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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Magnetic annealing effect on crystal and magnetic structure of silicon-iron
Magnetic disturbances examined for correlation of surface and satellite magnetic field measurements
Quantum theory of an electron gas with anomalous magnetic moments in intense magnetic fields
Mathematical model for computing magnetic field structure in magnetosphere after magnetic storm
IMP 2 magnetic field measurements in magnetosheath and interplanetary space compared with polar magnetic disturbances
Electron anomalous magnetic moment effect on spontaneous electron-positron pair production in strong magnetic field, noting relationship to expanding universe models
Relativistic electron motion in constant magnetic field noting electron anomalous magnetic moment, nonlinear Lagrangian for electromagnetic field and spontaneous pair production
Charged particle behavior in axisymmetric and multipolar magnetic mirrors, correlating magnetic moment variation and computing motion equations
Effects of strong magnetic fields and of magnetic field free environments on man and animals
Quantum theory of electron gas with anomalous magnetic moments in intense magnetic fields, noting pair creation from thermodynamic energy in system
Homogeneous conducting moon-solar wind interactions, describing time dependent lunar magnetic and electric fields induced by interplanetary magnetic field variations
Transient magnetic fields in plasma trapped in dipolar magnetic field
Lunar rocks magnetic properties and natural remanent magnetization, examining pyroxene paramagnetism, ferrosilite and ilmenite antiferromagnetism and native iron ferromagnetism
Superconductive magnets with different windings and modular construction for magnetic mirror apparatus, discussing performance tests
Polarity comparison of solar magnetic field and interplanetary magnetic field
Tests of permanent magnet and superconducting magnet MPD radiation cooled thrustors
During relatively quiet times in the period 1964-1968, AE is found to be greater when the interplanetary magnetic field (b sub IMF) is directed toward the sun in Jan., Feb., and Apr., and when B sub IMF is directed away from the sun in Oct. to Dec. Using Murmansk hourly H values and the AE components, AU and AL, it is shown that this sector dependence is present only in the negative H deviations. This observation supports the idea that negative bay magnitudes are determined chiefly by particle-produced ionization, while positive bay magnitudes are rather insensitive to increases in particle precipitation. The ratio of DP2-type magnetic activity in the southern polar cap to that in the northern polar cap is found to be greater by a factor of about 1.75 for B sub IMF toward the sun.
The analysis of forty-five years of inferred interplanetary magnetic field polarity shows an annual variation and a variation of about twenty years, associated here with the solar magnetic cycle. On the average the phase of the annual variation of the interplanetary field changes about 2 and 2/3 years after sunspot maximum, i.e. for about ten consecutive years the predominant polarity of the interplanetary field is away from the sun during the six-month interval in which the earth is at southern heliographic latitudes. Then a change of phase occurs so that for about the next ten years the predominant polarity is toward the sun, while the earth is at southern heliographic latitudes. The annual variation changes its predominant polarity within a few days of the times when the heliographic latitude of the earth is zero.