Changes in adrenal corticosterone concentration in rats - Method of bio-assay for ACTH.
Adrenal corticosterone concentration changes in response to various doses of ACTH and time pattern of changes in hypophysectomized rats
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Adrenal corticosterone concentration changes in response to various doses of ACTH and time pattern of changes in hypophysectomized rats
Aspect system on Pioneer VI and VII INCORPORATES digital computer for accurate time sector division of spin stabilized vehicle
Modified quasi-linearization method for numerically solving trajectory optimization problems with undetermined terminal time
Stability of feedback systems with monotone and odd monotone nonlinearities
Solar proton event /February 1965/, time history of low energy protons was more complex than that of higher energy particles
Interstellar gas and magnetic field periodic system stability noting free-fall time
Consolidation and retroactive interference in short-term recognition memory for pitch
Time-dependent changes in metabolism, mass, composition, and total heat production of brown adipose tissue in cold-exposed rats
Exponential decay and independence from irrelevant associations in short-term recognition memory for digits presented in serial order
Fixed-interval behavior maintained by conditioned reinforcement in pigeon
Response latency in visual pattern perception situation
Recency judgments in short-term visual memory task
On length difficulty relation in performance of tracking task
Resistance to bacterial pneumonia and influenza infection in space cabin environment tested on mice in simulation chamber
Manned space stations for future space exploration, discussing earth-like environment, artificial gravity, human factors and time dependence
AC power meters using electronic multiplier for overcoming limitations concerning frequency ranges, response times, power factor and distortion
Crack wave loading, investigating dynamic stress intensity factor and time response with photoelastic technique
A simple model of solar flare radiation event particle transport is developed to permit the calculation of fluxes and related quantities as a function of distance from the sun (R). This model assumes the particles spiral around the solar magnetic field lines with a constant pitch angle. The particle angular distributions and onset plus arrival times as functions of energy at 1 AU agree with observations if the pitch angle distribution peaks near 90 deg. As a consequence the time dependence factor is essentially proportional to R/1.7, (R in AU), and the event flux is proportional to R/2.