Establishment of spacecraft magnetic criteria and design restraints
Spacecraft magnetic field criteria and design restraints
SPACECRAFT DESIGN↗
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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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Mariner-Mars magnetic mapping tests
Mapping of permanent, and induced magnetic fields of Mariner Mars spacecraft
MARINER SPACE PROBE↗
Preliminary observations of the enhancement of superconducting current-carrying capacity in niobium through hydrogen treatment
Superconducting current carrying capacity of hydrogen treated niobium
MAGNETIC FIELD INTENSITY↗
Transition region magnetic field and polar magnetic disturbances.
Transition region magnetic field and polar magnetic disturbances, comparing Explorer XII DATA with ground measurements from Arctic observatories
POLAR REGION↗
Superconductivity of a composite of fine niobium wires in copper.
Superconductivity of composite of fine niobium wire in copper, measuring critical temperature, transverse magnetic field, current density, etc
NIOBIUM COMPOUND↗
Beam-plasma interactions
Wavelength, frequency, and growth rate dependence on density, stream velocity, and magnetic field strength
STREAM FUNCTION↗
Exact semiclassical theory for galvanomagnetic effects in metals
Closed form solution for conductivity tensor for magnetic field strength obtained from linearized Boltzmann equation for electron conduction distribution function
TENSOR FIELD↗
Magnetic flux flow and superconductor stabilization Quarterly report, Apr. 1 - Jun. 30, 1967
Magnetic flux flow and superconductor stabilization
SUPERCONDUCTOR↗
Some viscous flows of a saturated ferrofluid under the combined influence of thermal and magnetic field gradients.
Temperature and magnetic field gradient effects on magnetothermomechanical interaction of viscous incompressible ferrofluid with cold wall
VISCOUS FLOW↗
The motion of magnetic field lines.
Motion of magnetic lines of force including analysis of fluids with finite high conductivity
PARTICLE MOTION↗
A new effect in the low magnetic field ultrasonic attenuation of impure superconducting niobium.
Changes in ultrasonic attenuation of superconducting niobium at low magnetic fields, considering effects of low critical field impurity phases
IMPURITY↗
Two-phonon absorption in ultrasonic paramagnetic resonance of uranium-doped calcium fluoride.
Two-phonon absorption in ultrasonic paramagnetic resonance of uranium-doped calcium fluoride, relating wave attenuation to ultrasonic intensity and magnetic field angular variation
WAVE ATTENUATION↗
The attainment of zero magnetic field in a superconducting lead shell.
Zero magnetic field in superconducting lead shell using Meissner effect
METAL SHELL↗
Radiation temperature and enhanced diffusion in a radio-frequency discharge.
Helium RF discharge radiation temperature as magnetic field function measured, discussing enhanced diffusion role in radiation temperature determination
RADIO FREQUENCY DISCHARGE↗
Spectra-spectroheliograph observations
Spectraspectroheliograph observations, noting correlations between contour maps of solar continuum intensity and magnetic fields
Andelin, J. P.↗
A determination of the intensity of the ancient lunar magnetic field.
Thermal demagnetization of lunar breccia 15498,36 shows that the natural remanent magnetization is a simple thermoremanence carried by metallic iron. Using the classical Thellier-Thellier method the strength of the magnetizing field at the time of sample formation was found to be 2100 plus or minus 80 gammas.
Gose, W. A.↗
Neutral hydrogen flux measured at 100- to 200-km altitude in an electron aurora
Neutral hydrogen fluxes were measured at altitudes of 120-200 km by a rocket payload that also measured electron and proton fluxes and vector magnetic fields. An intense electron arc was crossed, while an upper limit to the flux of 0.5- to 20-keV protons was 1,000,000 per sq cm s sr keV. A neutral flux of 50,000,000 per sq cm s sr was observed, assuming hydrogen with greater than 1-keV energy, with greater north-south extent than the electron flux. Its pitch angle distribution was peaked toward 90 deg, tending toward isotropy in the center. This is fitted to a model describing spreading of an initial proton arc above 500 km.
Iglesias, G. E.↗