Turbulence in the ionosphere is important to understand because it can negatively affect communication signals. This work examines different scenarios in the ionosphere in which turbulence may develop. The two main causes of turbulence considered in this work are the gradient drift instability (GDI) and the Kelvin-Helmholtz instability (KHI). The likelihood of the development of the GDI during the August 17, 2017 total solar eclipse is studied numerically. This analysis uses the ``Sami3 is Also a Model of the Ionosphere" (SAMI3) model to study the effect of the eclipse on the plasma density. The calculated GDI growth rates are small compared to how quickly the eclipse moves over the Earth. Therefore, the GDI is not expected to occur during the solar eclipse. A novel 2D electrostatic pseudo-spectral fluid model is developed to study the growth of these two instabilities and the problem of ionospheric turbulence in general. To focus on the ionospheric turbulence, a set of perturbed governing equations are derived. The model accurately captures the GDI growth rate in different limits; it is also benchmarked to the evolution of instability development in different collisional regimes of a plasma cloud. The newly developed model is used to study if the GDI is the cause of density irregularities observed in subauroral polarization streams (SAPS). Data from Global Positioning System (GPS) scintillations and the Super Dual Auroral Radar Network (SuperDARN) are used to examine the latitudinal density and velocity profiles of SAPS. It is found that the GDI is stabilized by velocity shear and therefore will only generate density irregularities in regions of low velocity shear. Furthermore, the density irregularities cannot extend through regions of large velocity shear. In certain cases, the turbulence cascade power laws match observation and theory. The transition between the KHI and the GDI is studied by understanding the effect of collisions. In low collisionality regimes, the KHI is the dominant instability. In high collisionality regimes, the GDI is the dominant instability. Using nominal ionospheric parameters, a prediction is provided that suggests that there exists an altitude in the upper textit{F} region ionosphere above which the turbulence is dominated by the KHI. / Doctor of Philosophy / In the modern day, all wireless communication signals use electromagnetic waves that propagate through the atmosphere. In the upper atmosphere, there exists a region called the ionosphere, which consists of plasma (a mixture of ions, electrons, and neutral particles). Because ions and electrons are charged particles, they interact with the electromagnetic communication signals. A better understanding of ionospheric turbulence will allow for aid in forecasting space weather as well as improve future communication equipment. Communication signals become distorted as they pass through turbulent regions of the ionosphere, which negatively affects the signal quality at the receiving end. For a tangible example, when Global Positioning System (GPS) signals pass through turbulent regions of the ionosphere, the resulting position estimate becomes worse. This work looks at two specific causes of ionospheric turbulence: the gradient drift instability (GDI) and the Kelvin-Helmholtz instability (KHI). Under the correct background conditions, these instabilities have the ability to generate ionospheric turbulence. To learn more about the GDI and the KHI, a novel simulation model is developed. The model uses a method of splitting the equations such that the focus is on just the development of the turbulence while considering spatially constant realistic background conditions. The model is shown to accurately represent results from previously studied problems in the ionosphere. This model is applied to an ionospheric phenomenon known as subauroral polarization streams (SAPS) to study the development of the GDI and the KHI. SAPS are regions of the ionosphere with large westward velocity that changes with latitude. The shape of the latitudinal velocity profile depends on many other factors in the ionosphere such as the geomagnetic conditions. It is found that for certain profiles, the GDI will form in SAPS with some of these examples matching observational data. At higher altitudes, the model predicts that the KHI will form instead. While the model is applied to just the development of the GDI and the KHI in this work, it is written in a general manner such that other causes of ionospheric turbulence can be easily studied in the future.

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La projection par plasma d'arc de suspension permet d'obtenir des revêtements finement structurés à gradients de propriétés qui répondent aux besoins, par exemple, des applications photocatalytiques, les piles à combustible à oxyde solide ou les revêtements de barrière thermique. Cependant, les torches à plasma, même alimentées par dessources de courant continu régulé, génèrent des jets de plasma fortement fluctuants. Ces instabilités causent des variations importantes dans les transferts thermiques et dynamiques des particules, ce qui diminue la fiabilité et la reproductibilité de la méthode. Par conséquent, des efforts particuliers doivent être faits pour améliorer la projectionpar plasma d'arc de suspension et, ainsi, les propriétés des revêtements. Depuis de nombreuses années, la recherche s'est concentrée sur l'amélioration des transferts de chaleur et de quantité de mouvement entre la matière et le plasma au moyen de la mise au point de nouvelles torches et la réduction des instabilités de l'arc. Cette thèse présenteune nouvelle approche pour la projection par plasma d'arc de suspension. L'étude approfondie des instabilités du plasma sont réalisées ce qui conduit à la production du jet laminaire de plasma pulsé caractérisé par une forte modulation de l'enthalpie spécifique. Ces oscillations régulières de plasma sont associées à l'injection de la suspensionsynchronisée, ce qui est réalisé à l'aide de l'impression à jet d'encre déclenchée par le signal de tension d'arc. Les résultats sont évalués par le système d'imagerie résolue en temps et la spectroscopie d'émission optique résolue en temps. Cette nouvelle méthode offre la possibilité de contrôler les transferts de chaleur et de quantité de mouvemententre les particules et le plasma. / Suspension plasma spraying permits to elaborate finely structured coatings with graded properties which address the needs, for example, in the photocatalytic applications, the solid oxide fuels or the thermal barrier coatings. However, the plasma torches, even powered by dc regulated sources, generate highly fluctuating plasma jets. These instabilities result in large variations in dynamic and heat transfers to particles, what decreases the reproducibility and reliability of the method. Consequently, the special efforts have to be devoted to ameliorate the suspension plasma spraying method and, thus, the properties of the coatings. In recent years, the research has been focused on the improvement of heat and momentum transfers between material and plasma by means of the development of new non-conventional torches and the reduction of arc instabilities. The following dissertation presents a new approach to the suspension plasma spraying. The profound studies of the plasma instabilities are performed, what leads to the production of the pulsed laminar plasma jet characterized by high modulation of the specific enthalpy. These regular plasma oscillations are combined with phased injection of suspension, what is achieved by using the ink-jet printer triggered by the arc voltage signal. The results are evaluated by time-resolved imaging system and the time-resolved emission optical spectroscopy. This new method presents the possibility to control heat and momentum transfers between the particles and the plasma.

The common observation that the onset of a core MARFE (edge localized, poloidally asymmetric, highly radiating region) is followed immediately by a High-to-Low confinement mode transition in DIII-D was investigated by comparing a theoretical prediction of the threshold non-radiative power across the separatrix needed to maintain H-mode with an experimental determination of the non-radiative power flowing across the separatrix. It was found that in three shots with continuous gas fueling that the increased neutral influx associated with the MARFE formation caused a sharp increase in the predicted threshold non-radiative power crossing the separatrix that was required for the plasma to remain in H-mode to a value comparable to the experimental power crossing the separatrix, indicating a theoretical prediction of a H-L transition in agreement with experimental observation.