AERODYNAMIC DAMPING OF A 0.02-SCALE SATURN SA-1 MODEL VIBRATING IN THE FIRST FREE-FREE BENDING MODE
Aerodynamic damping of 0.02 scale saturn sa-1 model vibrating in first free-free bending mode
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Aerodynamic damping of 0.02 scale saturn sa-1 model vibrating in first free-free bending mode
Free flight and free oscillation methods for wind tunnel dynamic stability testing
The capture of volatile radioiodine from nuclear fuel reprocessing off-gas streams remains a critical challenge due to the high volatility, long half-life of 129I, and biological uptake of iodide from the environment. Although silver-based sorbents provide strong iodine chemisorption, their high cost and regulatory classification as mixed radioactive-hazardous waste motivate the development of alternative materials. Here, we report a silver-free Cu2O-Ti3C2Tx MXene hybrid for iodine gas capture at 150 °C. Structural and compositional analyses confirm the formation of Cu2O nanoparticles on Ti3C2Tx nanosheets and their subsequent conversion to thermodynamically stable CuI upon static iodine gas exposure, achieving an iodine mass loading of up to 1115 mg/g. These results demonstrate the potential of Cu2O-Ti3C2Tx MXene as a copper-based alternative to silver sorbents for elevated-temperature iodine gas capture.
Dynamic stability of free-free circular cylindrical shell subjected to gimballed variable end thrust
Free-free emission by intergalactic hydrogen calculated for steady state and closed evolving models
Fortran IV computer program for evaluation of natural frequencies and unstable values of thrust frequency for free-free circular cylindrical shell subjected to end thrust
Elastic stability of slender bar with free-free ends under dynamic loading - spacecraft stability
Damping and mass stiffness discontinuity effects on dynamic stability of free-free beam under gimballed pulsating end thrust
Dynamic stability of bending vibrations of uniform free-free beam under end thrust with application to rocket vehicles
Free-free galactic X-ray emission from hot fully- ionized hydrogenic plasma
Prediction of vibration frequencies and modes for free-free truncated conical shells, using Rayleigh-Ritz method
Thin film technique for determination of electron mean free path and free electron density changes in bulk metals under applied strain
Thermal and free-free emission from planetary nebulae based on graphite grain model, discussing IR fluxes
Monte Carlo analysis of free and near free molecular flow through circular tubes for mass, momentum and energy transfer
Free-free opacity of stellar interiors by ion correlations applied to red giant degenerate cores
A relationship between the inverse bremsstrahlung absorption cross section and the electron neutral momentum transfer cross section has been utilized to determine the infrared free-free continuum absorption coefficient for the negative ions of helium, neon, argon, krypton, and xenon. The values of the momentum transfer cross section for this calculation have been obtained from experimental measurements. Analytical expressions for the absorption coefficient have also been developed. From the results of this calculation, it is possible to determine the absorption coefficient per unit electron density per neutral atom for temperatures in the range from 2500 to 25,000 K. The results are compared with those from tabulations of previous calculations and those computed from theoretical values of the phase shifts for the elastic scattering of electrons by neutral atoms.
If G is a grammar such that in each non-context-free rule of G, the right side contains a string of terminals longer than any terminal string appearing between two nonterminals in the left side, then the language generated by G is context free. Six previous results follow as corollaries of this theorem.
The free-free microwave emission is calculated from a series of model magnetic loops. The loops are surrounded by a cooler external plasma, as required by recent simultaneous X ray and microwave observations, and a narrow transition zone separating the loops from the external plasma. To be consistent with the observational results, upper limits on the density and temperature scale lengths in the transition zone are found to be 360 km and 250 km, respectively. The models which best produce agreement with X ray and microwave observations also yielded emission measure curves which agree well with observational emission measure curves for solar active regions.