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adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A
Stability diagrams are calculated for hydromagnetic kink instabilities in a zero‐pressure plasma confined in a stellarator geometry with arbitrary mixtures of l = 2 and l = 3 multipolar helical fields and with various radial distributions of the current parallel to the confining magnetic field The introduction of small pressure gradients increases the size of the unstable regions
·After a brief review of magnetospheric and interplanetary phenomena for intervals with enhanced solar wind magnetosphere interaction an attempt is made to define a geomagnetic storm as an interval of time when a sufficiently intense and long lasting interplanetary convection electric field leads through a substantial energization in the magnetosphere ionosphere
Friedberg Ideal Magnetohydrodynamics Plenum New York 1987 Google Scholar Thompson An Introduction to Plasma Physics Pergamon Oxford 1962 MATH Google Scholar G Schmidt Physics of High Temperature Plasmas Academic New York 1966 Google Scholar Shafranov Plasma Equilibrium in a Magnetic Held in Reviews of Plasma Physics Vol
A hydromagnetic theory is presented which explains the average characteristics of geomagnetic storms The magnetic storm is caused by a sudden increase in the intensity of the solar wind Stresses are then set up in the geomagnetic field by the solar plasma impinging upon the geomagnetic field and becoming trapped in it These stresses which
·Anjali Devi and Prakash [14] examined the hydromagnetic flow over a slandering stretching sheet by taking viscosity and thermal conductivity as functions of temperature Umavathi et al [15
Semantic Scholar extracted view of "Hydrodynamic and Hydromagnetic Stability By S CHANDRASEKHAR Clarendon Press Oxford University Press 1961 652 pp £5 5s " by Louis N Howard
·Semantic Scholar extracted view of "Similarity in the Asymptotic Behavior of Collision Free Hydromagnetic Waves and Water Waves" by C S Gardner et al
The compressional wave in the shock generates transverse hydromagnetic waves that propagate to high latitudes along the magnetic field lines Since the field lines are firmly anchored in the conducting core of the earth a strong shock may cause the field lines to oscillate for a considerable length of time These oscillations are in fact
·Dr Chandrasekhar s book received high praise when it first appeared in 1961 as part of Oxford University Press International Series of Monographs on Physics Since then it has been reprinted numerous times in its expensive hardcover format This first lower priced sturdy paperback edition will be welcomed by graduate physics students and scientists familiar with
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·Semantic Scholar extracted view of "Unsteady Hydromagnetic Natural Convection Flow of a Dusty Fluid Past an Impulsively Moving Vertical Plate With Ramped Temperature in the Presence of Thermal Radiation" by R Nandkeolyar et al
·A separator based on the principle of inertial collisions mainly refers to wave plate mist eliminators which usually consist of two parts specially designed vanes and a flushing system Fig 4 displays all types of vanes used in mist eliminators Generally vanes have one of three structures arc trapezoid and triangle
·Kinematic dynamos For kinematic dynamos the field strength is negligible so the flow can be considered given It must still be a solution to the Navier Stokes equations although this restriction is sometimes given boundary conditions vacuum outside the dynamo domain this constitutes an eigenvalue problem where the largest real
select article Influence of chemical kinetic exponent on transient mixed convective hydromagnetic flow in vertical channel with convective boundary condition Sand settling in a three phase flow inside a horizontal separator Ahmed Basyouny Article 100235 View PDF Article preview
Hydrodynamic and hydromagnetic stability ResearchGate 0 ： 1102 ： S Chandrasekhar ： Not Available ： Fluid dynamics DOI： /
·In addition the development of high magnetic intensity reaching as high as T high gradient magnetic separators has been achieved with which it is feasible to economically separate non ferrous minerals copper molybdenum copper lead copper zinc separation During this period several magnetic separation technologies have been
·Kinematic dynamos For kinematic dynamos the field strength is negligible so the flow can be considered given It must still be a solution to the Navier Stokes equations although this restriction is sometimes given boundary conditions vacuum outside the dynamo domain this constitutes an eigenvalue problem where the largest real
·Recent progress in astrophysical hydromagnetic turbulence is being reviewed The physical ideas behind the now widely accepted Goldreich Sridhar model and its extension to compressible magnetohydrodynamic turbulence are introduced Implications for cosmic ray diffusion and acceleration is being discussed Dynamo generated magnetic fields with and
Journal Pre proof Entropy generation in hydromagnetic nanofluids flow inside a tilted square enclosure under local thermal nonequilibrium conditions
·ProSlide s HydroMAGNETIC technology powers the most advanced water coasters in the world Using Linear Induction Motors LIM rafts are propelled uphill at an accelerated speed thanks to the electromagnetic power generated from the reaction of magnets underneath the fiberglass flume with the metal plates in the rafts This patented technology is
The stability of the hydromagnetic flow of two uniform infinite streams with planar interface exhibiting this type of discontinuity has been analyzed in detail Two necessary and sufficient criteria for its stability have been obtained in contrast to only one that is usually given The stabilizing effect of magnetic field is strongly
Entropy generation in hydromagnetic nanofluids flow inside a tilted square enclosure under local thermal nonequilibrium condition Khamis S Al Kalbani Rahman M Ziad Saghir Article 100031
The first term on the right‐hand side of Eq represents a tension in the field lines; the second term contributes an isotropic magnetic pressure which is about 4 atm for a field strength of 1 TThese interpretations will be useful in the Section on the perfect conductor below It is worth emphasizing that the magnetic field alone contributes to the EM force on the conductor to the EM
Numerical solutions have been obtained for the dispersion relation for hydromagnetic waves in an infinite uniform collisionless plasma Except for the Alfvn shear mode all hydromagnetic waves are strongly damped in plasmas of moderate or high β fluid pressure/magnetic pressure
·In this paper we investigate the influence of temperature dependent fluid properties on the flow and heat transfer characteristics of an electrically conducting dusty fluid over a stretching sheet Temperature dependent fluid properties are assumed to vary as a function of the temperature The governing coupled nonlinear partial differential equations
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