab9e72
141. Predicting the geoeffective properties of coronal mass ejections: current status, open issues and path forward A. Vourlidas et al. 10.1098/rsta.2018.0096
142. Interplanetary Coronal Mass Ejections Observed by Ulysses Through Its Three Solar Orbits D. Du et al. 10.1007/s11207-009-9505-8
143. Type II solar radio bursts: 2. Detailed comparison of theory with observations D. Hillan et al. 10.1029/2011JA016755
144. Resolving the Ambiguity of a Magnetic Cloud’s Orientation Caused by Minimum Variance Analysis Comparing it with a Force-Free Model R. Rosa Oliveira et al. 10.1007/s11207-021-01921-2
145. Propagation characteristics of coronal mass ejections (CMEs) in the corona and interplanetary space F. Shen et al. 10.1007/s41614-022-00069-1
146. Impact of the Solar Activity on the Propagation of ICMEs: Simulations of Hydro, Magnetic and Median ICMEs at the Minimum and Maximum of Activity B. Perri et al. 10.3847/1538-4357/acec6f
147. Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections P. Démoulin et al. 10.1007/s11207-008-9221-9
148. Geomagnetic Effects of Corotating Interaction Regions B. Vršnak et al. 10.1007/s11207-017-1165-5
149. HELIOSPHERIC PROPAGATION OF CORONAL MASS EJECTIONS: COMPARISON OF NUMERICAL WSA-ENLIL+CONE MODEL AND ANALYTICAL DRAG-BASED MODEL B. Vršnak et al. 10.1088/0067-0049/213/2/21
150. Dependence of Coronal Mass Ejection Properties on Their Solar Source Active Region Characteristics and Associated Flare Reconnection Flux S. Pal et al. 10.3847/1538-4357/aada10
151. Deflected propagation of a coronal mass ejection from the corona to interplanetary space Y. Wang et al. 10.1002/2013JA019537
152. Over-expansion of coronal mass ejections modelled using 3D MHD EUHFORIA simulations C. Verbeke et al. 10.1016/j.asr.2022.06.013
153. Underlying scaling relationships between solar activity and geomagnetic activity revealed by multifractal analyses Z. Yu et al. 10.1002/2014JA019893
154. Investigating the kinematics of coronal mass ejections with the automated CORIMP catalog J. Byrne 10.1051/swsc/2015020
155. Solar wind diamagnetic structures as a source of substorm-like disturbances V. Parkhomov et al. 10.1016/j.jastp.2018.10.010
156. Probabilistic prediction of geomagnetic storms and theKpindex S. Chakraborty & S. Morley 10.1051/swsc/2020037
157. Comment on “Geoeffectiveness of Halo Coronal Mass Ejections” by N. Gopalswamy, S. Yashiro, and S. Akiyama (J. Geophys. Res. 2007, 112, doi:10.1029/2006JA012149) Y. Yermolaev 10.1134/S0010952508060099
158. HELIOSPHERIC PROPAGATION OF CORONAL MASS EJECTIONS: DRAG-BASED MODEL FITTING T. Žic et al. 10.1088/0067-0049/218/2/32
159. Predicting the CME arrival time based on the recommendation algorithm Y. Shi et al. 10.1088/1674-4527/21/8/190
160. Near real‐time predictions of the arrival at Earth of flare‐related shocks during Solar Cycle 23 S. McKenna‐Lawlor et al. 10.1029/2005JA011162
161. Investigation of the Geoeffectiveness of CMEs Associated with IP Type II Radio Bursts V. Vasanth et al. 10.1007/s11207-015-0713-0
162. Transit times of interplanetary coronal mass ejections and the solar wind speed B. Vršnak & T. Žic 10.1051/0004-6361:20077499
163. Correspondence of a global isolated substorm to the McPherron statistical model V. Parhomov et al. 10.12737/szf-82202206
164. Image of Forbush Decrease in a Magnetic Cloud by Three Moments of Cosmic Ray Distribution Function A. Petukhova et al. 10.1029/2018JA025964
165. S/WAVES: The Radio and Plasma Wave Investigation on the STEREO Mission J. Bougeret et al. 10.1007/s11214-007-9298-8
166. Solar Weather Event Modelling and Prediction M. Messerotti et al. 10.1007/s11214-009-9574-x
167. The Physical Processes of CME/ICME Evolution W. Manchester et al. 10.1007/s11214-017-0394-0
