67 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.
2. Wind Magnetic Clouds for the Period 2013 – 2015: Model Fitting, Types, Associated Shock Waves, and Comparisons to Other Periods R. Lepping et al.
3. Machine Learning Approach for Solar Wind Categorization H. Li et al.
4. Classifying Different Types of Solar-Wind Plasma with Uncertainty Estimations Using Machine Learning T. Narock et al.
5. Statistical Comparison of Magnetic Clouds with Interplanetary Coronal Mass Ejections for Solar Cycle 23 C. Wu & R. Lepping
6. Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation M. Janvier et al.
7. The first super geomagnetic storm of solar cycle 24: “The St. Patrick’s day event (17 March 2015)” C. Wu et al.
8. The Width of Magnetic Ejecta Measured near 1 au: Lessons from STEREO-A Measurements in 2021–2022 N. Lugaz et al.
9. Wind Magnetic Clouds for 2010 – 2012: Model Parameter Fittings, Associated Shock Waves, and Comparisons to Earlier Periods R. Lepping et al.
10. Physics‐based solar wind driver functions for the magnetosphere: Combining the reconnection‐coupled MHD generator with the viscous interaction J. Borovsky
11. Does spacecraft trajectory strongly affect detection of magnetic clouds? P. Démoulin et al.
12. Geomagnetic activity associated with magnetic clouds, magnetic cloud-like structures and interplanetary shocks for the period 1995–2003 C. Wu & R. Lepping
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.
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.
15. The 04 – 10 September 2017 Sun–Earth Connection Events: Solar Flares, Coronal Mass Ejections/Magnetic Clouds, and Geomagnetic Storms C. Wu et al.
16. Properties and geoeffectiveness of magnetic clouds during solar cycles 23 and 24 N. Gopalswamy et al.
17. Space weather effects on the bow shock, the magnetic barrier, and the ion composition boundary at Venus D. Vech et al.
18. RU-net: A Residual U-net for Automatic Interplanetary Coronal Mass Ejection Detection J. Chen et al.
19. Multi-Spacecraft Study of the 21 January 2005 ICME C. Foullon et al.
20. Average Thickness of Magnetosheath Upstream of Magnetic Clouds at 1 AU versus Solar Longitude of Source R. Lepping et al.
21. On the variations of the solar wind magnetic field about the Parker spiral direction J. Borovsky
22. A new four‐plasma categorization scheme for the solar wind F. Xu & J. Borovsky
23. Statistical study of magnetic cloud erosion by magnetic reconnection A. Ruffenach et al.
24. A Quarter Century ofWindSpacecraft Discoveries L. Wilson et al.
25. Simultaneous multi-class detection of interplanetary space weather events G. Nguyen et al.
26. CME propagation through the heliosphere: Status and future of observations and model development M. Temmer et al.
27. Relationships Among Magnetic Clouds, CMES, and Geomagnetic Storms C. Wu et al.
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.
29. Investigating Coronal Mass Ejections through Multispacecraft Measurements: STEREO-A and L1 in 2022–2023 S. Banu et al.
30. Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005 J. Zhang et al.
31. Geo-effectiveness of ICMES/MCs of different magnetic-polarity configurations W. Alotaibi et al.
32. STEREO Observations of Interplanetary Coronal Mass Ejections in 2007–2016 L. Jian et al.
33. 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.
34. Yearly Comparison of Magnetic Cloud Parameters, Sunspot Number, and Interplanetary Quantities for the First 18 Years of the Wind Mission R. Lepping et al.
35. Understanding the variability of magnetic storms caused by ICMEs R. Benacquista et al.
36. Relationships Among Geomagnetic Storms, Interplanetary Shocks, Magnetic Clouds, and Sunspot Number During 1995 – 2012 C. Wu & R. Lepping
37. Longitudinally spaced observations of a magnetic-cloud-like structure embedded in a co-rotating interaction region M. Maunder et al.
38. Statistical relationship between solar wind conditions and geomagnetic storms in 1998–2008 D. Xu et al.
39. The Electron Structure of the Solar Wind J. Borovsky et al.
40. A STEREO Survey of Magnetic Cloud Coronal Mass Ejections Observed at Earth in 2008–2012 B. Wood et al.
41. Model Fitting of Wind Magnetic Clouds for the Period 2004 – 2006 R. Lepping et al.
42. Exploring the radial evolution of interplanetary coronal mass ejections using EUHFORIA C. Scolini et al.
43. Differences between CME‐driven storms and CIR‐driven storms J. Borovsky & M. Denton
44. Comparison of the Characteristics of Magnetic Clouds and Magnetic Cloud-Like Structures for the Events of 1995 – 2003 C. Wu & R. Lepping
45. Understanding the Internal Magnetic Field Configurations of ICMEs Using More than 20 Years of Wind Observations T. Nieves-Chinchilla et al.
46. Magnetic Clouds at/near the 2007 – 2009 Solar Minimum: Frequency of Occurrence and Some Unusual Properties R. Lepping et al.
47. 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.
48. 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.
49. Comparisons of Characteristics of Magnetic Clouds and Cloud-Like Structures During 1995 – 2012 C. Wu & R. Lepping
50. Substorm occurrence rates, substorm recurrence times, and solar wind structure J. Borovsky & K. Yakymenko
51. Classification Scheme for Solar Wind I. Veselovsky et al.
52. Automatic Detection of Interplanetary Coronal Mass Ejections from In Situ Data: A Deep Learning Approach G. Nguyen et al.
53. A new class of complex ejecta resulting from the interaction of two CMEs and its expected geoeffectiveness N. Lugaz & C. Farrugia
54. Unraveling the Internal Magnetic Field Structure of the Earth-directed Interplanetary Coronal Mass Ejections During 1995 – 2015 T. Nieves-Chinchilla et al.
55. Solar sources and geospace consequences of interplanetary magnetic clouds observed during solar cycle 23 N. Gopalswamy et al.
56. The plasma structure of coronal hole solar wind: Origins and evolution J. Borovsky
57. The trailing edges of high‐speed streams at 1 AU J. Borovsky & M. Denton
58. Are There Different Populations of Flux Ropes in the Solar Wind? M. Janvier et al.
59. Properties of Interplanetary Coronal Mass Ejections N. Gopalswamy
60. Major geomagnetic storms (Dst ≤ −100 nT) generated by corotating interaction regions I. Richardson et al.
61. Observations of an interplanetary switch‐on shock driven by a magnetic cloud H. Feng et al.
62. Are all leading shocks driven by magnetic clouds? H. Feng et al.
63. Alfvén wave‐driven ionospheric mass outflow and electron precipitation during storms S. Hatch et al.
64. Magnetic Flux and Helicity of Magnetic Clouds P. Démoulin et al.
65. Coronal Mass Ejections travel time C. Braga et al.
66. Relationships for predicting magnetic cloud-related geomagnetic storm intensity C. Wu & R. Lepping
67. An Alternative Method for Identifying Interplanetary Magnetic Cloud Regions A. Ojeda-Gonzalez et al.