Add to ORKGRayleigh-Taylor instability Barium clouds". r " 20. ABSTRACT (Conttnue on rev ide it nec s ary ad Identify by block mbaor /"-- this repot,VeStdY the stability of high velocity ion clouds in the ionosphere-magnetosphere. We derive the instability growth rate; show that the growth is very fast; and present our conclu-sions DD I JOARM73 1473 EDITION Of I NOV 65 IS OBSOLETE r j. SIN 01 02.LF.01 4-660
International audienceMagnetic reconnexion and Kelvin-Helmholtz (KH) instability are usually recogni...
250-253The role of Kelvin-Helmholtz (K-H) instability in ionospheric phenomena under the electrostat...
The modeling of ionospheric plasma density irregularities (ΔN/N) is a necessary first step towards ...
Three aspects of barium ion cloud dynamics are discussed. First, the effect of the ratio of ion clou...
Abstract The linear growth rates of the Rayleigh-Taylor (R-T) instability in the ionosphere from 201...
Seasonal and zonal climatologies of Rayleigh–Taylor growth rates under geomagnetically quiet conditi...
An active experiment has been conducted in space that allows a test for the theory of nonlinear deve...
High Velocity Clouds are baryonic gas clouds scattered throughout the galactic halo, whose velocitie...
The joint NASA-Max Planck Institute Barium Ion Cloud (BIC) Experiment on September 21, 1971 involved...
textA substorm is a frequently occurring ordered sequence of global energetic events in the magneto...
The ionospheric feedback instability (IFI) has been considered one of the main generation mechanisms...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
The heliosphere is the bubble formed by the solar wind as it interacts with the interstellar medium ...
A weakly ionized plasma with gradients in the ionization density under the influence of the crossed ...
The morphology of the ion cloud in the radial shaped charge barium injection was studied. The shape ...
International audienceMagnetic reconnexion and Kelvin-Helmholtz (KH) instability are usually recogni...
250-253The role of Kelvin-Helmholtz (K-H) instability in ionospheric phenomena under the electrostat...
The modeling of ionospheric plasma density irregularities (ΔN/N) is a necessary first step towards ...
Three aspects of barium ion cloud dynamics are discussed. First, the effect of the ratio of ion clou...
Abstract The linear growth rates of the Rayleigh-Taylor (R-T) instability in the ionosphere from 201...
Seasonal and zonal climatologies of Rayleigh–Taylor growth rates under geomagnetically quiet conditi...
An active experiment has been conducted in space that allows a test for the theory of nonlinear deve...
High Velocity Clouds are baryonic gas clouds scattered throughout the galactic halo, whose velocitie...
The joint NASA-Max Planck Institute Barium Ion Cloud (BIC) Experiment on September 21, 1971 involved...
textA substorm is a frequently occurring ordered sequence of global energetic events in the magneto...
The ionospheric feedback instability (IFI) has been considered one of the main generation mechanisms...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
The heliosphere is the bubble formed by the solar wind as it interacts with the interstellar medium ...
A weakly ionized plasma with gradients in the ionization density under the influence of the crossed ...
The morphology of the ion cloud in the radial shaped charge barium injection was studied. The shape ...
International audienceMagnetic reconnexion and Kelvin-Helmholtz (KH) instability are usually recogni...
250-253The role of Kelvin-Helmholtz (K-H) instability in ionospheric phenomena under the electrostat...
The modeling of ionospheric plasma density irregularities (ΔN/N) is a necessary first step towards ...