168. Propagating Conditions and the Time of ICME Arrival: A Comparison of the Effective Acceleration Model with ENLIL and DBEM Models E. Paouris et al. 10.1007/s11207-020-01747-4
169. The radial speed‐expansion speed relation for Earth‐directed CMEs P. Mäkelä et al. 10.1002/2015SW001335
170. Differences in the development of the initial phase of the formation of two types of coronal mass ejections V. Eselevich & M. Eselevich 10.1134/S0010952515010049
171. CME Arrival Time Prediction Using Convolutional Neural Network Y. Wang et al. 10.3847/1538-4357/ab2b3e
172. Ambient solar wind's effect on ICME transit times A. Case et al. 10.1029/2008GL034493
173. An operational solar wind prediction system transitioning fundamental science to operations J. Wang et al. 10.1051/swsc/2018025
174. Coronal Observations of CMEs R. Schwenn et al. 10.1007/s11214-006-9016-y
175. Pseudo-automatic characterization of the morphological and kinematical properties of coronal mass ejections using a texture-based technique C. Braga et al. 10.1016/j.asr.2012.05.009
176. How Does Large Flaring Activity from the Same Active Region Produce Oppositely Directed Magnetic Clouds? L. Harra et al. 10.1007/s11207-007-9002-x
177. Interplanetary Coronal Mass Ejections Resulting from Earth-Directed CMEs Using SOHO and ACE Combined Data During Solar Cycle 23 E. Paouris & H. Mavromichalaki 10.1007/s11207-017-1050-2
178. Features of the Dynamics of a Shock Excited by Fast Coronal Mass Ejections V. Eselevich & M. Eselevich 10.1134/S001095251903002X
179. Understanding the Origins of Problem Geomagnetic Storms Associated with “Stealth” Coronal Mass Ejections N. Nitta et al. 10.1007/s11214-021-00857-0
180. Study of CME transit speeds for the event of 07-NOV-2004 J. Culhane et al. 10.1016/j.asr.2007.01.005
181. Global Energetics of Solar Flares. VI. Refined Energetics of Coronal Mass Ejections M. Aschwanden 10.3847/1538-4357/aa8952
182. Tracking the 3D evolution of a halo coronal mass ejection using the revised cone model Q. Zhang 10.1051/0004-6361/202142942
183. Full‐halo coronal mass ejections: Arrival at the Earth C. Shen et al. 10.1002/2014JA020001
184. On the Statistical Relationship Between CME Speed and Soft X-Ray Flux and Fluence of the Associated Flare C. Salas-Matamoros & K. Klein 10.1007/s11207-015-0677-0
185. A Probabilistic Approach to the Drag-Based Model G. Napoletano et al. 10.1017/S1743921317008122
186. Multipoint remote and in situ observations of interplanetary coronal mass ejection structures during 2011 and associated geomagnetic storms W. Mishra et al. 10.1093/mnras/stab1721
187. An operational method for shock arrival time prediction by one‐dimensional CESE‐HD solar wind model X. Feng et al. 10.1029/2009JA014385
188. ERUPTING FILAMENTS WITH LARGE ENCLOSING FLUX TUBES AS SOURCES OF HIGH-MASS THREE-PART CMEs, AND ERUPTING FILAMENTS IN THE ABSENCE OF ENCLOSING FLUX TUBES AS SOURCES OF LOW-MASS UNSTRUCTURED CMEs J. Hutton & H. Morgan 10.1088/0004-637X/813/1/35
189. Dynamics of coronal mass ejections B. Vršnak et al. 10.1051/0004-6361:200810215
190. Predicting coronal mass ejections transit times to Earth with neural network D. Sudar et al. 10.1093/mnras/stv2782
191. Study of the development of geomagnetic storms in the magnetosphere using solar wind data of three different time resolutions B. Badruddin et al. 10.1007/s10509-021-04030-5
192. Modeling the Thermodynamic Evolution of Coronal Mass Ejections Using Their Kinematics W. Mishra & Y. Wang 10.3847/1538-4357/aadb9b
193. Ensemble Prediction of a Halo Coronal Mass Ejection Using Heliospheric Imagers T. Amerstorfer et al. 10.1029/2017SW001786
194. Impact of Major Coronal Mass Ejections on Geospace during 2005 September 7–13 Y. Wang et al. 10.1086/504676
