Rankine-Hugoniot relations in turbulent shocks
A collisionless shock is often regarded as a discontinuity with a plasma flow across it. Plasma parameters before the shock (upstream) and behind the shock (downstream) are related by the Rankine-Hugoniot relations (RH) which essentially are the mass ...
Michael Gedalin
doaj +1 more source
Magnetohydrodynamic Shocks Revisited: Magnetically Constraining the Upstream Solar Wind Condition
Magnetohydrodynamic (MHD) shocks are commonly found in various space and astrophysical systems. One often encounters the problem that only the magnetic field data are available when studying interplanetary shocks and planetary bow shocks in the solar ...
Daniel Schmid, Yasuhito Narita
doaj +1 more source
Simulations of Electron Acceleration at Collisionless Shocks: The Effects of Surface Fluctuations [PDF]
Energetic electrons are a common feature of interplanetary shocks and planetary bow shocks, and they are invoked as a key component of models of nonthermal radio emission, such as solar radio bursts.
Anderson K. A. +14 more
core +2 more sources
Morphological and kinematical analysis of the planetary nebula Hu 1-2 and its irradiated bow-shocks [PDF]
AbstractWe present narrow-band optical and near-IR images, and high-resolution long-slit spectra of the planetary nebula Hu 1-2 that allow us to make a detailed description of its unusual morphology and internal kinematics. The data also reveal that the ansae of Hu 1-2 probably represent bow-shocks associated to high velocity outflows that are ...
Luis F. Miranda +3 more
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Properties of mass-loading shocks, 2. Magnetohydrodynamics [PDF]
The one-dimensional magnetohydrodynamics of shocked flows subjected to significant mass loading are considered. Recent observations at comets Giacobini-Zinner and Halley suggest that simple nonreacting MHD is an inappropriate description for active ...
Neubauer, F. M. +3 more
core +2 more sources
Efficient Energy Conversion through Vortex Arrays in the Turbulent Magnetosheath
Turbulence is often enhanced when transmitted through a collisionless plasma shock. We investigate how the enhanced turbulent energy in the Earth's magnetosheath effectively dissipates via vortex arrays.
Chuanpeng Hou +7 more
doaj +1 more source
Magnetic Fields Recorded by Chondrules Formed in Nebular Shocks
Recent laboratory efforts (Fu et al., 2014) have constrained the remanent magnetizations of chondrules and the magnetic field strengths at which the chondrules were exposed to as they cooled below their Curie points.
Boley, Aaron C. +3 more
core +1 more source
Unveiling shocks in planetary nebulae [PDF]
The propagation of a shock wave into a medium is expected to heat the material beyond the shock, producing noticeable effects in intensity line ratios such as [O III]/Halpha.
Guerrero, M. A. +6 more
core +1 more source
Unveiling the structure of the planetary nebula M 2-48: Kinematics and physical conditions [PDF]
The kinematics and physical conditions of the bipolar planetary nebula M 2-48 are analysed from high and low dispersion long-slit spectra. Previous CCD narrow-band optical observations have suggested that this nebula is mainly formed by a pair of ...
A. Raga +37 more
core +2 more sources
Impact of solar wind turbulence on a planetary bow shock
Over the past decades, near-Earth spacecraft observations have provided insights into the physics of the bow shock, suggesting that solar wind intrinsic turbulence influences the bow shock dynamics. On the other hand, theoretical studies, based on global numerical simulations, have not yet investigated the global 3D interaction between a turbulent ...
E. Behar +6 more
openaire +4 more sources

