Distortions in the radiation cavity as measured by an 1100-kilometer polar orbiting satellite.
Distortions in spatial distribution of high energy electrons observed by polar orbiting satellite
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Distortions in spatial distribution of high energy electrons observed by polar orbiting satellite
Asymptotic acceptance cone variation of cosmic ray neutron monitors in geomagnetic field distorted by solar wind, noting particle trajectories
Four-terminal network forms a bidirectional valve which will switch or alternate an ac signal without crossover distortion or threshold effect. In this network, an isolated control signal is sufficient for circuit turn-on.
Trapped charged particle motion in geomagnetic field distorted by solar wind
Adiabatic invariant trapped radiation shells and cosmic ray cutoff magnetosphere models distorted by solar wind
Terminal rise velocity of small distorted gas bubbles in liquid of small viscosity
Distorted wave one-meson-exchange /DWOME/ for high-energy elementary particle reaction analysis, leading to different expression for transition amplitude
Magnetosphere shape and distortion of magnetic field within magnetosphere
Adiabatic theory of distorted motion of charged particles in geomagnetic field, showing dependence on equatorial pitch angle
In the design and development of dynamically similar structural models a distorted model of the panel is used. The panel thickness is made larger than that dictated by geometric scaling, and the mass of the panel is decreased by adding mass to the surface of the panel to counteract the additional stiffness obtained by the thickness increase.
Amplifier translates the square pulses generated by a boron-trifluoride neutron sensitive detector located adjacent to a nuclear reactor to slower, long exponential decay pulses. These pulses are transmitted over long coaxial cables with minimum distortion and loss of frequency.
Explorer XII satellite measurements of geomagnetic field distortion by solar wind
Two-dimensional multiple wave distortions effect on heat transfer to wall in hypersonic flow
Magnetospheric distortion during geomagnetic storm on September 30, 1961, examining Explorer XII satellite evidence on ring currents
Dayside distortion of geomagnetic field by solar wind beyond 3.5 earth radii measured and compared with three magnetosphere models
Inelastic differential scattering cross sections and angular distribution of Ni first-excited- state protons determined by distorted wave calculation
Harmonic distortion analyzer effects rapid and accurate setup and calibration of magnetic tape instrumentation recorders. The analyzer is portable, requires no warmup period and need not be calibrated for normal usage. Average setup time with this analyzer is approximately 30 seconds per track.
Modified spectrometer system with a low-noise preamplifier reduces rate-dependent distortions at high counting rates, 25,000 counts per second. Pole-zero cancellation minimizes pulse undershoots due to multiple time constants, baseline restoration improves resolution and prevents spectral shifts.