140 citations as recorded by crossref.

1. Stream Interactions and Interplanetary Coronal Mass Ejections at 0.72 AU L. Jian et al. 10.1007/s11207-008-9161-4
2. Multipoint Study of Successive Coronal Mass Ejections Driving Moderate Disturbances at 1 au E. Palmerio et al. 10.3847/1538-4357/ab1850
3. Observations of ICMEs and ICME-like Solar Wind Structures from 2007 – 2010 Using Near-Earth and STEREO Observations E. Kilpua et al. 10.1007/s11207-012-9957-0
4. Effect of solar features and interplanetary parameters on geomagnetosphere during solar cycle-23 S. Kumar & A. Raizada 10.1007/s12043-008-0189-7
5. Multi-spacecraft observed magnetic clouds as seen by Helios mission A. de Lucas et al. 10.1016/j.jastp.2011.02.007
6. Partially ejected flux ropes: Implications for interplanetary coronal mass ejections S. Gibson & Y. Fan 10.1029/2008JA013151
7. Understanding the variability of magnetic storms caused by ICMEs R. Benacquista et al. 10.5194/angeo-35-147-2017
8. Statistical Comparison of Magnetic Clouds with Non-magnetic Clouds in Interplanetary Coronal Mass Ejections for Solar Cycle 24 F. LOU & Y. YE 10.11728/cjss2017.04.381
9. 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
10. Numerical simulations of ICME–ICME interactions T. Niembro et al. 10.1051/swsc/2018049
11. Solar Energetic Particle Events and Forbush Decreases Driven by the Same Solar Sources A. Belov et al. 10.3390/universe8080403
12. Pursuing Forecasts of the Behavior and Arrival of Coronal Mass Ejections through Modeling and Observations H. Cremades 10.1017/S1743921317010882
13. Forbush decreases associated with coronal mass ejections from active and non-active regions: statistical comparison A. Melkumyan et al. 10.1093/mnras/stac2017
14. First Observations of the Disruption of the Earth's Foreshock Wave Field During Magnetic Clouds L. Turc et al. 10.1029/2019GL084437
15. Forbush Decreases and Geomagnetic Disturbances: 1. Events Associated with Different Types of Solar and Interplanetary Sources A. Melkumyan et al. 10.1134/S0016793223600650
16. The geo-effectiveness of interplanetary small-scale magnetic fluxropes X. Zhang et al. 10.1016/j.jastp.2012.12.006
17. Do All Interplanetary Coronal Mass Ejections Have a Magnetic Flux Rope Structure Near 1 au? H. Song et al. 10.3847/2041-8213/abb6ec
18. A Study of Fluctuations in Magnetic Cloud‐Driven Sheaths C. Moissard et al. 10.1029/2019JA026952
19. Consequences of the force‐free model of magnetic clouds for their heliospheric evolution M. Leitner et al. 10.1029/2006JA011940
20. Development of Forbush Decreases Associated with Coronal Ejections from Active Regions and non-Active Regions A. Melkumyan et al. 10.1134/S0016793222600394
21. Geoeffectiveness (Dst and Kp) of interplanetary coronal mass ejections during 1995–2009 and implications for storm forecasting I. Richardson & H. Cane 10.1029/2011SW000670
22. Outer Van Allen belt trapped and precipitating electron flux responses to two interplanetary magnetic clouds of opposite polarity H. George et al. 10.5194/angeo-38-931-2020
23. Understanding the Internal Magnetic Field Configurations of ICMEs Using More than 20 Years of Wind Observations T. Nieves-Chinchilla et al. 10.1007/s11207-018-1247-z
24. High-latitude GPS phase scintillation and cycle slips during high-speed solar wind streams and interplanetary coronal mass ejections: a superposed epoch analysis P. Prikryl et al. 10.1186/1880-5981-66-62
25. Relative occurrence rate and geoeffectiveness of large-scale types of the solar wind Y. Yermolaev et al. 10.1134/S0010952510010016
26. Geoeffectiveness of solar wind interplanetary magnetic structures M. Alves et al. 10.1016/j.jastp.2010.07.024
