Development of space-stable thermal-control coatings, 1 May - 30 September 1969
Development of thermal control surface coatings, including zinc orthotitanate
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Development of thermal control surface coatings, including zinc orthotitanate
Thermal stability of protective coatings for large space vehicles
Theoretical models and spectral reflectance measurements of white pigmented, low solar absorptance coatings for spacecraft temperature control
Development and performance of solar wind simulation facility for studying thermal-control coatings
Convolution formulas for Cauchy and standard normal random variable distributions derived from geometry of circular symmetric distribution on plane
Space erectable boom with interlocked seam, perforations and coatings to provide torsional rigidity and thermal stability
Monomer solutions have high solubility and low solution viscosity. Since monomers are shipped in powder form and reaction to polyimide-acid prepolymer is omitted, the cost is low and handling is easy.
Investigating problems of stability and flux jumping in superconducting materials
Polyimide resin and resin reinforced composites
Using zinc orthotitanate-pigmented potassium silicate paints for thermal control surface coatings
Synthesis and thermal properties of fluoroaromatic silicon and carbon polymers for space use
Accelerated longitude drift regimes of eccentric 12 hour orbits due to resonant geopotential
Stability of model tracking adaptive control systems with reduced state feedback and measurement noise
Liapunov functions generation for input-output stability of dynamical systems, using causal operator and state space realization
Stability theory for thermal stratified viscous parallel flows at Prandtl number of unity, considering atmospheric boundary layer and jet stream mechanisms
Plasmaspheric ambient hydrogen and helium atomic cations density measurement by OGO 5 ion mass spectrometer during magnetic storm, noting relationship to auroral red arcs
Apollo 11 and 12 fines cosmogenic He, Ne and Ar radionuclides composition determination, using electron microprobe analysis
Apollo 11 and 12 fines analysis, observing no quarks