13,998 research outputs found
Strapdown calibration and alignment study. Volume 2 - Procedural and parametric trade-off analyses document Final report
Parametric and procedural tradeoffs for alignment and calibration of inertial sensing uni
Strapdown calibration and alignment study. Volume 2 - Procedural and parametric trade- off analyses document
Techniques for laboratory calibration and alignment of strapdown inertial sensing unit - procedural and parametric trade-off analyse
Buneman instability in a magnetized current-carrying plasma with velocity shear
Buneman instability is often driven in magnetic reconnection. Understanding
how velocity shear in the beams driving the Buneman instability affects the
growth and saturation of waves is relevant to turbulence, heating, and
diffusion in magnetic reconnection. Using a Mathieu-equation analysis for weak
cosine velocity shear together with Vlasov simulations, the effects of shear on
the kinetic Buneman instability are studied in a plasma consisting of strongly
magnetized electrons and cold unmagnetized ions. In the linearly unstable
phase, shear enhances the coupling between oblique waves and the sheared
electron beam, resulting in a wider range of unstable eigenmodes with common
lower growth rates. The wave couplings generate new features of the electric
fields in space, which can persist into the nonlinear phase when electron holes
form. Lower hybrid instabilities simultaneously occur at
with a much lower growth
rate, and are not affected by the velocity shear.Comment: Accepted by Physics of Plasm
Solcore: A multi-scale, python-based library for modelling solar cells and semiconductor materials
Computational models can provide significant insight into the operation
mechanisms and deficiencies of photovoltaic solar cells. Solcore is a modular
set of computational tools, written in Python 3, for the design and simulation
of photovoltaic solar cells. Calculations can be performed on ideal,
thermodynamic limiting behaviour, through to fitting experimentally accessible
parameters such as dark and light IV curves and luminescence. Uniquely, it
combines a complete semiconductor solver capable of modelling the optical and
electrical properties of a wide range of solar cells, from quantum well devices
to multi-junction solar cells. The model is a multi-scale simulation accounting
for nanoscale phenomena such as the quantum confinement effects of
semiconductor nanostructures, to micron level propagation of light through to
the overall performance of solar arrays, including the modelling of the
spectral irradiance based on atmospheric conditions. In this article we
summarize the capabilities in addition to providing the physical insight and
mathematical formulation behind the software with the purpose of serving as
both a research and teaching tool.Comment: 25 pages, 18 figures, Journal of Computational Electronics (2018
Detailed Structure and Dynamics in Particle-in-Cell Simulations of the Lunar Wake
The solar wind plasma from the Sun interacts with the Moon, generating a wake
structure behind it, since the Moon is to a good approximation an insulator,
has no intrinsic magnetic field and a very thin atmosphere. The lunar wake in
simplified geometry has been simulated via a 1-1/2-D electromagnetic
particle-in-cell code, with high resolution in order to resolve the full phase
space dynamics of both electrons and ions. The simulation begins immediately
downstream of the moon, before the solar wind has infilled the wake region,
then evolves in the solar wind rest frame. An ambipolar electric field and a
potential well are generated by the electrons, which subsequently create a
counter-streaming beam distribution, causing a two-stream instability which
confines the electrons. This also creates a number of electron phase space
holes. Ion beams are accelerated into the wake by the ambipolar electric field,
generating a two stream distribution with phase space mixing that is strongly
influenced by the potentials created by the electron two-stream instability.
The simulations compare favourably with WIND observations.Comment: 10 pages, 13 figures, to be published in Physics of Plasma
The Effect on the Lunar Exosphere of a Coroual Mass Ejection Passage
Solar wind bombardment onto exposed surfaces in the solar system produces an energetic component to the exospheres about those bodies. The solar wind energy and composition are highly dependent on the origin of the plasma. Using the measured composition of the slow wind, fast wind, solar energetic particle (SEP) population, and coronal mass ejection (CME), broken down into their various components, we have estimated the total sputter yield for each type of solar wind. We show that the heavy ion component, especially the He++ and 0+7 can greatly enhance the total sputter yield during times when the heavy ion population is enhanced. Folding in the flux, we compute the source rate for several species during different types of solar wind. Finally, we use a Monte Carlo model developed to simulate the time-dependent evolution of the lunar exosphere to study the sputtering component of the exosphere under the influence of a CME passage. We simulate the background exosphere of Na, K, Ca, and Mg. Simulations indicate that sputtering increases the mass of those constituents in the exosphere a few to a few tens times the background values. The escalation of atmospheric density occurs within an hour of onset The decrease in atmospheric density after the CME passage is also rapid, although takes longer than the increase, Sputtered neutral particles have a high probability of escaping the moon,by both Jeans escape and photo ionization. Density and spatial distribution of the exosphere can be tested with the LADEE mission
Strapdown calibration and alignment study. Volume 1 - Development document Final report
Calibration and alignment techniques for inertial sensing uni
Deliverable 4.2 Support of joint learing and innovation in grassroots development initiatives: operational quality of arrangements
Multi-centre retrospective study of long-term outcomes following traumatic elbow luxation in 37 dogs
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