28 citations as recorded by crossref.

1. Deflection flows ahead of ICMEs as an indicator of curvature and geoeffectiveness Y. Liu et al. 10.1029/2007JA012996
2. Prospects for the In Situ detection of Comet C/2019 Y4 ATLAS by Solar Orbiter G. Jones et al. 10.3847/2515-5172/ab8fa6
3. The prolonged southward IMF-Bzevent of 2-4 May 1998: Solar, interplanetary causes and geomagnetic consequences S. Bisoi et al. 10.1002/2015JA022185
4. Combining remote and in situ observations of coronal mass ejections to better constrain magnetic cloud reconstruction M. Owens 10.1029/2008JA013589
5. ULF Wave Activity in the Magnetosphere: Resolving Solar Wind Interdependencies to Identify Driving Mechanisms S. Bentley et al. 10.1002/2017JA024740
6. On the origins and timescales of geoeffective IMF M. Lockwood et al. 10.1002/2016SW001375
7. Ways in which ICME sheaths differ from magnetosheaths G. Siscoe & D. Odstrcil 10.1029/2008JA013142
8. MAGNETIC FIELD-LINE LENGTHS IN INTERPLANETARY CORONAL MASS EJECTIONS INFERRED FROM ENERGETIC ELECTRON EVENTS S. Kahler et al. 10.1088/0004-637X/736/2/106
9. Non-radial solar wind flows and IMF Bz during 1973–2003 F. Pereira & T. Girish 10.1016/j.pss.2009.01.001
10. Multi-Spacecraft Study of the 21 January 2005 ICME C. Foullon et al. 10.1007/s11207-007-0355-y
11. Understanding Interplanetary Coronal Mass Ejection Signatures R. Wimmer-Schweingruber et al. 10.1007/s11214-006-9017-x
12. Method for inferring the axis orientation of cylindrical magnetic flux rope based on single-point measurement Z. Rong et al. 10.1029/2012JA018079
13. EVOLUTION OF PILED-UP COMPRESSIONS IN MODELED CORONAL MASS EJECTION SHEATHS AND THE RESULTING SHEATH STRUCTURES I. Das et al. 10.1088/0004-637X/729/2/112
14. Numerical modeling of interplanetary coronal mass ejections and comparison with heliospheric images N. Lugaz & I. Roussev 10.1016/j.jastp.2010.08.016
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. Observations of a comet tail disruption induced by the passage of a CME T. Kuchar et al. 10.1029/2007JA012603
17. Magnetic cloud distortion resulting from propagation through a structured solar wind: Models and observations M. Owens 10.1029/2006JA011903
18. PREDICTING THE ARRIVAL TIME OF CORONAL MASS EJECTIONS WITH THE GRADUATED CYLINDRICAL SHELL AND DRAG FORCE MODEL T. Shi et al. 10.1088/0004-637X/806/2/271
19. Solar origin of heliospheric magnetic field inversions: Evidence for coronal loop opening within pseudostreamers M. Owens et al. 10.1002/jgra.50259
20. A kinematically distorted flux rope model for magnetic clouds M. Owens et al. 10.1029/2005JA011460
21. Advancing in situ modeling of ICMEs: New techniques for new observations T. Mulligan et al. 10.1002/jgra.50101
22. Coronal mass ejections are not coherent magnetohydrodynamic structures M. Owens et al. 10.1038/s41598-017-04546-3
23. Direct Detection of Solar Angular Momentum Loss with the Wind Spacecraft A. Finley et al. 10.3847/2041-8213/ab4ff4
24. (Non)radial Solar Wind Propagation through the Heliosphere Z. Němeček et al. 10.3847/2041-8213/ab9ff7
25. Thermospheric nitric oxide response to shock‐led storms D. Knipp et al. 10.1002/2016SW001567
26. A Computationally Efficient, Time-Dependent Model of the Solar Wind for Use as a Surrogate to Three-Dimensional Numerical Magnetohydrodynamic Simulations M. Owens et al. 10.1007/s11207-020-01605-3
27. LEARNING FROM THE OUTER HELIOSPHERE: INTERPLANETARY CORONAL MASS EJECTION SHEATH FLOWS AND THE EJECTA ORIENTATION IN THE LOWER CORONA R. Evans et al. 10.1088/0004-637X/728/1/41
28. Lightning as a space-weather hazard: UK thunderstorm activity modulated by the passage of the heliospheric current sheet M. Owens et al. 10.1002/2015GL066802