27 citations as recorded by crossref.

1. Maximum Aligned Directional Derivative (MADD) Technique for Planar Structure Analysis in Space Y. Liu et al. 10.3847/1538-4365/ad077c
2. Three-dimensional magnetohydrodynamic description of the process of impingement of a solar wind rotational discontinuity on the Earth’s bow shock E. Pushkar 10.1134/S0015462811020141
3. Geomagnetic and Ionospheric Responses to the Interplanetary Shock Wave of March 17, 2015 V. Pilipenko et al. 10.1134/S1069351318050129
4. On one mechanism for the generation of a reverse solar wind shock in the magnetosheath in front of the Earth’s magnetosphere S. Grib 10.1134/S106377371112005X
5. Magnetic Discontinuities in the Inner Heliosphere: Do Intermediate Shocks Exist? Y. Liu et al. 10.3847/1538-4357/ace04c
6. Impact of the interplanetary magnetic field on thewave flow pattern in the neighborhood of the Earth’s bow shock under sharp variations in the solar wind dynamic pressure D. Donskoi & E. Pushkar 10.1134/S0015462816030133
7. Interplanetary shock–bow shock interaction: Comparison of a global MHD model and observation O. Goncharov et al. 10.1016/j.pss.2014.12.001
8. The classical Rankine-Hugoniot jump conditions, an important cornerstone of modern shock wave physics: ideal assumptions vs. reality P. Krehl 10.1140/epjh/e2015-50010-4
9. On the RH relations across weak and strong shocks in van der Waals gases R. Anand 10.1080/03091929.2017.1357716
10. Exact solutions of magnetohydrodynamics for describing different structural disturbances in solar wind S. Grib & S. Leora 10.1134/S0016793216020079
11. Collision of an interplanetary shock wave with the Earth’s bow shock. Hydrodynamic parameters and magnetic field A. Korolev & E. Pushkar 10.1134/S001546281402015X
12. Understanding the response of the ionosphere-magnetosphere system to sudden solar wind density increases Y. Yu & A. Ridley 10.1029/2010JA015871
13. Collisionless Plasma Processes at Magnetospheric Boundaries: Role of Strong Nonlinear Wave Interactions S. Savin et al. 10.1134/S0021364019170028
14. An empirical model of the Earth’s bow shock based on an artificial neural network G. Pallocchia & L. Trenchi 10.1016/j.pss.2021.105196
15. Acceleration of an interplanetary shock through the magnetosheath: a global hybrid simulation C. Moissard et al. 10.3389/fspas.2024.1330397
16. Geoeffectiveness of interplanetary shocks controlled by impact angles: A review D. Oliveira & A. Samsonov 10.1016/j.asr.2017.10.006
17. Observation of discontinuities accompanied by interplanetary shock within the Martian magnetosheath L. He & J. Guo 10.1051/0004-6361/202451322
18. MHD simulation of the distribution of the gasdynamic parameters and magnetic field behind the Earth’s bow shock under sharp variations in the solar wind dynamic pressure D. Donskoi & E. Pushkar 10.1134/S0015462817030127
19. Features in the Behavior of the Solar Wind behind the Bow Shock Front near the Boundary of the Earth’s Magnetosphere S. Grib & S. Leora 10.1134/S0016793217080102
20. Characteristics of Interplanetary Discontinuities in the Inner Heliosphere Revealed by Parker Solar Probe Y. Liu et al. 10.3847/1538-4357/ac06a1
21. Multispacecraft observations of the terrestrial bow shock and magnetopause during extreme solar wind disturbances M. Tátrallyay et al. 10.5194/angeo-30-1675-2012
22. PRESSURE PULSES AT VOYAGER 2: DRIVERS OF INTERSTELLAR TRANSIENTS? J. Richardson et al. 10.3847/1538-4357/834/2/190
23. Collision of a solar wind shock wave with the Earth’s bow shock. Wave flow pattern E. Pushkar & A. Korolev 10.1134/S0081543813040160
24. Global frequency distributions of pulsations driven by sharp decrease of solar wind dynamic pressure Z. Wang 10.1007/s11430-015-5168-5
25. Propagation of a sudden impulse through the magnetosphere initiating magnetospheric Pc5 pulsations A. Samsonov et al. 10.1029/2011JA016706
26. PROPAGATION OF THE 2012 MARCH CORONAL MASS EJECTIONS FROM THE SUN TO HELIOPAUSE Y. Liu et al. 10.1088/2041-8205/788/2/L28
27. Magnetic Discontinuities in the Solar Wind and Magnetosheath: Magnetospheric Multiscale Mission (MMS) Observations Y. Liu et al. 10.3847/1538-4357/ac62d2