27. Rotation and interaction of the CMEs of September 8 and 10, 2014, tested with EUHFORIA A. Maharana et al. 10.1051/0004-6361/202345902
28. Coronal mass ejections and their sheath regions in interplanetary space E. Kilpua et al. 10.1007/s41116-017-0009-6
29. Similarities and Differences between Forbush Decreases Associated with Streams from Coronal Holes, Filament Ejections, and Ejections from Active Regions A. Melkumyan et al. 10.1134/S0016793222030112
30. Forbush Decreases and Associated Geomagnetic Storms: Statistical Comparison in Solar Cycles 23 and 24 A. Melkumyan et al. 10.1007/s11207-024-02281-3
31. Magnetic clouds' structure in the magnetosheath as observed by Cluster and Geotail: four case studies L. Turc et al. 10.5194/angeo-32-1247-2014
32. Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness M. Xiong et al. 10.1029/2007JA012320
33. Solar connections of geoeffective magnetic structures N. Gopalswamy 10.1016/j.jastp.2008.06.010
34. New Metric for Minimum Variance Analysis Validation in the Study of Interplanetary Magnetic Clouds R. Rosa Oliveira et al. 10.1007/s11207-020-01610-6
35. Statistical Study of ICMEs and Their Sheaths During Solar Cycle 23 (1996 – 2008) E. Mitsakou & X. Moussas 10.1007/s11207-014-0505-y
36. AN EMPIRICAL RECONSTRUCTION OF THE 2008 APRIL 26 CORONAL MASS EJECTION B. Wood & R. Howard 10.1088/0004-637X/702/2/901
37. Interhemispheric comparison of GPS phase scintillation at high latitudes during the magnetic-cloud-induced geomagnetic storm of 5–7 April 2010 P. Prikryl et al. 10.5194/angeo-29-2287-2011
38. Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations S. Yardley et al. 10.1051/0004-6361/202141142
39. Magnetic Structure and Propagation of Two Interacting CMEs From the Sun to Saturn E. Palmerio et al. 10.1029/2021JA029770
40. Statistical analysis of interplanetary coronal mass ejections and their geoeffectiveness during the solar cycles 23 and 24 P. Alexakis & H. Mavromichalaki 10.1007/s10509-019-3677-y
41. Asymmetric development of magnetospheric storms during magnetic clouds and sheath regions K. Huttunen et al. 10.1029/2005GL024894
42. Development of Forbush Decreases Associated with Coronal Ejections from Active Regions and non-Active Regions A. Melkumyan et al. 10.31857/S0016794022060098
43. 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
44. ICMEs in the Inner Heliosphere: Origin, Evolution and Propagation Effects R. Forsyth et al. 10.1007/s11214-006-9022-0
45. 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
46. Geoeffectiveness and efficiency of CIR, sheath, and ICME in generation of magnetic storms Y. Yermolaev et al. 10.1029/2011JA017139
47. Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections P. Démoulin et al. 10.1007/s11207-008-9221-9
48. 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
49. Solar energetic electron probes of magnetic cloud field line lengths S. Kahler et al. 10.1029/2010JA015328
50. Multi-Spacecraft Study of the 21 January 2005 ICME C. Foullon et al. 10.1007/s11207-007-0355-y
51. Radial Evolution of Coronal Mass Ejections Between MESSENGER, Venus Express, STEREO, and L1: Catalog and Analysis T. Salman et al. 10.1029/2019JA027084
52. A comparison of bow shock models with Cluster observations during low Alfvén Mach number magnetic clouds L. Turc et al. 10.5194/angeo-31-1011-2013
53. High-rigidity Forbush decreases: due to CMEs or shocks? K. Arunbabu et al. 10.1051/0004-6361/201220830
54. 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
55. CME–CME Interactions as Sources of CME Geoeffectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in 2017 Early September C. Scolini et al. 10.3847/1538-4365/ab6216
