Charge storage effects in Mylar resulting from electron irradiation, June 1965 - June 1966
Charge storage effects in Mylar from electron irradiation
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Charge storage effects in Mylar from electron irradiation
Adenine synthesis by electron irradiation of gas mixture of methane, ammonia, and water
Equatorial ionospheric propagation studies using rocket sounding techniques
Observation and analysis of auroral zone electron microbursts recorded by Injun 3 satellite
Annealing behavior and uniaxial stress response of radiation induced defects in Si causing 1.8, 3.3 and 3.9 micron IR absorption bands examined via EPR studies
Conversion process and ESR in gamma-irradiated dihydrothymine noting reaction rate
Subthreshold electron irradiation effects on surface recombination properties of n- and p-type germanium and silicon crystals
Electron temperature of H II region related to high temperature main sequence stars determined as function of electron density and radiation dilution factor
Isochronal annealing of short-circuit current of electron irradiated silicon solar cells
Partition of recombination energy among electrons and radiation in decaying rare gas plasmas
Intrinsic magnetic dipole moment of Venus based on absence of radiation belt electrons
Recombination rate of electrons in high pressure helium-like plasma with gas temperature fixed at 300 K and electron temperature varied between 300-2000 K
RF synchrotron emission from electrons trapped in earth magnetic field observed by satellite, using magnetospheric environment model
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.
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The various subdisciplines of high-energy astrophysics are surveyed in a series of articles which attempt to give an overall view of the subject as a whole by emphasizing the basic physics common to all fields in which high-energy particles and quanta play a role. Successive chapters cover cosmic ray experimental observations, the abundances of nuclei in the cosmic radiation, cosmic electrons, solar modulation, solar particles (observation, relationship to the sun acceleration, interplanetary medium), radio astronomy, galactic X-ray sources, the cosmic X-ray background, and gamma ray astronomy. Individual items are announced in this issue.
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A Monte Carlo method is described for evaluation of the spectrum, directivity and polarization of X-rays diffusely reflected from stellar photospheres. the accuracy of the technique is evaluated through comparison with analytic results. Using the characteristics of the incident X-rays of the model for solar X-ray flares, the spectrum, directivity and polarization of the reflected and the total X-ray fluxes are evaluated. The results are compared with observations.