Radiation damage in thick copper and gold specimens produced by low-energy protons
Radiation damage in low energy proton irradiated thick copper and gold foils and subsequent annealing characteristics
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Radiation damage in low energy proton irradiated thick copper and gold foils and subsequent annealing characteristics
Phenomenological study of radiation damage and recoverability of metal oxide field effect transistors
Mechanisms of recovery of radiation damaged silicate treated zinc oxide thermal control coatings
Silicon solar cells radiation damage from low energy protons, discussing current degradation as function of exposed area and particle energy
Lithium doped silicon solar cells under electron irradiation and determination of semiconductor parameters
Space environment radiation effects on solar cell degradation
Radiation damage and transport damage in solar cells
Thermal annealing of silicon solar cells with direct solar heating or electric storage methods to avoid radiation damage
This study investigates the evolution of radiation damage in three metals in the low temperature and high radiant flux regime using molecular statics and a Frenkel pair accumulation method to simulate up to 2.0 displacements per atom. The metals considered include Fe, equiatomic CrCoNi, and a fictitious metal with similar bulk properties to the CrCoNi composed of a single atom type referred to as an A-atom. CrCoNi is found to sustain higher concentrations of dislocations than either the Fe or A-atom systems and more stacking faults than the A-atom system. The results suggest that the difference between the concentrations of vacancies and interstitials is substantially smaller for CrCoNi than the A-atom system, perhaps reflecting that the sink capture radius is smaller in CrCoNi due to the roughened potential energy landscape. A model that partitions the major contributions from defects to the stored energy is described, and serves to highlight a general need for higher fidelity approaches to point defect identification.
Structure of radiation damage in lithium diffused solar cells
ATS-F solar cell radiation damage experiment design and ground tests including space environment simulation and low-energy proton and electron irradiation
The improved infrared response (IRR) technique has been used to qualitatively compare radiation effects on Si(Li) detectors with energy levels reported for silicon in the literature. Measurements have been made on five commercial silicon detectors and one fabricated in-house, both before and after irradiation with fast neutrons, 1.9-MeV protons, and 1.6-MeV electrons. Effects dependent upon the extent of radiation damage have been observed. It seems likely that the photo-EMF, or photo-voltage, effect is the basic mechanism for the observation of IRR in p-i-n diodes with a wide i-region. Experimental characteristics of the IRR measurement are in agreement with those of the photovoltage effect.
Annealing of radiation damage was observed for the first time in VPE-grown, 2- by 2-cm, n+/p/p+ GaAs shallow homojunction solar cells. Electrical performance of several cells was determined as a function of 1-MeV electron fluence in the range of 10 to the 13th power to 10 to the 15th power e-/sq cm and as a function of thermal annealing time at various temperatures. Degradation of normalized power output after a fluence of 10 to the 15th power 1-MeV electrons/sq cm ranged from a low of 24 to 31 percent of initial maximum power. Normalized short circuit current degradation was limited to the range from 10 to 19 percent of preirradiated values. Thermal annealing was carried out in a flowing nitrogen gas ambient, with annealing temperatures spanning the range from 125 to 200 C. Substantial recovery of short circuit current was observed at temperatures as low as 175 C. In one case improvement by as much as 10 percent of the postirradiated value was observed. The key features of these cells are their extremely thin emitter layers (approxmately 0.05 micrometers), the absence of any Al sub xGd sub 1-x As passivating window layer, and their fabrication by vapor phase epitaxy.
Effects of impurities in base material of silicon solar cells junction characteristics and radiation damage
Radiation damage to silicon and germanium semiconductors by high energy electrons
Alpha particles radiation damage effects in silicon surface barrier detector
High-voltage electron microscopy has been used to compare radiation effects in micron-size soil grains from the Luna 16 site (Mare Fecunditatis) and the four Apollo landing sites. Radiation damage by heavy solar particles is strikingly greater in the Luna 16 sample than in the other four samples. It is suggested that less movement of the soil at Mare Fecunditatis has taken place, perhaps because of its proximity to the limb and consequent lower exposure to energetic electrons in the earth's magnetospheric tail, which would cause electrostatic agitation of fine particles.
Design and performance of an experimental silicon p-n junction cell which is resistant to radiation damage and intended for space application