Electron precipitation pulsations
Electron precipitation modulation exponential dependence on micropulsation amplitude derived from idealized model
Engineering topics
Publications and source records attributed to Coroniti, F. V..
Electron precipitation modulation exponential dependence on micropulsation amplitude derived from idealized model
Linear fluid equations are used to estimate wave train properties of strong collisionless shocks. Fast shocks exhibit several dispersion changes with increasing Mach number. For perpendicular propagation into a finite-beta plasma, an ion cyclotron radius trailing wave train exists only for (M sub F)2 is smaller than 2. Oblique fast shocks have a leading ion inertia wave train if M sub A is smaller than root of M(+)/M(-) cos theta/2 and a trailing electron inertia train if M sub A is greater than root of M(+)/M(-) cos theta/2. If the downstream sound speed exceeds the flow speed, linear wave theory predicts a trailing ion acoustic structure which probably resides within the magnetic shock. For a turbulent shock model in which an effective electron-ion collision frequency exceeds the lower hybrid frequency, ions decouple from the magnetic field; the shock wave train now trails with electron inertia and electron gyroradius lengths. Comparisons of this turbulent model and observations on the earth's bow shock are made.
Finite Larmor radius interchange and LF drift oscillations due to magnetospheric temperature and density gradient stresses in trapped plasma
Laminar collisionless fast and slow shock wave theory by finite-Larmor-radius hydromagnetic fluid equations
Electron precipitation pulsations and loss of charged particles from the magnetosphere
Alfven wave drift instability predictions by electron plasma sheet and thermal gradient studies
Collisionless magnetospheric plasma turbulent conductivities for weak and strong electric fields parallel to magnetic field
Energetic electron precipitation and geomagnetic micropulsations related to auroral substorms from balloon X ray and ground based data
Temporal, energy and spatial characteristics of energetic auroral zone electron precipitation
Temporal characteristics of geomagnetic micropulsations and related energetic auroral zone electron precipitation as function of local time
Auroral substorm magnetospheric effects, noting energetic electron precipitation and geomagnetic micropulsations
Characteristics of modulated energetic electron precipitation occurring during auroral substorms
Concept of auroral magnetospheric substorm and relation to electron precipitation and micropulsations