Free vibration of a centrally clamped spinning circular disk
Centrally clamped spinning circular disk free transverse vibration analysis within accuracy of numerical computations
Dodson, R. O., Jr.↗
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Results for “Disks”
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Models of partially relaxed stellar disks
Models of partially relaxed stellar disks in galaxies, discussing gravitational instability and stellar velocities
Shu, F. H.↗
Group velocity of spiral waves in galactic disks
Group velocity of spiral density waves propagating in disk galaxies implying self destruction, discussing possible replenishment sources
Toomre, A.↗
Wavelength dependence of polarization. XX - The integrated disk of the moon
Integrated lunar disk wavelength dependence of polarization using photoelectric polarimeter, tabulating results
Coyne, G. V.↗
Stellar hydrodynamic equations for a thin disk galaxy
Stellar hydrodynamic equations for thin disk galaxy derived from collisionless Boltzmann equation moments
Hunter, C.↗
Sudden disappearance of a large quiescent prominence on the solar disk, April 28, 1967
Sudden disappearance of large quiescent prominence on solar disk with subsequent brightenings, using photospheric and gravitational model
Mccabe, M.↗
A precession in a disk dynamo model of the earth's dipole field
Earth dipole field disk dynamo model, studying connection between polarity intervals and precession effects
Suffolk, G. C. J.↗
Simplified analysis of a trifragment rotor disk interaction with a containment ring
Computerized analysis of shear failure at initial fragment collision during trifragment rotor disk interaction with containment rings
Mccallum, R. B.↗
Cooling airflow through a stationary turbine disk and blade
Measurement of cooling air pressure changes through stationary turbine disk and airflow distribution within a blade at room temperature and pressures from 28 to 100 psia
Cochran, R. P.↗
Flight tests of cross, modified ringsail, and disk-gap-band parachutes from a deployment altitude of 3.05 km /10,000 ft/
Flight tests of cross, modified ringsail, and disk-gap-band parachute deployment performance from low altitudes with structural load data
Eckstrom, C. V.↗
Elastohydrodynamic film thickness between rolling disks with a synthetic paraffinic oil to 589 K /600 F/
Elastohydrodynamic film thickness between rolling disks with synthetic paraffinic oil at temperatures from 339 to 589 K
Kannel, J. W.↗
High-Altitude Flight Test of a Reefed 12.2-Meter-Diameter Disk-Gap-Band Parachute with Deployment at a Mach Number of 2.58
High altitude flight test of reefed 12.2-meter-diameter disk-gap-band parachute with deployment at 2.58 Mach number
Preisser, J. S.↗
Color changes and absorption-line variations over the inner disk of M31 and the central regions of M32 and NGC 4472
Color changes and absorption line variations in M31, M32 and NGC 4472, attempting synthesis of M31 disk population
Gunn, J. E.↗
Turbulent boundary layer on a rotating disk calculated with an effective viscosity
Skewed turbulent boundary layer and incompressible laminar flow on rotating disk, considering effective viscosity relations and applications domain
Cooper, P.↗
Engineering applications of current and potential distributions in disk electrode systems
Integral transform methods for analytic solutions to current and potential distribution on disk in infinite plane for four limiting cases
Kesselman, W.↗
Mach disk in underexpanded exhaust plumes
Mach disk in underexpanded exhaust plume predicted by dividing flow field into subregions
Abbett, M.↗
Laminar flow between two infinite disks, one rotating and the other stationary
Constant property fluid laminar flow between rotating and stationary infinite disks for limiting Reynolds numbers based on gap width
Reshotko, E.↗
The 1969 opposition effect of Mars - Full disk, Syrtis Major and Arabia
Mars 1969 opposition effects, describing Syrtis Major, Arabia and disk brightness, color and spectrum
Jackel, L.↗