56. Galactic Cosmic Ray Density Variations in Magnetic Clouds A. Belov et al. 10.1007/s11207-015-0678-z
57. Determining the Intrinsic CME Flux Rope Type Using Remote-sensing Solar Disk Observations E. Palmerio et al. 10.1007/s11207-017-1063-x
58. Forbush Decreases and Geomagnetic Disturbances: 1. Events Associated with Different Types of Solar and Interplanetary Sources A. Melkumyan et al. 10.31857/S0016794023600503
59. Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations A. Ojeda González et al. 10.1016/S0016-7169(14)71494-1
60. Interplanetary Coronal Mass Ejections Observed by MESSENGER and Venus Express S. Good & R. Forsyth 10.1007/s11207-015-0828-3
61. Minimum Variance Analysis of Interplanetary Coronal Mass Ejections Around Solar Cycle 23 Maximum (1998–2002) E. Echer et al. 10.1007/s11207-006-2380-7
62. Multipoint ICME encounters: Pre-STEREO and STEREO observations E. Kilpua et al. 10.1016/j.jastp.2010.10.012
63. Interplanetary conditions causing intense geomagnetic storms (Dst ≤ −100 nT) during solar cycle 23 (1996–2006) E. Echer et al. 10.1029/2007JA012744
64. Thermospheric nitric oxide response to shock‐led storms D. Knipp et al. 10.1002/2016SW001567
65. Modeling the behavior of the cosmic ray density in magnetic clouds A. Belov et al. 10.1088/1742-6596/632/1/012051
66. Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison E. Mitsakou et al. 10.1016/j.asr.2008.08.003
67. PC index as a proxy of the solar wind energy that entered into the magnetosphere: 3. Development of magnetic storms O. Troshichev & D. Sormakov 10.1016/j.jastp.2017.10.012
68. Solar cycle–dependent helicity transport by magnetic clouds B. Lynch et al. 10.1029/2005JA011137
69. On the Spatial Coherence of Magnetic Ejecta: Measurements of Coronal Mass Ejections by Multiple Spacecraft Longitudinally Separated by 0.01 au N. Lugaz et al. 10.3847/2041-8213/aad9f4
70. Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005 J. Zhang et al. 10.1029/2007JA012321
71. Study of local regularities in solar wind data and ground magnetograms V. Klausner et al. 10.1016/j.jastp.2014.01.013
72. A Stealth CME Bracketed between Slow and Fast Wind Producing Unexpected Geoeffectiveness W. He et al. 10.3847/1538-4357/aac381
73. Low-latitude ionospheric response from GPS, IRI and TIE-GCM TEC to Solar Cycle 24 S. Rao et al. 10.1007/s10509-019-3701-2
74. Multipoint Observations of the June 2012 Interacting Interplanetary Flux Ropes E. Kilpua et al. 10.3389/fspas.2019.00050
75. On the relationship between interplanetary coronal mass ejections and magnetic clouds E. Kilpua et al. 10.5194/angeo-31-1251-2013
76. Geoeffectiveness of Coronal Mass Ejections in the SOHO Era M. Dumbović et al. 10.1007/s11207-014-0613-8
77. Galactic Cosmic Ray Intensity Response to Interplanetary Coronal Mass Ejections/Magnetic Clouds in 1995 – 2009 I. Richardson & H. Cane 10.1007/s11207-011-9774-x
78. On Fields and Mass Constraints for the Uniform Propagation of Magnetic-Flux Ropes Undergoing Isotropic Expansion D. Berdichevsky 10.1007/s11207-012-0176-5
79. Forbush Effects Created by Coronal Mass Ejections with Magnetic Clouds M. Abunina et al. 10.1134/S0016793221050029
80. Main Time Characteristics of Cosmic Ray Variations and Related Parameters in Magnetic Clouds M. Abunina et al. 10.1134/S0016793223600856
81. Geoeffectiveness of magnetic clouds occurred during solar cycle 23 S. Kumar & A. Raizada 10.1016/j.pss.2009.11.009
82. The flux rope nature of coronal mass ejections A. Vourlidas 10.1088/0741-3335/56/6/064001
83. Cosmic ray cutoff rigidity governing by solar wind and magnetosphere parameters during the 2017 Sep 6–9 solar-terrestrial event N. Ptitsyna et al. 10.1016/j.jastp.2023.106067
