Amberly Evans Jensen
Utah State University
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Featured researches published by Amberly Evans Jensen.
Proceedings of SPIE | 2013
Jr Dennison; Amberly Evans Jensen; Gregory Wilson; Justin Dekany; Charles W. Bowers; Robert Meloy
Electron irradiation experiments have investigated the diverse electron-induced optical and electrical signatures observed in ground-based tests of various space observatory materials at low temperature. Three types of light emission were observed: (i); long-duration cathodoluminescence which persisted as long as the electron beam was on (ii) short-duration (<1 s) arcing, resulting from electrostatic discharge; and (iii) intermediate-duration (~100 s) glow—termed “flares”. We discuss how the electron currents and arcing—as well as light emission absolute intensity and frequency—depend on electron beam energy, power, and flux and the temperature and thickness of different bulk (polyimides, epoxy resins, and silica glasses) and composite dielectric materials (disordered SiO2 thin films, carbon- and fiberglass-epoxy composites, and macroscopically-conductive carbon-loaded polyimides). We conclude that electron-induced optical emissions resulting from interactions between observatory materials and the space environment electron flux can, in specific circumstances, make significant contributions to the stray light background that could possibly adversely affect the performance of space-based observatories.
IEEE Transactions on Plasma Science | 2013
Gregory Wilson; Jr Dennison; Amberly Evans Jensen; Justin Dekany
Measurements of the charge distribution in electron-bombarded, thin-film, and multilayer dielectric samples showed that charging of multilayered materials evolves with time and is highly dependent on incident energy; this is driven by electron penetration depth, electron emission, and material conductivity. Based on the net surface potentials dependence on beam current, electron range, electron emission, and conductivity, measurements of the surface potential, displacement current, and beam energy allow the charge distribution to be inferred. To take these measurements, a thin-film disordered SiO2 structure with a conductive middle layer was charged using 200-eV and 5-keV electron beams with regular 15-s pulses at 1-500 nA/cm2. Results show that there are two basic charging scenarios, which are consistent with simple charging models; these are analyzed using independent determinations of the materials electron range, yields, and conductivity. Large negative net surface potentials led to electrostatic breakdown and large visible arcs, which have been observed to lead to detrimental spacecraft charging effects.
Proceedings of SPIE | 2013
Amberly Evans Jensen; Jr Dennison; Gregory Wilson; Justin Dekany; Charles W. Bowers; Robert Meloy; James B. Heaney
Disordered thin film SiO2/SiOx coatings undergoing electron-beam bombardment exhibit cathodoluminescence, which can produce deleterious stray background light in cryogenic space-based astronomical observatories exposed to high energy electron fluxes from space plasmas. As future observatory missions push the envelope into more extreme environments and more complex and sensitive detection, a fundamental understanding of the dependencies of this cathodoluminescence becomes critical to meet performance objectives of these advanced space-based observatories. Measurements of absolute radiance and emission spectra as functions of incident electron energy, flux, and power typical of space environments are presented for thin (~60-200 nm) SiO2/SiOx optical coatings on reflective metal substrates over a range of sample temperatures (~40-400 K) and emission wavelengths (~260-5000 nm). Luminescent intensity and peak wavelengths of four distinct bands were observed in UV/VIS/NIR emission spectra, ranging from 300 nm to 1000 nm. A simple model is proposed that describes the dependence of cathodoluminescence on irradiation time, incident flux and energy, sample thickness, and temperature.
ieee international conference on solid dielectrics | 2013
Amberly Evans Jensen; Jr Dennison; Justin Dekany; Gregory Wilson
Electron irradiation experiments were conducted to investigate the electron transport, charging, discharging, cathodoluminescence and emission properties of high-conductivity carbon-loaded polyimide (Black Kapton™). We discuss how these results are related to the nanoscale structure of the composite material. Measurements were conducted in an ultrahigh vacuum electron emission test chamber from <;40 K to 290 K, using a monoenergetic beam with energies ranging from 3 keV to 25 keV and flux densities from 0.1 nA/cm2 to 100 nA/cm2 to deposit electrons in the material surface layer. Various experiments measured transport and displacement currents to a rear grounded electrode, absolute electron emission yields, electron-induced absolute photon emission yields and photon emission spectra (~250 nm to 1700 nm), and arcing rates and location. Numerous arcing events from the material edge to an electrically isolated grounded sample holder (particularly at lower temperatures) were observed, which are indicative of charge accumulation within the insulating regions of the material. Three types of light emission were also observed: (i) short duration (<;1 s) arcing resulting from electrostatic discharge, (ii) long duration cathodoluminescence that turned on and off with the electron beam and (iii) intermediate duration (~100 s) glow that dissipated exponentially with time after infrequent and rapid onset. We discuss how the electron currents and arcing, as well as light emission absolute intensity and frequency, depend on electron beam energy, power, flux and temperature.
IEEE Transactions on Plasma Science | 2015
Justin Dekany; Justin Christensen; Jr Dennison; Amberly Evans Jensen; Gregory Wilson; Todd A. Schneider; Charles W. Bowers; Robert Meloy
Many contemporary spacecraft materials exhibit cathodoluminescence when exposed to electron flux from the space plasma environment. A quantitative physics-based model has been developed to predict the intensity of the total glow as a function of incident electron current density and energy, temperature, and intrinsic material properties. We present a comparative study of the absolute spectral radiance for more than 20 types of dielectric and composite materials based on this model, which spans more than three orders of magnitude. Variations in intensity are contrasted for different electron environments, different sizes of samples and sample sets, different testing and analysis methods, and data acquired at different test facilities. Together, these results allow us to estimate the accuracy and precision to which laboratory studies may be able to determine the response of spacecraft materials in the actual space environment. It also provides guidance as to the distribution of emissions that may be expected for sets of similar flight hardware under similar environmental conditions.
IEEE Transactions on Plasma Science | 2015
Amberly Evans Jensen; Jr Dennison
Electron beam measurements show that disordered SiO2 exhibits electron-induced luminescence and that it varies with incident beam energy and current density, sample temperature, and wavelength. A simple model based on the electronic band structure and defect density of states-initially used to explain electron transport in highly disordered insulating materials-has been extended to predict the relative cathodoluminescent intensity and spectral radiance for disordered SiO2 as a function of these variables. Due to the large bandgap of insulating SiO2, thermal excitation from the valence to conduction band is highly improbable; excitation is through collisions of the incident high-energy electrons. For visible and near-infrared light to be emitted, there must be other states within the forbidden bandgap for electrons to occupy. These localized defect or trap states of disordered SiO2 are due to structural or substitutional chemical defects. Results for both thin-film samples with penetrating radiation and thick bulk samples with nonpenetrating radiation are presented. The data were fit with the proposed model using saturation dose rate and mean shallow trap energy as fitting parameters, which favorably compare with results from independent experiments.
Proceedings of the 13th Spacecraft Charging Technology Conference | 2014
Amberly Evans Jensen; Jr Dennison
Archive | 2014
Amberly Evans Jensen
Archive | 2013
Ryan Hoffmann; Jr Dennison; Greg Wilson; Amberly Evans Jensen
Archive | 2011
Amberly Evans Jensen; Gregory Wilson; Jr Dennison