59 citations as recorded by crossref.

1. Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model B. Vršnak et al. 10.1007/s11207-012-0035-4
2. A kinematically distorted flux rope model for magnetic clouds M. Owens et al. 10.1029/2005JA011460
3. Forecasting the Arrival Time of Coronal Mass Ejections: Analysis of the CCMC CME Scoreboard P. Riley et al. 10.1029/2018SW001962
4. Mass-loss Rates from Coronal Mass Ejections: A Predictive Theoretical Model for Solar-type Stars S. Cranmer 10.3847/1538-4357/aa6f0e
5. Eddy viscosity and flow properties of the solar wind: Co-rotating interaction regions, coronal-mass-ejection sheaths, and solar-wind/magnetosphere coupling J. Borovsky 10.1063/1.2200308
6. 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
7. Influence of Convective Effect of Solar Winds on the CME Transit Time S. Lu-yuan 10.1016/j.chinastron.2017.11.004
8. A probabilistic approach to the drag-based model G. Napoletano et al. 10.1051/swsc/2018003
9. Probabilistic Drag-Based Ensemble Model (DBEM) Evaluation for Heliospheric Propagation of CMEs J. Čalogović et al. 10.1007/s11207-021-01859-5
10. Characteristic magnetic field and speed properties of interplanetary coronal mass ejections and their sheath regions M. Owens et al. 10.1029/2004JA010814
11. Evolution of the 12 July 2012 CME from the Sun to the Earth: Data‐constrained three‐dimensional MHD simulations F. Shen et al. 10.1002/2014JA020365
12. EVOLUTION OF CORONAL MASS EJECTION MORPHOLOGY WITH INCREASING HELIOCENTRIC DISTANCE. II. IN SITU OBSERVATIONS N. Savani et al. 10.1088/0004-637X/732/2/117
13. On geomagnetic storms and associated solar activity phenomena observed during 1996–2009 N. Mittal & V. Verma 10.1016/j.actaastro.2015.12.038
14. Pseudo-automatic Determination of Coronal Mass Ejections’ Kinematics in 3D C. Braga et al. 10.3847/1538-4357/aa755f
15. 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
16. Ambient solar wind's effect on ICME transit times A. Case et al. 10.1029/2008GL034493
17. Medium-scale traveling ionospheric disturbances in the Korean region on 10 November 2004: Potential impact on GPS-based navigation systems M. Yoon & J. Lee 10.1002/2013SW001002
18. Prediction of the 1‐AU arrival times of CME‐associated interplanetary shocks: Evaluation of an empirical interplanetary shock propagation model K. Kim et al. 10.1029/2006JA011904
19. Space Physics for Graduate Students: An Activities‐Based Approach N. Gross et al. 10.1029/2009EO020001
20. Arrival time of solar eruptive CMEs associated with ICMEs of magnetic cloud and ejecta A. Shanmugaraju et al. 10.1007/s10509-015-2251-5
21. Three-dimensional reconstruction of coronal mass ejections using heliospheric imager data T. Howard 10.1016/j.jastp.2010.08.009
22. Tracking a Ulysses High-latitude ICME Event Back to Its Solar Origins C. Dumitrache et al. 10.1007/s11207-011-9811-9
23. Influence of Convection Effects of Solar Wind Speed on CME Transit Time L. SUN 10.11728/cjss2016.06.828
24. Application of Ojih-Okeke modified empirical coronal mass ejection arrival (ECA) model in predicting the arrival time of coronal mass ejections (CMEs) V. Ojih & F. Okeke 10.5897/IJPS2017.4645
25. Solar Wind and Heavy Ion Properties of Interplanetary Coronal Mass Ejections M. Owens 10.1007/s11207-018-1343-0
26. Effects of Background Solar Wind and Drag Force on the Propagation of Coronal-mass-ejection-driven Shocks C. Wu et al. 10.3847/1538-4357/ad88ee
27. Origin and Ion Charge State Evolution of Solar Wind Transients during 4 – 7 August 2011 D. Rodkin et al. 10.1007/s11207-017-1109-0
28. Development of Ojih-Okeke modified emperical coronal mass ejection arrival (ECA) model for predicting arrival times of CMEs F. Okeke & V. Ojih 10.1007/s40808-018-0539-5
29. Solar flares, coronal mass ejections and solar energetic particle event characteristics A. Papaioannou et al. 10.1051/swsc/2016035