195. Analysis of Coronal Mass Ejection Flux Rope Signatures Using 3DCORE and Approximate Bayesian Computation A. Weiss et al. 10.3847/1538-4365/abc9bd
196. NO TRACE LEFT BEHIND:STEREOOBSERVATION OF A CORONAL MASS EJECTION WITHOUT LOW CORONAL SIGNATURES E. Robbrecht et al. 10.1088/0004-637X/701/1/283
197. Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 1. Review of Theory T. Howard & S. Tappin 10.1007/s11214-009-9542-5
198. Solar and interplanetary sources of geomagnetic storms: Space weather aspects Y. Yermolaev & M. Yermolaev 10.1134/S0001433810070017
199. Numerical Study of Two Injection Methods for the 2007 November 15 Coronal Mass Ejection in the Inner Heliosphere M. Zhang et al. 10.3847/1538-4357/ac0b3f
200. Automated detection of coronal mass ejections in three-dimensions using multi-viewpoint observations J. Hutton & H. Morgan 10.1051/0004-6361/201629516
201. CME propagation through the heliosphere: Status and future of observations and model development M. Temmer et al. 10.1016/j.asr.2023.07.003
202. A practical database method for predicting arrivals of “average” interplanetary shocks at Earth X. Feng et al. 10.1029/2008JA013499
203. Numerical simulations of ICME–ICME interactions T. Niembro et al. 10.1051/swsc/2018049
204. Influence of Solar Wind Speed and Heliospheric Current Sheet on the CMEs Transit Time T. LUO & Y. XIE 10.11728/cjss2013.04.381
205. Characteristics of X-class flares of solar cycles 23 and 24 in X-ray and EUV bands K. Pandey et al. 10.1016/j.asr.2023.02.022
206. The Sun – Earth Workshop: A Summary of the Outcome J. Culhane & G. Siscoe 10.1007/s11207-007-9037-z
207. Three-dimensional reconstruction of the streamer belt and other large-scale structures of the solar corona F. Saez et al. 10.1051/0004-6361:20066777
208. Magnetohydrodynamic simulation of the interaction between interplanetary strong shock and magnetic cloud and its consequent geoeffectiveness: 2. Oblique collision M. Xiong et al. 10.1029/2006JA011901
209. Studying geoeffective interplanetary coronal mass ejections between the Sun and Earth: Space weather implications of Solar Mass Ejection Imager observations D. Webb et al. 10.1029/2008SW000409
210. Global Nature of Solar Coronal Shock Waves Shown by Inconsistency between EUV Waves and Type II Radio Bursts A. Fulara & R. Kwon 10.3847/2041-8213/ac230d
211. The Significance of the Influence of the CME Deflection in Interplanetary Space on the CME Arrival at Earth B. Zhuang et al. 10.3847/1538-4357/aa7fc0
212. Near-Earth Interplanetary Coronal Mass Ejections During Solar Cycle 23 (1996 – 2009): Catalog and Summary of Properties I. Richardson & H. Cane 10.1007/s11207-010-9568-6
213. Coronal and Interplanetary Propagation of CME/Shocks from Radio, In Situ and White‐Light Observations M. Reiner et al. 10.1086/518683
214. Space weather: the solar perspective M. Temmer 10.1007/s41116-021-00030-3
215. Statistical properties of the most powerful solar and heliospheric disturbances O. Yakovchouk et al. 10.1016/j.asr.2008.09.025
216. Study of the evolution of the geomagnetic disturbances during the passage of high-speed streams from coronal holes in solar cycle 2009-2016 A. Kumar & B. Badruddin 10.1007/s10509-021-03927-5
217. Quantifying the Uncertainty in CME Kinematics Derived From Geometric Modeling of Heliospheric Imager Data L. Barnard et al. 10.1029/2021SW002841
218. Effects of solar flares on ionospheric TEC over Iceland before and during the geomagnetic storm of 8 September 2017 C. Idosa & K. Shogile 10.1063/5.0098971
219. The Flux of Flux Ropes Embedded Within Magnetic Clouds Near 5 AU Y. Zhao et al. 10.1029/2020JA028594
220. Large-scale structure of solar wind and geomagnetic phenomena M. Olyak 10.1016/j.jastp.2012.06.011
