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Optical Properties of Front and Second Surface Silver-Based
Optical Properties of Front and Second Surface Silver-Based

... Houda Ennaceri was born in Morocco. She is currently conducting her PhD research in physics of materials at University Mohammed V-Agdal, Rabat 10000, Morocco, and holds a master’s degree in sustainable energy management in (MSSEM) from Al Akhawayn University in 2013, and a bachelor’s degree in engin ...
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R E S U M E - UCF College of Sciences

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... black holes and neutron stars, as discussed later in this chapter. The upper end of the relevant temperature range is achieved in the limit of the optically thin emission. It is not unreasonable to link it to the virial temperature of particles near the black hole, kTvir = GMm/r ∝ mc2 /(r/r g ). Unl ...
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... is due to a variety of processes including collisional cooling, gasgrain energy transfer and recombination on grain surfaces. The gas initially lies within a radius of 10 kpc, and has an initial temperature of 700 K. The implementation of stellar feedback will be described in detail in a forthcoming ...
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... into account with simple approximated recipes. The main advantage of these models resides in the possibility of predicting the properties of whole galaxy populations in a short amount of computing time, thus making it possible to achieve a good sampling of the parameter space. However, it has been r ...
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... On the giant molecular cloud scale, given an approximate mass one can calculate the gravitational potential energy and find that it is far greater in absolute value than the thermal energy. Thus the clouds are certainly highly gravitationally bound, but in general they are not collapsing. The linewi ...
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... Writing the metric in this form shows that if κ is non-zero, angular lengths are either decreased (for positive curvature) or increased (for negative). Just as importantly, this metric indicates that, like in Minkowski space, time is orthogonal to position (meaning we can foliate the spacetime such ...
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... which effectively smooths the output images from FWHM ≈ 5000 to ≈5400 . See Mangum et al. (2007) for more detail on the on-the-fly mapping technique used here. The Arecibo data were taken at a spectral resolution of 0.68 km s−1 . The spectra were regridded onto a velocity grid from −50 to 150 km s−1 ...
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... describing a syndrome of apparently related processes at various wavelengths. The problem is even more acute in other languages, such as German and French, denoting flares with the equivalent to “eruption”, which may be confused with Coronal Mass Ejections (CMEs) that often happen simultaneously at ...
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Microplasma



Microplasmas are plasmas of small dimensions, ranging from tens to thousands of micrometers. They can be generated at a variety of temperatures and pressures, existing as either thermal or non-thermal plasmas. Non-thermal microplasmas that can maintain their state at standard temperatures and pressures are readily available and accessible to scientists as they can be easily sustained and manipulated under standard conditions. Therefore, they can be employed for commercial, industrial, and medical applications, giving rise to the evolving field of microplasmas.
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