30. Current status of CME/shock arrival time prediction X. Zhao & M. Dryer 10.1002/2014SW001060
31. The radial speed‐expansion speed relation for Earth‐directed CMEs P. Mäkelä et al. 10.1002/2015SW001335
32. OBSERVATIONAL EVIDENCE OF A CORONAL MASS EJECTION DISTORTION DIRECTLY ATTRIBUTABLE TO A STRUCTURED SOLAR WIND N. Savani et al. 10.1088/2041-8205/714/1/L128
33. Constraints to the drag-based reverse modeling J. Čalogović et al. 10.1051/0004-6361/202346874
34. An Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles V. Grechnev et al. 10.1007/s11207-008-9245-1
35. The Impact of Coronal Mass Ejections on the Seasonal Variation of the Ionospheric Critical Frequency f0F2 H. Farid et al. 10.3390/universe6110200
36. Derivation of fluid conservation relations to infer near‐Sun properties of coronal mass ejections from in situ measurements P. Riley & D. McComas 10.1029/2009JA014436
37. Coronal mass ejections: a driver of severe space weather L. Green & D. Baker 10.1002/wea.2437
38. The Physical Processes of CME/ICME Evolution W. Manchester et al. 10.1007/s11214-017-0394-0
39. Ion Charge States and Potential Geoeffectiveness: The Role of Coronal Spectroscopy for Space‐Weather Forecasting M. Owens et al. 10.1029/2018SW001855
40. 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
41. INFLUENCE OF THE AMBIENT SOLAR WIND FLOW ON THE PROPAGATION BEHAVIOR OF INTERPLANETARY CORONAL MASS EJECTIONS M. Temmer et al. 10.1088/0004-637X/743/2/101
42. Aditya Solar Wind Particle Experiment (ASPEX) on Board Aditya—L1: The Solar Wind Ion Spectrometer (SWIS) P. Kumar et al. 10.1007/s11207-025-02443-x
43. Development of a formalism for computing transits of Earth-directed CMEs, plasma sheaths, and shocks. Towards a forecasting tool P. Corona-Romero & J. Gonzalez-Esparza 10.1016/j.asr.2016.01.009
44. A Bayesian approach to the drag-based modelling of ICMEs S. Chierichini et al. 10.1051/swsc/2023032
45. Causes and Consequences of Magnetic Complexity Changes within Interplanetary Coronal Mass Ejections: A Statistical Study C. Scolini et al. 10.3847/1538-4357/ac3e60
46. Forecasting the Structure and Orientation of Earthbound Coronal Mass Ejections E. Kilpua et al. 10.1029/2018SW001944
47. Dst of the Carrington storm of 1859 G. Siscoe et al. 10.1016/j.asr.2005.02.102
48. 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
49. 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
50. Magnetohydrodynamic Simulation of Multiple Coronal Mass Ejections: An Effect of “Pre-events” C. Wu et al. 10.3847/1538-4357/ac7f2a
51. Calculating travel times and arrival speeds of CMEs to Earth: An analytic tool for space weather forecasting P. Corona‐Romero et al. 10.1002/2016SW001489
52. Predicting the magnetic vectors within coronal mass ejections arriving at Earth: 1. Initial architecture N. Savani et al. 10.1002/2015SW001171
53. HELIOSPHERIC PROPAGATION OF CORONAL MASS EJECTIONS: DRAG-BASED MODEL FITTING T. Žic et al. 10.1088/0067-0049/218/2/32
54. Testing the current paradigm for space weather prediction with heliospheric imagers L. Barnard et al. 10.1002/2017SW001609
55. Reconstructing the 3-D Trajectories of CMEs in the Inner Heliosphere S. Maloney et al. 10.1007/s11207-009-9364-3
56. An operational method for shock arrival time prediction by one‐dimensional CESE‐HD solar wind model X. Feng et al. 10.1029/2009JA014385
57. On the arrival times of halo Coronal Mass Ejections in the vicinity of the Earth N. Mittal & U. Narain 10.1016/j.nrjag.2015.05.001
58. Decadal trends in the diurnal variation of galactic cosmic rays observed using neutron monitor data S. Thomas et al. 10.5194/angeo-35-825-2017
59. The Solar Wind Speed Expansion Factor [${v}$–$f _{\text{s}}$] Relationship at the Inner Boundary (18 $\text{R}_{\odot }$) of the Heliosphere C. Wu et al. 10.1007/s11207-019-1576-6