221. Statistical study of coronal mass ejection source locations: Understanding CMEs viewed in coronagraphs Y. Wang et al. 10.1029/2010JA016101
222. Bridging EUV and White-Light Observations to Inspect the Initiation Phase of a “Two-Stage” Solar Eruptive Event J. Byrne et al. 10.1007/s11207-014-0585-8
223. Observational Study of an Earth-affecting Problematic ICME from STEREO Y. Chi et al. 10.3847/1538-4357/aacf44
224. Detailed Analysis of Solar Data Related to Historical Extreme Geomagnetic Storms: 1868 – 2010 L. Lefèvre et al. 10.1007/s11207-016-0892-3
225. Parametric study of the kinematic evolution of coronal mass ejection shock waves and their relation to flaring activity M. Jarry et al. 10.1051/0004-6361/202245480
226. On improvement to the Shock Propagation Model (SPM) applied to interplanetary shock transit time forecasting H. Li et al. 10.1029/2008JA013167
227. Statistical Study of ICMEs and Their Sheaths During Solar Cycle 23 (1996 – 2008) E. Mitsakou & X. Moussas 10.1007/s11207-014-0505-y
228. Operational solar flare prediction model using Deep Flare Net N. Nishizuka et al. 10.1186/s40623-021-01381-9
229. Current status of CME/shock arrival time prediction X. Zhao & M. Dryer 10.1002/2014SW001060
230. The first coronal mass ejection observed in both visible-light and UV H I Ly-αchannels of the Metis coronagraph on board Solar Orbiter V. Andretta et al. 10.1051/0004-6361/202142407
231. On the Interplanetary Coronal Mass Ejection Shocks in the Vicinity of the Earth M. Youssef 10.1007/s11038-012-9398-7
232. Properties of Interplanetary Coronal Mass Ejections N. Gopalswamy 10.1007/s11214-006-9102-1
233. Pseudo-automatic Determination of Coronal Mass Ejections’ Kinematics in 3D C. Braga et al. 10.3847/1538-4357/aa755f
234. Statistical Methods Applied to Space Weather Science D. Telloni 10.3389/fspas.2022.865880
235. A Coronal Mass Ejection Source Region Catalog and Their Associated Properties S. Majumdar et al. 10.3847/1538-4365/aceb62
236. The “Same Side – Opposite Side Effect” of the Heliospheric Current Sheet in Ionospheric Negative Storms Z. Li et al. 10.1007/s11207-010-9559-7
237. Radial Sizes and Expansion Behavior of ICMEs in Solar Cycles 23 and 24 W. Mishra  et al. 10.3389/fspas.2021.713999
238. Parameter Distributions for the Drag‐Based Modeling of CME Propagation G. Napoletano et al. 10.1029/2021SW002925
239. Dynamic and Thermal Disappearance of Prominences and Their Geoeffectiveness L. Taliashvili et al. 10.1007/s11207-009-9414-x
240. The evolution of coronal mass ejections in the inner heliosphere: Implementing the spheromak model with EUHFORIA C. Verbeke et al. 10.1051/0004-6361/201834702
241. Coronal Mass Ejections travel time C. Braga et al. 10.1017/S1743921317003714
242. Periodic Appearance of Coronal Holes and the Related Variation of Solar Wind Parameters M. Temmer et al. 10.1007/s11207-007-0336-1
243. The inversion of the real kinematic properties of coronal mass ejections by forward modeling Y. Wu & P. Chen 10.1088/1674-4527/11/2/011
244. CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU C. Möstl et al. 10.1088/0004-637X/787/2/119
245. Evaluation of a Revised Interplanetary Shock Prediction Model: 1D CESE-HD-2 Solar-Wind Model Y. Zhang et al. 10.1007/s11207-014-0513-y
246. Field-Line Draping Around ICMES Z. Kaymaz & G. Siscoe 10.1007/s11207-006-0308-x
247. Characterization of the Complex Ejecta Measured In Situ on 19 – 22 March 2001 by Six Different Methods A. Ojeda-González et al. 10.1007/s11207-017-1182-4
248. Propagation of coronal mass ejections from the Sun to the Earth W. MISHRA & L. TERIACA 10.1007/s12036-023-09910-6
249. Transfer Entropy Approach to Discovering the Ranking of Solar Wind Drivers to Geomagnetic Storm J. YU et al. 10.11728/cjss2022.03.210406045
