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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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Daylight ionospheric scatter propagation and absorption during energetic electron precipitation event in auroral zone using bremsstrahlung observations at balloon altitude
Bremsstrahlung radiation in intense magnetic field proposed as emission mechanism from pulsars, discussing absorption coefficient
Bremsstrahlung radiation emitted from homogeneous, field free, nonrelativistic plasma, deriving formulas
Neutrino production by synchroton process /magnetic bremsstrahlung/ in relativistic electron gas under intense magnetic field
Bremsstrahlung and photoneutrons from electron- photon cascades in thick tungsten and tantalum targets bombarded with low energy electrons
Nonrelativistic electron bremsstrahlung in dense plasma with strong magnetic field
Electrons optical scale time averaged motion dependence in focused laser beam on light intensity gradient, calculating bremsstrahlung spectrum
Angular distribution of thick target bremsstrahlung produced by electron bombardment of Be, Sn and Au surfaces
Coulomb corrections to Bethe-Heitler cross sections for electron-nucleus bremsstrahlung
Suprathermal proton bremsstrahlung cross section calculated by Weizsaecker-Williams method
Metagalactic gamma ray spectra calculated for relativistic electron bremsstrahlung interactions
Calculation of electron and bremsstrahlung dose deposition with energy deposition, transmission, and reflection coefficients for electrons
Magnetic fields, bremsstrahlung, and synchrotron emission in solar flare of October 24, 1969
Calculation of radiation cross section for relativistic suprathermal proton bremsstrahlung to determine contribution to cosmic gamma rays
Electron trapping in dielectrics, providing effective light and inexpensive spacecraft bremsstrahlung shield and lower average radiation energy at synchronous altitudes
Magnetic fields, bremsstrahlung and synchrotron emission in impulsive flare of 24 October 1969
Suprathermal proton bremsstrahlung cross section calculation, using Weizsacker-Williams method
In the process of suprathermal proton bremsstrahlung a suprathermal proton, or if you prefer, simply an energetic proton, strikes a relatively motionless electron in a background plasma and causes the electron to radiate. The differential cross section as a function of energy of the emitted photon calculated was believed to be superior to the conventional one in the case of relativistic collisions.