Effects of modeled ionospheric conductance and electron loss on self‐consistent ring current simulations during the 5–7 April 2010 storm
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Reiterative method for determining boundary shape between plasma and magnetic field
Free-space einstein equations for concentrations of radiation held together by gravitational attraction, investigating gravity wave perturbations on background metric
Problem of collisionless, fully ionized single component plasma treated by means of Green function
Harmonic models and Doppler data used to analyze orbital perturbation of Lunar Orbiter
Hartree-Fock single determinant wavefunction calculated numerically for normal state of hydrogen molecule
Residuals from earth based coherent two way radio Doppler data from Lunar Orbiter three orders of magnitude larger than observations from spacecraft
Examination of Liwshitz-Singer model for comparison with Lyman alpha rocket spectrograph
Free electron model for electron work functions and number density distributions and surface potentials in metals
Electric fields and electron work functions, surface potentials and number density distributions in selected metals surfaces determined using free electron model
Residuals from earth based coherent two way radio Doppler data from Lunar Orbiter three orders of magnitude larger than observations from spacecraft
Ionized gas galactic cluster stabilization model construction, considering ionizing radiation enhanced cosmic flux and quasar PKS 1116 plus 12 absorption spectrum
Gas bubble in liquid under surface tension, weightlessness and rotation, determining angular velocity for fluid system disintegration
The solar wind is assumed to be a sufficient source for the radiation belts of Jupiter, with radial diffusion as the process for getting the solar wind fluxes into the inner regions of the radiation belts. The process of a radial diffusion source is combined with pitch-angle diffusion losses to estimate an upper limit to the proton and electron fluxes. The upper limit to the integral proton and electron fluxes in the outer zone scale as L to the -6th power throughout the outer zone, assuming that the magnetic moment is conserved. It is important that these fluxes are above the stably trapped flux levels in the outer regions of the belts; the instability will work because the energies of the particles are above the critical value required.
The vacuum transient response of the moon to a time-varying spatially uniform magnetic field is determined for a lunar electrical conductivity model that was based on the harmonic analysis of Apollo 12 and Explorer 35 dayside magnetometer data. The transient response of the model is found to provide a plausible explanation of the behavior of the local vertical-surface magnetic field for an Apollo 12 magnetometer darkside transient event. A model containing a conducting core and a highly conducting thin subsurface layer is presented, and its transient behavior is discussed.
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