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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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Single-axis meter design and development for measuring feeble torques on massive bodies, discussing calibration, testing results, evaluation of static dipole moments and spacecraft spin-rate control moments
Literature survey and chemical analyses on effect of lithophilous lichens in weathering of massive crystalline rocks
Structure and pulsational properties of hydrogen poor massive blue stars with helium cores
Thesis on flow field about inviscid massive blowing two dimensional cylinder with fixed contact surface using one strip method of integral relations.
Massive supergiant star models construction for core He plasma burning evolution phase, discussing luminosity and temperature sensitivity to internal instability
Microwave and IR opacities of dry massive model of Venus atmosphere
Venus microwave phase effect analyzed assuming dry massive Venus atmospheric model, discussing heat transfer processes
Structure and pulsational properties of massive stars with helium cores and thin hydrogen poor envelopes
Stagnation point analysis of coupled viscous radiating flow with massive blowing
Models constructed for advanced evolution phases in massive convective red supergiants, considering carbon, Ne and oxygen burning in stellar core
Massive blowing effect on stagnation point radiative energy transfer of ablative heat shield during planetary entry at hypersonic velocities
Massive hydrogen burning stars evolution with pulsational mass loss based on minimizing pulsational instability degree to specify mass loss rate
Massive homogeneous star pulsation stability, determining maximum mass by opacity formula
Maxwell equations and equations of massive-vector- meson fields in spatially homogeneous Bianchi cosmologies, obtaining formula for homogeneous EM field
Diagnosability and recovery from massive faults in digital systems
Numerical analysis of complex boundary layer at axisymmetric stagnation point with massive blowing
Normal O, blue supergiants and brightest yellow and red supergiant massive stars, considering evolution, luminosity, lifetime mass loss, pulsational instability and supernovae