Carbon isotope fractionation in the Fischer-Tropsch synthesis and in meteorites
Carbon isotope fractionation in Fischer-Tropsch synthesis and in meteorites
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Carbon isotope fractionation in Fischer-Tropsch synthesis and in meteorites
Turtle bladders isolated mucosal and serosal fractions histological and physiological properties, discussing ion transport and oxygen consumption
Oxygen isotope fractionation and formation temperature of minerals from Apollo 11 rocks, including plagioclase-clinopyroxene-magnetite concordancy diagram
Fixed-ratio performance patterns of pigeon key- peck responses to fractional punishments by electric shock
Electron radiation damaged Si, investigating p type defect concentration effect on isochronal temperature in annealing by fractionation experiment
Oxygen isotopic compositions and fractionations between coexisting minerals found in lunar samples from Apollo 11 and Apollo 12 flights
Design optimization for fractional factorial experiments by finite decision problem based on prior information
Engineering design of high fuel fraction diode for in-pile testing and evaluation of components under typical thermal stress conditions
Carbon kinetic isotope fractionation into carbon dioxide and organic compounds in meteorite-like Fischer-Tropsch reaction with nickel-iron or magnetite catalyst
Chemical fractionations in meteorites, considering trace elements abundance in L chondrites and implications for cosmothermometry
Oxygen isotope fractionation in Apollo 12 rocks and soils, noting plagioclase ilmenite isotopic temperature
Ejection fraction relation to left ventricular dimensional changes in patients with heart disease, using angiocardiograms
Sixteen monkeys trained to perform continuous and discrete-avoidance and fixed-ratio tasks with visual and auditory cues were performance-tested before, during, and after 10-day gamma-ray exposures totaling 0, 500, 750, and 1000 rads. Approximately 14 months after the performance-test exposures, surviving animals were exposed to 100-rad gamma-ray fractions at 56-day intervals to observe injury and recovery patterns of blood-forming tissues. The fixed-ratio, food-reward task performance showed a transient decline in all dose groups within 24 hours of the start of gamma-ray exposure, followed by recovery to normal food-consumption levels within 48 to 72 hours. Avoidance tasks were performed successfully by all groups during the 10-day exposure, but reaction times of the two higher dose-rate groups in which animals received 3 and 4 rads per hour or total doses of 750 and 1000 rads, respectively, were somewhat slower.
Experiments have been conducted on several Apollo 12 and 14 samples that confirm the identification of CH4 and C2H6 in lunar fines and breccias. In particular, data for various size fractions of sample 14240,5 are reported which show that the concentrations of these species are dependent on particle size. Results strongly support proposals that solar wind activity is a source of CH4 in lunar samples.
A prototypical, high fuel volume fraction, thermionic emitter body was designed and tested. The emitter body is all tungsten, with a 1.40-cm ID, a 3.23-cm OD, and eight full-length axial fins. The emitter thickness is 0.15 cm while the fins and outer clad are 0.075 cm thick. Different methods of fabrication were used in making the test samples. Stress analysis was performed with a three-dimensional elastic code. Thermal testing of the samples, duplicating calculated radial temperature gradients, heatup and cooldown rates, and emitter body temperatures in operation, was performed with no structural failures noted (six heatup and cooldown cycles per sample). Further emitter analysis and testing is planned.
An algorithm and computer program are presented for generating all the distinct 2(p-q) fractional factorial designs. Some applications of this algorithm to the construction of tables of designs and of designs for nonstandard situations and its use in Bayesian design are discussed. An appendix includes a discussion of an actual experiment whose design was facilitated by the algorithm.
Review of the results of inert gas measurements performed on six grain-size fractions and two single particles from four samples of Luna 20 material. Presented and discussed data include the inert gas contents, element and isotope systematics, radiation ages, and Ar-36/Ar-40 systematics.
The coefficients in the partial fraction expansion considered are given by Heaviside's formula. The evaluation of the coefficients involves the differential of a quotient of two polynomials. A simplified approach for the evaluation of the coefficients is discussed. Leibniz rule is applied and a recurrence formula is derived. A coefficient can also be determined from a system of simultaneous equations. Practical methods for the performance of the computational operations involved in both approaches are considered.