84. Periodicity in the most violent solar eruptions: recent observations of coronal mass ejections and flares revisited P. Gao et al. 10.1088/1674-4527/12/3/008
85. Estimating the Magnetic Structure of an Erupting CME Flux Rope From AR12158 Using Data-Driven Modeling E. Kilpua et al. 10.3389/fspas.2021.631582
86. 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
87. An Observationally Constrained Analytical Model for Predicting the Magnetic Field Vectors of Interplanetary Coronal Mass Ejections at 1 au R. Sarkar et al. 10.3847/1538-4357/ab5fd7
88. 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
89. Solar sources and geospace consequences of interplanetary magnetic clouds observed during solar cycle 23 N. Gopalswamy et al. 10.1016/j.jastp.2007.08.070
90. Geoeffective Properties of Solar Transients and Stream Interaction Regions E. Kilpua et al. 10.1007/s11214-017-0411-3
91. Lack of relationship between geoeffectiveness and orientations of magnetic clouds with bipolar Bz and unipolar southward Bz W. Teh et al. 10.1016/j.pss.2014.11.021
92. Studying the Spheromak Rotation in Data-constrained Coronal Mass Ejection Modeling with EUHFORIA and Assessing Its Effect on the B z Prediction R. Sarkar et al. 10.3847/1538-4365/ad0df4
93. Statistical comparison of time profiles of Forbush decreases associated with coronal mass ejections and streams from coronal holes in solar cycles 23–24 A. Melkumyan et al. 10.1093/mnras/stad772
94. Solar and interplanetary triggers of the largest Dst variations of the solar cycle 23 Y. Cerrato et al. 10.1016/j.jastp.2011.09.001
95. Comparison of geoeffectiveness of coronal mass ejections and corotating interaction regions G. Verbanac et al. 10.1051/0004-6361/201220417
96. Commission 10: Solar Activity D. Melrose et al. 10.1017/S1743921306004388
97. 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
98. Modeling variations in CR density in magnetic clouds A. Belov et al. 10.3103/S1062873815050159
99. Solar flare associated coronal mass ejections causing geo-effectiveness and Forbush decreases B. Bhatt & H. Chandra 10.1007/s10509-017-3024-0
100. Benchmarking CME Arrival Time and Impact: Progress on Metadata, Metrics, and Events C. Verbeke et al. 10.1029/2018SW002046
101. Geoeffectivity of Coronal Mass Ejections H. Koskinen & K. Huttunen 10.1007/s11214-006-9103-0
102. Magnetic clouds and origins in STEREO era L. Yan et al. 10.1002/2013JA019538
103. Nonlinear fluctuation analysis for a set of 41 magnetic clouds measured by the Advanced Composition Explorer (ACE) spacecraft A. Ojeda González et al. 10.5194/npg-21-1059-2014
104. Main time characteristics of cosmic ray variations and related parameters in magnetic clouds M. Abunina et al. 10.31857/S0016794024010048
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106. On the relationship between magnetic cloud field polarity and geoeffectiveness E. Kilpua et al. 10.5194/angeo-30-1037-2012
107. Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23 E. Echer et al. 10.1029/2007GL031755
108. The Relationship between the Magnetic Cloud Boundary Layer and the Substorm Expansion Phase P. Zuo et al. 10.1007/s11207-007-0407-3
109. Density variations of galactic cosmic rays in magnetic clouds A. Belov et al. 10.1134/S0016793215040027
110. Forecasting the Structure and Orientation of Earthbound Coronal Mass Ejections E. Kilpua et al. 10.1029/2018SW001944
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112. 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
113. A model of the magnetosheath magnetic field during magnetic clouds L. Turc et al. 10.5194/angeo-32-157-2014
