Transport of solar wind into Earth's magnetosphere through rolled-up Kelvin–Helmholtz vortices

By H. Hasegawa, M. Fujimoto, T. Phan, H. Rème, A. Balogh, M. Dunlop, C. Hashimoto, R. Tandokoro. Nature, 2004

656 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/cd2152b91de488ec2a57da93ea6b1823677bdcbb

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In Astronomy and Astrophysics

1. V. Angelopoulos
2. Xuzhi Zhou
3. T. Van Doorsselaere
4. Giuseppe Nisticò
5. Valery M. Nakariakov
6. Karl-Heinz Glassmeier
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In Molecular Biology

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6. B. Lavraud
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Citations in the corpus

• The Upgraded CARISMA Magnetometer Array in the THEMIS Era (2008, background): “…1999) verses natural waveguide mode harmonic resonances (cf. the simulations of Wright and Rickard 1995), the role of the magnetopause over-reflection mechanism (e.g. Mann et al. 1999), the role of nonlinear KH vortex development (cf. Hasegawa et al. 2004; Fairfield et al. 2007 and many others).”
• Single-spacecraft detection of rolled-up Kelvin-Helmholtz vortices at the flank magnetopause (2006, neutral): “Citation: Hasegawa, H., M. Fujimoto, K. Takagi, Y. Saito, T. Mukai, and H. Rème (2006), Single-spacecraft detection of rolled-up”
• MAGNETIC KELVIN–HELMHOLTZ INSTABILITY AT THE SUN (2011, neutral): “…(panel (c) in Figure 3), which entrain magnetic fields of opposing direction (Nykyri & Otto 2004), allowing reconnection to occur as a secondary process and thus, for the magnetopause, allowing solar wind plasma to gain access to the magnetosphere (Nykyri & Otto 2001; Hasegawa et al. 2004).”
• Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, methodology): “Using the observations of the Cluster satellites, Hasegawa et al. (2004) demonstrated the nonlinear growth of KHI and associated vortices along the duskflank during a time period when the IMF was northward.”
• The interaction of ultra-low-frequency pc3-5 waves with charged particles in Earth’s magnetosphere (2017, background): “H instability produces large-scale vortices that transport solar wind plasma into the magnetosphere (Fairfield et al. 2000; Hasegawa et al. 2004).”
• Altered solar wind-magnetosphere interaction at low Mach numbers: Coronal mass ejections (2008, background): “However, it was later argued [Petrinec et al., 1997] (a) that such observations could result from either reconnection-related processes or high-energy particle leakage and (b) that magnetosheath flow may not exceed the solar wind speed by more than a few percent.”
• The Search-Coil Magnetometer for MMS (2016, background): “…1982; Gendrin 1983; Chaston et al. 2008) and impulsive penetration (Lemaire 1977; Sibeck 1990), Kelvin–Helmholtz instability (Sckopke et al. 1981; Hasegawa et al. 2004; Smets et al. 2007) are physical mechanisms which are still extensively studied (see Phan et al. 2005 for a detailed review).”
• Solar wind driving of magnetospheric ULF waves: Pulsations driven by velocity shear at the magnetopause (2008, background): “…the onset of the KH instability at the magnetopause boundary, which114 is valid for incompressible plasmas separated by a tangential discontinuity [Hasegawa, 1975]:115 (k · v)2 > 1 µomi ( 1 n1 + 1 n2 )[ (k ·B1) 2 + (k ·B2) 2 ] (1) B is the magnetic field,n is the number density,µo the…”