66 citations as recorded by crossref.

1. The Magnetic Morphology of Magnetic Clouds: Multi-spacecraft Investigation of Twisted and Writhed Coronal Mass Ejections N. Al-Haddad et al. 10.3847/1538-4357/aaf38d
2. Wind Magnetic Clouds for the Period 2013 – 2015: Model Fitting, Types, Associated Shock Waves, and Comparisons to Other Periods R. Lepping et al. 10.1007/s11207-018-1273-x
3. Machine Learning Approach for Solar Wind Categorization H. Li et al. 10.1029/2019EA000997
4. Classifying Different Types of Solar-Wind Plasma with Uncertainty Estimations Using Machine Learning T. Narock et al. 10.1007/s11207-024-02379-8
5. Statistical Comparison of Magnetic Clouds with Interplanetary Coronal Mass Ejections for Solar Cycle 23 C. Wu & R. Lepping 10.1007/s11207-010-9684-3
6. Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation M. Janvier et al. 10.1051/0004-6361/201321442
7. The first super geomagnetic storm of solar cycle 24: “The St. Patrick’s day event (17 March 2015)” C. Wu et al. 10.1186/s40623-016-0525-y
8. The Width of Magnetic Ejecta Measured near 1 au: Lessons from STEREO-A Measurements in 2021–2022 N. Lugaz et al. 10.3847/1538-4357/ad17b9
9. Wind Magnetic Clouds for 2010 – 2012: Model Parameter Fittings, Associated Shock Waves, and Comparisons to Earlier Periods R. Lepping et al. 10.1007/s11207-015-0755-3
10. Physics‐based solar wind driver functions for the magnetosphere: Combining the reconnection‐coupled MHD generator with the viscous interaction J. Borovsky 10.1002/jgra.50557
11. Does spacecraft trajectory strongly affect detection of magnetic clouds? P. Démoulin et al. 10.1051/0004-6361/201220535
12. Geomagnetic activity associated with magnetic clouds, magnetic cloud-like structures and interplanetary shocks for the period 1995–2003 C. Wu & R. Lepping 10.1016/j.asr.2007.02.027
13. Estimating the effects of ionospheric plasma on solar wind/magnetosphere coupling via mass loading of dayside reconnection: Ion‐plasma‐sheet oxygen, plasmaspheric drainage plumes, and the plasma cloak J. Borovsky et al. 10.1002/jgra.50527
14. Comparison of I-ICME and M-ICME Fittings and In Situ Observation Parameters for Solar Cycles 23 and 24 and Their Influence on Geoeffectiveness Z. Zhang et al. 10.1007/s11207-023-02225-3
15. 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
16. Properties and geoeffectiveness of magnetic clouds during solar cycles 23 and 24 N. Gopalswamy et al. 10.1002/2015JA021446
17. Space weather effects on the bow shock, the magnetic barrier, and the ion composition boundary at Venus D. Vech et al. 10.1002/2014JA020782
18. RU-net: A Residual U-net for Automatic Interplanetary Coronal Mass Ejection Detection J. Chen et al. 10.3847/1538-4365/ac4587
19. Multi-Spacecraft Study of the 21 January 2005 ICME C. Foullon et al. 10.1007/s11207-007-0355-y
20. Average Thickness of Magnetosheath Upstream of Magnetic Clouds at 1 AU versus Solar Longitude of Source R. Lepping et al. 10.1007/s11207-007-9111-6
21. On the variations of the solar wind magnetic field about the Parker spiral direction J. Borovsky 10.1029/2009JA015040
22. A new four‐plasma categorization scheme for the solar wind F. Xu & J. Borovsky 10.1002/2014JA020412
23. Statistical study of magnetic cloud erosion by magnetic reconnection A. Ruffenach et al. 10.1002/2014JA020628
24. A Quarter Century ofWindSpacecraft Discoveries L. Wilson et al. 10.1029/2020RG000714
25. Simultaneous multi-class detection of interplanetary space weather events G. Nguyen et al. 10.1051/swsc/2025016
26. CME propagation through the heliosphere: Status and future of observations and model development M. Temmer et al. 10.1016/j.asr.2023.07.003
27. Relationships Among Magnetic Clouds, CMES, and Geomagnetic Storms C. Wu et al. 10.1007/s11207-006-0037-1
28. Some Properties of the Solar Wind Turbulence at 1 AU Statistically Examined in the Different Types of Solar Wind Plasma J. Borovsky et al. 10.1029/2019JA026580
29. Investigating Coronal Mass Ejections through Multispacecraft Measurements: STEREO-A and L1 in 2022–2023 S. Banu et al. 10.3847/1538-4357/adb60c
30. Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005 J. Zhang et al. 10.1029/2007JA012321
31. STEREO Observations of Interplanetary Coronal Mass Ejections in 2007–2016 L. Jian et al. 10.3847/1538-4357/aab189
32. 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
33. Yearly Comparison of Magnetic Cloud Parameters, Sunspot Number, and Interplanetary Quantities for the First 18 Years of the Wind Mission R. Lepping et al. 10.1007/s11207-014-0622-7
34. Understanding the variability of magnetic storms caused by ICMEs R. Benacquista et al. 10.5194/angeo-35-147-2017
35. Relationships Among Geomagnetic Storms, Interplanetary Shocks, Magnetic Clouds, and Sunspot Number During 1995 – 2012 C. Wu & R. Lepping 10.1007/s11207-015-0806-9
36. Longitudinally spaced observations of a magnetic-cloud-like structure embedded in a co-rotating interaction region M. Maunder et al. 10.5194/angeo-43-37-2025
37. Statistical relationship between solar wind conditions and geomagnetic storms in 1998–2008 D. Xu et al. 10.1016/j.pss.2009.07.015
38. The Electron Structure of the Solar Wind J. Borovsky et al. 10.3389/fspas.2021.690005
39. A STEREO Survey of Magnetic Cloud Coronal Mass Ejections Observed at Earth in 2008–2012 B. Wood et al. 10.3847/1538-4365/229/2/29
40. Model Fitting of Wind Magnetic Clouds for the Period 2004 – 2006 R. Lepping et al. 10.1007/s11207-020-01630-2
41. Exploring the radial evolution of interplanetary coronal mass ejections using EUHFORIA C. Scolini et al. 10.1051/0004-6361/202040226
42. Differences between CME‐driven storms and CIR‐driven storms J. Borovsky & M. Denton 10.1029/2005JA011447
43. 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
44. 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
45. Magnetic Clouds at/near the 2007 – 2009 Solar Minimum: Frequency of Occurrence and Some Unusual Properties R. Lepping et al. 10.1007/s11207-010-9646-9
46. 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
47. 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
48. Comparisons of Characteristics of Magnetic Clouds and Cloud-Like Structures During 1995 – 2012 C. Wu & R. Lepping 10.1007/s11207-015-0656-5
49. Substorm occurrence rates, substorm recurrence times, and solar wind structure J. Borovsky & K. Yakymenko 10.1002/2016JA023625
50. Classification Scheme for Solar Wind I. Veselovsky et al. 10.1134/S1063778818050186
51. Automatic Detection of Interplanetary Coronal Mass Ejections from In Situ Data: A Deep Learning Approach G. Nguyen et al. 10.3847/1538-4357/ab0d24
52. A new class of complex ejecta resulting from the interaction of two CMEs and its expected geoeffectiveness N. Lugaz & C. Farrugia 10.1002/2013GL058789
53. 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
54. 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
55. The plasma structure of coronal hole solar wind: Origins and evolution J. Borovsky 10.1002/2016JA022686
56. The trailing edges of high‐speed streams at 1 AU J. Borovsky & M. Denton 10.1002/2016JA022863
57. Are There Different Populations of Flux Ropes in the Solar Wind? M. Janvier et al. 10.1007/s11207-014-0486-x
58. Properties of Interplanetary Coronal Mass Ejections N. Gopalswamy 10.1007/s11214-006-9102-1
59. Major geomagnetic storms (Dst ≤ −100 nT) generated by corotating interaction regions I. Richardson et al. 10.1029/2005JA011476
60. Observations of an interplanetary switch‐on shock driven by a magnetic cloud H. Feng et al. 10.1029/2009GL037354
61. Are all leading shocks driven by magnetic clouds? H. Feng et al. 10.1029/2009JA014875
62. Alfvén wave‐driven ionospheric mass outflow and electron precipitation during storms S. Hatch et al. 10.1002/2016JA022805
63. Magnetic Flux and Helicity of Magnetic Clouds P. Démoulin et al. 10.1007/s11207-015-0836-3
64. Coronal Mass Ejections travel time C. Braga et al. 10.1017/S1743921317003714
65. Relationships for predicting magnetic cloud-related geomagnetic storm intensity C. Wu & R. Lepping 10.1016/j.jastp.2004.07.040
66. An Alternative Method for Identifying Interplanetary Magnetic Cloud Regions A. Ojeda-Gonzalez et al. 10.3847/1538-4357/aa6034