Ring current effects on trapped particles.
Ring current-induced variations in geomagnetically trapped particle fluxes
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Ring current-induced variations in geomagnetically trapped particle fluxes
Growth and decay of ring current and polar electrojet, using magnetic storm examples
Current sheet approximation of effect of ring current on distribution of unbound particles in magnetosphere
Performance of miniature slip rings in high-vacuum conditions
Geometrical parameters, loading, and condition of momentlessness of radial guy net in hanging roof with momentless contour ring
Finite element modeling of circular ring using half and quarter symmetry
Field model equations for calculating higher order ring currents and particle energy storage in magnetosphere
Buckling equations used to determine structural efficiency of ring stiffened corrugated cylinders in axial compression
Ring laser inertial sensor for aerospace systems obtaining high accuracy angular resolution and mechanical simplicity
Damping coefficients for rigid and flexible ring baffles for slosh suppression
Nonlinear flexural vibrations of rings studied without assuming zero midplane strain
Charged particles of extraterrestrial ring current during geomagnetic storms, with Ogo 3 measurements of proton and electron differential energy spectrums
Elastic buckling loads of shallow spherical shells supported by edge rings including nonlinear prebuckling effects
The present report presents as a supplement to the fourth report (available as ATI 5045, Air Materiel Command) in the series of investigations concerning the flow about ring-shaped cowlings further wind-tunnel measurements on inlet devices which are to show the influence of the radius of the nose of the cowling on the flow conditions. Moreover, a simple rule for the design of such arrangements, containing a hub in the interior, is suggested.
We discuss an extended feature in the Perseus molecular cloud complex, most prominent in the IRAS database as an almost complete ring of radius 0.75 degrees, but also clearly seen in optical surveys and in radio continuum emission.
The satellites of Saturn were observed with the 60-inch telescope at Palomar Mountain during the Saturn Ring Plane Crossing (RPX) on August 9-12, 1995. Observations were obtained with a 1024 square CCD and a methane filter to reduce light from Saturn.
High frequency (22 GHz) data have been used two resolve two compact components of the strong gravitational lens PKS 1830-211. The two bright components are at opposite sides of a one arcsecond diameter Einstein ring.
We present the first observations of the Jovian ring system viewed at near-infrared wavelengths in forward-scattered light.