45 citations as recorded by crossref.

1. On the possible formation of Alfvén wings at Mercury during encounters with coronal mass ejections M. Sarantos & J. Slavin 10.1029/2008GL036747
2. THE DYNAMICS OF STELLAR CORONAE HARBORING HOT JUPITERS. II. A SPACE WEATHER EVENT ON A HOT JUPITER O. Cohen et al. 10.1088/0004-637X/738/2/166
3. Solar wind‐magnetosphere coupling efficiency during ejecta and sheath‐driven geomagnetic storms M. Myllys et al. 10.1002/2016JA022407
4. Magnetohydrodynamic Perspective on the Disappearance of Mercury’s Bow Shock by Helios Data Exploration S. Lai et al. 10.3847/1538-4357/ad0a8a
5. Earth’s magnetosphere and outer radiation belt under sub-Alfvénic solar wind N. Lugaz et al. 10.1038/ncomms13001
6. Magnetosheath control of solar wind‐magnetosphere coupling efficiency T. Pulkkinen et al. 10.1002/2016JA023011
7. Alfvén wings in the lunar wake: The role of pressure gradients H. Zhang et al. 10.1002/2016JA022360
8. Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals D. Sibeck et al. 10.1007/s11214-018-0504-7
9. Saturation of transpolar potential for large Y component interplanetary magnetic field E. Mitchell et al. 10.1029/2009JA015119
10. Impact of Changing Stellar and Planetary Magnetic Fields on (Exo)planetary Environments and Atmospheric Mass Loss S. Gupta et al. 10.3847/1538-4357/acd93b
11. The Cross‐Polar Cap Saturation in GUMICS‐4 During High Solar Wind Driving A. Lakka et al. 10.1002/2017JA025054
12. A statistical study of BRIs (SMCs), isolated substorms, and individual sawtooth injections A. DeJong et al. 10.1029/2008JA013870
13. The Relative Importance of Geoeffective Length Versus Alfvén Wing Formation in the Saturation of the Ionospheric Reverse Convection Potential F. Wilder et al. 10.1029/2018GL080639
14. Does the polar cap area saturate? V. Merkin & C. Goodrich 10.1029/2007GL029357
15. Incorporating Inner Magnetosphere Current-driven Electron Acceleration in Numerical Simulations of Exoplanet Radio Emission A. Sciola et al. 10.3847/1538-4357/abefd9
16. Simulated ring current response during periods of dawn‐dusk oriented interplanetary magnetic field (By) E. Mitchell et al. 10.1002/jgra.50269
17. Interplay of solar wind parameters and physical mechanisms producing the saturation of the cross polar cap potential M. Myllys et al. 10.1002/2017GL072676
18. Aspects of global coherence of magnetospheric behavior G. Siscoe 10.1016/j.jastp.2010.11.005
19. MAGNETOSPHERIC STRUCTURE AND ATMOSPHERIC JOULE HEATING OF HABITABLE PLANETS ORBITING M-DWARF STARS O. Cohen et al. 10.1088/0004-637X/790/1/57
20. Understanding the Mechanisms of Radiation Belt Dropouts Observed by Van Allen Probes Z. Xiang et al. 10.1002/2017JA024487
21. Polar cap potential saturation, dayside reconnection, and changes to the magnetosphere J. Borovsky et al. 10.1029/2009JA014058
22. Contribution from the Earth's Bow Shock to Region 1 Current under Low Alfvén Mach Numbers P. Zhong & H. You-Qiu 10.1088/0256-307X/26/4/049401
23. Dynamics of Cosmic-Ray Cutoff Rigidity and Magnetospheric Parameters during Different Phases of the Storm of November 20, 2003 N. Ptitsyna et al. 10.1134/S0016793221010114
24. Magnetohydrodynamic modelling of star–planet interaction and associated auroral radio emission S. Turnpenney et al. 10.1093/mnras/staa824
25. Altered solar wind‐magnetosphere interaction at low Mach numbers: Coronal mass ejections B. Lavraud & J. Borovsky 10.1029/2008JA013192
26. 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
27. Stellar winds and planetary bodies simulations: Magnetized obstacles in super-Alfvénic and sub-Alfvénic flows Y. Vernisse et al. 10.1016/j.pss.2016.08.012
28. SuperDARN cross polar cap potential dependence on the solar wind conditions and comparisons with models D. Mori & A. Koustov 10.1016/j.asr.2013.06.019
29. Mercury's three‐dimensional asymmetric magnetopause J. Zhong et al. 10.1002/2015JA021425
30. The role of the bow shock in solar wind-magnetosphere coupling R. Lopez et al. 10.5194/angeo-29-1129-2011
31. Reconstructing Solar Wind Profiles Associated With Extreme Magnetic Storms: A Machine Learning Approach R. Kataoka & S. Nakano 10.1029/2021GL096275
32. The role of magnetic flux tube deformation and magnetosheath plasma beta in the saturation of the Region 1 field‐aligned current system F. Wilder et al. 10.1002/2014JA020533
33. Investigation of a rare event where the polar ionospheric reverse convection potential does not saturate during a period of extreme northward IMF solar wind driving C. Clauer et al. 10.1002/2016JA022557
34. GUMICS-4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds A. Lakka et al. 10.5194/angeo-37-561-2019
35. Steady State Characteristics of the Terrestrial Geopauses H. Trung et al. 10.1029/2019JA026636
36. Validation of the Space Weather Modeling Framework using observations from CHAMP and DMSP H. Wang et al. 10.1029/2007SW000355
37. Validation of SWMF magnetic field and plasma D. Welling & A. Ridley 10.1029/2009SW000494
38. The solar wind electric field does not control the dayside reconnection rate J. Borovsky & J. Birn 10.1002/2013JA019193
39. The nonlinear response of the polar cap potential under southward IMF: A statistical view F. Wilder et al. 10.1029/2011JA016924
40. The CRONOS Code for Astrophysical Magnetohydrodynamics R. Kissmann et al. 10.3847/1538-4365/aabe75
41. Saturation of the polar cap potential: Inference from Alfvén wing arguments M. Kivelson & A. Ridley 10.1029/2007JA012302
42. Reverse convection potential saturation during northward IMF under various driving conditions F. Wilder et al. 10.1029/2009JA014266
43. Validation of the space weather modeling framework using ground‐based magnetometers Y. Yu & A. Ridley 10.1029/2007SW000345
44. Predicted dependence of the cross polar cap potential saturation on the type of solar wind stream N. Nikolaeva et al. 10.1016/j.asr.2015.06.029
45. 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