114. Unraveling the Internal Magnetic Field Structure of the Earth-directed Interplanetary Coronal Mass Ejections During 1995 – 2015 T. Nieves-Chinchilla et al. 10.1007/s11207-019-1477-8
115. Investigating the variations in the composition and heating of interacting ICMEs N. Srivastava et al. 10.3389/fspas.2023.1154612
116. Forecasting Periods of Strong Southward Magnetic Field Following Interplanetary Shocks T. Salman et al. 10.1029/2018SW002056
117. Comparison of the Characteristics of Magnetic Clouds and Magnetic Cloud-Like Structures for the Events of 1995 – 2003 C. Wu & R. Lepping 10.1007/s11207-007-0323-6
118. Coronal Magnetic Structure of Earthbound CMEs and In Situ Comparison E. Palmerio et al. 10.1002/2017SW001767
119. Analysis of GPS-TEC and IRI model over equatorial and EIA stations during solar cycle 24 S. Kumar Chaurasiya et al. 10.1016/j.asr.2023.09.014
120. Distributions of Energy and Mass of Coronal Mass Ejections P. Gao et al. 10.1007/s11207-011-9853-z
121. ROTATION OF CORONAL MASS EJECTIONS DURING ERUPTION B. Lynch et al. 10.1088/0004-637X/697/2/1918
122. From space weather toward space climate time scales: Substorm analysis from 1993 to 2008 E. Tanskanen et al. 10.1029/2010JA015788
123. The Automatic Predictability of Super Geomagnetic Storms from halo CMEs associated with Large Solar Flares H. Song et al. 10.1007/s11207-006-0164-8
124. 20 Years of ACE Data: How Superposed Epoch Analyses Reveal Generic Features in Interplanetary CME Profiles F. Regnault et al. 10.1029/2020JA028150
125. Multispacecraft recovery of a magnetic cloud and its origin from magnetic reconnection on the Sun C. Möstl et al. 10.1029/2008JA013657
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127. A STATISTICAL STUDY OF THE AVERAGE IRON CHARGE STATE DISTRIBUTIONS INSIDE MAGNETIC CLOUDS FOR SOLAR CYCLE 23 H. Song et al. 10.3847/0067-0049/224/2/27
128. Elliptical magnetic clouds and geomagnetic storms I. Antoniadou et al. 10.1016/j.pss.2007.10.002
129. ROTATION OF WHITE-LIGHT CORONAL MASS EJECTION STRUCTURES AS INFERRED FROM LASCO CORONAGRAPH V. Yurchyshyn et al. 10.1088/0004-637X/705/1/426
130. Cosmic noise absorption signature of particle precipitation during interplanetary coronal mass ejection sheaths and ejecta E. Kilpua et al. 10.5194/angeo-38-557-2020
131. On the variation of interplanetary magnetic cloud type through solar cycle 23: Wind events R. Lepping & C. Wu 10.1029/2006JA012140
132. Forbush decreases and turbulence levels at coronal mass ejection fronts P. Subramanian et al. 10.1051/0004-6361:200809551
133. Forward Modeling of Coronal Mass Ejection Flux Ropes in the Inner Heliosphere with 3DCORE C. Möstl et al. 10.1002/2017SW001735
134. Solar Wind Properties and Geospace Impact of Coronal Mass Ejection‐Driven Sheath Regions: Variation and Driver Dependence E. Kilpua et al. 10.1029/2019SW002217
135. A Statistical Study of Solar Filament Eruptions that Form High-speed Coronal Mass Ejections P. Zou et al. 10.3847/1538-4357/ab4355
136. A Catalog of Interplanetary Coronal Mass Ejections Observed by Juno between 1 and 5.4 au E. Davies et al. 10.3847/1538-4357/ac2ccb
137. Difference in the parameters of ICMEs in Ejecta and Sheath region and their impact on Dst index during 1997–2014 A. Goswami 10.1016/j.asr.2018.05.017
138. Modeling inner boundary values at 18 solar radii during solar quiet time for global three-dimensional time-dependent magnetohydrodynamic numerical simulation C. Wu et al. 10.1016/j.jastp.2020.105211
139. Solar Wind Low-Temperature Periods and Forbush Decreases: a Statistical Comparison A. Melkumyan et al. 10.1134/S0016793224600565
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