Magnetopause energy and mass transfer: results from a global MHD simulation [PDF]
We use the global MHD model GUMICS-4 to investigate the energy and mass transfer through the magnetopause and towards the closed magnetic field as a response to the interplanetary magnetic field (IMF) clock angle θ=arctan (BY/BZ), IMF magnitude ...
M. Palmroth +2 more
doaj +1 more source
Particle orbits at the magnetopause: Kelvin-Helmholtz induced trapping
The Kelvin-Helmholtz instability (KHI) is a known mechanism for penetration of solar wind matter into the magnetosphere. Using three-dimensional, resistive magnetohydrodynamic simulations, the double mid-latitude reconnection (DMLR) process was shown to ...
Keppens, Rony +2 more
core +1 more source
MeV magnetosheath ions energized at the bow shock [PDF]
A causal relationship between midlatitude magnetosheath energetic ions and bow shock magnetic geometry was previously established for ion energy up to 200 keV e−1 for the May 4, 1998, storm event.
Blake +49 more
core +2 more sources
Asymmetrically Distributed Kelvin‐Helmholtz Instability at Venusian Magnetosphere
Abstract The asymmetric distribution of Kelvin‐Helmholtz (KH) instability at Venusian ionopause is investigated using a multifluid model. Results show that KH instability distributes asymmetrically, preferentially developing in the −E (anti‐parallel to the interplanetary electric field) hemisphere.
Maodong Yan +7 more
wiley +1 more source
A linear perturbation analysis of magnetopause motion in the Newton-Busemann limit [PDF]
The response of the magnetopause surface to time-varying solar wind dynamic pressure is examined. We argue that to a first approximation the magnetopause surface may be considered as analogous to an elastic membrane. Upon displacement from equilibrium
M. P. Freeman +2 more
doaj +1 more source
Reconnection Preferentially Accelerates Light Ions at Ganymede's Magnetopause
Abstract Juno's flyby of Ganymede revealed ion composition in its vicinity with the Jovian Auroral Distributions Experiment–Ion (JADE‐I) instrument. Throughout this flyby, we derive species‐resolved ion density and velocity moments by decomposing the time‐of‐flight data into contributions from individual ion species using species‐dependent fits. At the
T. W. Oberg +7 more
wiley +1 more source
The azimuthal extent of three flux transfer events [PDF]
In early 2006, the Cluster spacecraft crossed the dayside magnetopause twice each orbit with the spacecraft at their largest separation of the entire mission (~10 000 km).
R. C. Fear +5 more
doaj +1 more source
Kinetic-scale magnetic turbulence and finite Larmor radius effects at Mercury
We use a nonstationary generalization of the higher-order structure function technique to investigate statistical properties of the magnetic field fluctuations recorded by MESSENGER spacecraft during its first flyby (01/14/2008) through the near Mercury ...
Alexandrova +89 more
core +1 more source
Asymmetric magnetic reconnection with a flow shear and applications to the magnetopause [PDF]
We perform a theoretical and numerical study of anti-parallel 2D magnetic reconnection with asymmetries in the density and reconnecting magnetic field strength in addition to a bulk flow shear across the reconnection site in the plane of the reconnecting
Cassak, P. A. +5 more
core +3 more sources
Universal Time Influence on Stormtime Magnetosphere Ionosphere Coupling
Abstract The offset between Earth's magnetic and rotational axes introduces a diurnal dependence in the high‐latitude EUV exposure of the northern hemisphere (NH) and southern hemisphere (SH). This variation raises the question: Does the Universal Time (UT) of geomagnetic storm onset impact its geospace consequences?
Kalpesh Ghag +6 more
wiley +1 more source

