Fluidic decoder and display device
Feasibility and advantages of spacecraft fluidic decoder and display device
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Feasibility and advantages of spacecraft fluidic decoder and display device
Prediction curves for launch vehicle vibration levels in region of spacecraft adaptor
Summary of random vibration prediction procedures for aerospace vehicles, with bibliography
Design and fabrication of oxygen fluoride/diborane thrust chambers
Fluidic systems for control of matrix plasma displays
Flapper valve using a bimorph piezoelectric ceramic bender converts an electrical input into a pneumatic output signal capable of operating fluidic logic elements in a decoder and display system.
Optimum clamp combinations for strap down inertial measuring units with field replaceable sensors
Crosstalk problems and cross grid control, and experimental hardware design for fluidically controlled plasma display devices
Oscillatory grid control, plasma cell matrix design, and control system for fluidically controlled plasma display devices
Fluidic display, discussing applications for fluidic computers and control systems
Fluidic logic elements to control firing and extinction of plasma matrix display system cells with constant electrical power supply
Fluidic logic elements for controlling selected cells extinction in hybrid plasma-fluidic display
Observational errors effects on surface waves resolution, describing shear velocity determination in crust and mantle from observed waves
Experimental techniques for prealigning and clamping inertial measurement sensors without major system recalibration
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Observed line-blocking factors for stars of spectral types B6 to A0 are presented which were measured on spectral tracings observed over the wavelength ranges from 2064 to 2158 A, 2496 to 2590 A, and 2775 to 2867 A with the S 59 spectrometer on the ESRO TD 1A satellite. Twenty-six stars having normal spectra were observed along with 12 stars having abnormal spectra. The results for normal and abnormal stars are compared to determine the changes in line blocking related to each type of spectral peculiarity. Detailed descriptions are given of the line-blocking factors in different spectral channels for a B8 supergiant, three Be stars, a shell star, two eclipsing binaries, an Hg-Mn star, and several peculiar B and A stars.
Ultraviolet spectra of Omicron And, Alpha CrB, Eta Ori A, and Alpha Vir, which were obtained with the S59 spectrometer at a resolution of 1.7 A in three 100-A-wide regions centered at 2110, 2454, and 2825 A, have been studied for the presence or absence of effects due to their binary nature. As may have been anticipated from their orbital and other characteristics, no indication of strong binary interactions were seen in these observations. However, there are certain spectral peculiarities suggesting the possibility of modifications of spectral classifications for some of these objects. A rather unusual spectral behavior in Alpha Vir is also noted. In addition, based primarily on a review of available literature, attention is drawn to a remarkable property of the third component in Eta Ori A.