250. Forecast evaluation of the coronal mass ejection (CME) geoeffectiveness using halo CMEs from 1997 to 2003 R. Kim et al. 10.1029/2005JA011218
251. Projection effects in coronal mass ejections B. Vršnak et al. 10.1051/0004-6361:20077175
252. Overexpansion-dominated coronal mass ejection formation and induced radio bursts B. Wang et al. 10.1051/0004-6361/202244275
253. Observation-based modelling of magnetised coronal mass ejections with EUHFORIA C. Scolini et al. 10.1051/0004-6361/201935053
254. MHD study of the planetary magnetospheric response during extreme solar wind conditions: Earth and exoplanet magnetospheres applications J. Varela et al. 10.1051/0004-6361/202141181
255. ICMEs in the Inner Heliosphere: Origin, Evolution and Propagation Effects R. Forsyth et al. 10.1007/s11214-006-9022-0
256. Multipoint observations of coronal mass ejection and solar energetic particle events on Mars and Earth during November 2001 T. Falkenberg et al. 10.1029/2010JA016279
257. A comparison of CME expansion speeds between solar cycles 23 and 24 F. Dagnew et al. 10.1088/1742-6596/1620/1/012003
258. Refined Modeling of Geoeffective Fast Halo CMEs During Solar Cycle 24 E. Yordanova et al. 10.1029/2023SW003497
259. Sources of SEP Acceleration during a Flare – CME Event N. Lehtinen et al. 10.1007/s11207-007-9093-4
260. Evolution of the Radial Size and Expansion of Coronal Mass Ejections Investigated by Combining Remote and In Situ Observations B. Zhuang et al. 10.3847/1538-4357/acd847
261. Acceleration and Expansion of a Coronal Mass Ejection in the High Corona: Role of Magnetic Reconnection B. Zhuang et al. 10.3847/1538-4357/ac75d4
262. Energy spectrum of interplanetary magnetic flux ropes and its connection with solar activity D. Wu et al. 10.1051/0004-6361:20079173
263. Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision M. Xiong et al. 10.1029/2009JA014079
264. Type IV Radio Bursts and Associated Active Regions in Sunspot Cycle 24 A. Kumari 10.1007/s11207-022-02032-2
265. Statistical Study of Geo-Effectiveness of Planar Magnetic Structures Evolved within ICME’s K. Ghag et al. 10.3390/universe9080350
266. Full Velocities and Propagation Directions of Coronal Mass Ejections Inferred from Simultaneous Full-disk Imaging and Sun-as-a-star Spectroscopic Observations H. Lu et al. 10.3847/1538-4357/acd6a1
267. Linking Remote-Sensing and In Situ Observations of Coronal Mass Ejections Using STEREO L. Rodriguez et al. 10.1007/s11207-011-9784-8
268. The challenge of predicting the occurrence of intense storms N. Srivastava 10.1007/BF02702526
269. The role of aerodynamic drag in dynamics of coronal mass ejections B. Vršnak et al. 10.1017/S1743921309029391
270. Magnetohydrodynamic Simulation of Multiple Coronal Mass Ejections: An Effect of “Pre-events” C. Wu et al. 10.3847/1538-4357/ac7f2a
271. Phase shift (time) between storm-time maximum negative excursions of geomagnetic disturbance index Dst and interplanetary Bz R. Kane & E. Echer 10.1016/j.jastp.2007.03.008
272. Full halo coronal mass ejections: Do we need to correct the projection effect in terms of velocity? C. Shen et al. 10.1002/2013JA018872
273. MEASURING THE MAGNETIC FIELD OF CORONAL MASS EJECTIONS NEAR THE SUN USING PULSARS T. Howard et al. 10.3847/0004-637X/831/2/208
274. Modeling a Coronal Mass Ejection from an Extended Filament Channel. II. Interplanetary Propagation to 1 au E. Palmerio et al. 10.3847/1538-4357/ad0229
275. Geoeffectiveness of an Eruptive Prominence V. Parkhomov et al. 10.17150/2713-1734.2022.4(2).123-151
276. Space weather explorer – The KuaFu mission C. Tu et al. 10.1016/j.asr.2007.04.049
277. Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum E. Kilpua et al. 10.1007/s11207-014-0552-4