67 research outputs found
A new numerical algorithm for a drift-diffusion system
Electrical potentials and free boundary separating the depletion and neutrality regions in a junction field transistor can be computed using a drift-diffusion model for a MESFET. This paper presents a new numerical algorithm of this model using a fixed point method. Numerical results are encouraging and provides a reasonably free boundary.Electrical potentials and free boundary separating the depletion and neutrality regions in a junction field transistor can be computed using a drift-diffusion model for a MESFET. This paper presents a new numerical algorithm of this model using a fixed point method. Numerical results are encouraging and provides a reasonably free boundary
A Global Fireball Observatory
The world's meteorite collections contain a very rich picture of what the
early Solar System would have been made of, however the lack of spatial context
with respect to their parent population for these samples is an issue. The
asteroid population is equally as rich in surface mineralogies, and mapping
these two populations (meteorites and asteroids) together is a major challenge
for planetary science. Directly probing asteroids achieves this at a high cost.
Observing meteorite falls and calculating their pre-atmospheric orbit on the
other hand, is a cheaper way to approach the problem. The Global Fireball
Observatory (GFO) collaboration was established in 2017 and brings together
multiple institutions (from Australia, USA, Canada, Morocco, Saudi Arabia, the
UK, and Argentina) to maximise the area for fireball observation time and
therefore meteorite recoveries. The members have a choice to operate
independently, but they can also choose to work in a fully collaborative manner
with other GFO partners. This efficient approach leverages the experience
gained from the Desert Fireball Network (DFN) pathfinder project in Australia.
The state-of-the art technology (DFN camera systems and data reduction) and
experience of the support teams is shared between all partners, freeing up time
for science investigations and meteorite searching. With all networks combined
together, the GFO collaboration already covers 0.6% of the Earth's surface for
meteorite recovery as of mid-2019, and aims to reach 2% in the early 2020s. We
estimate that after 5 years of operation, the GFO will have observed a fireball
from virtually every meteorite type. This combined effort will bring new,
fresh, extra-terrestrial material to the labs, yielding new insights about the
formation of the Solar System.Comment: Accepted in PSS. 19 pages, 9 figure
Effects of medroxyprogesterone acetate on cerebral oedema and spatial learning performance after traumatic brain injury in rats
Comprehensive molecular characterization of human adipocytes reveals a transient brown phenotype
Constraints on the structure and seasonal variations of Tritonâs atmosphere from the 5 October 2017 stellar occultation and previous observationsâ
Context. A stellar occultation by Neptune's main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of which yielded a central flash detection. Aims. We aimed at constraining Triton's atmospheric structure and the seasonal variations of its atmospheric pressure since the Voyager 2 epoch (1989). We also derived the shape of the lower atmosphere from central flash analysis. Methods. We used Abel inversions and direct ray-tracing code to provide the density, pressure, and temperature profiles in the altitude range âŒ8 km to âŒ190 km, corresponding to pressure levels from 9 ÎŒbar down to a few nanobars. Results. (i) A pressure of 1.18 ± 0.03 ÎŒbar is found at a reference radius of 1400 km (47 km altitude). (ii) A new analysis of the Voyager 2 radio science occultation shows that this is consistent with an extrapolation of pressure down to the surface pressure obtained in 1989. (iii) A survey of occultations obtained between 1989 and 2017 suggests that an enhancement in surface pressure as reported during the 1990s might be real, but debatable, due to very few high S/N light curves and data accessible for reanalysis. The volatile transport model analysed supports a moderate increase in surface pressure, with a maximum value around 2005-2015 no higher than 23 ÎŒbar. The pressures observed in 1995-1997 and 2017 appear mutually inconsistent with the volatile transport model presented here. (iv) The central flash structure does not show evidence of an atmospheric distortion. We find an upper limit of 0.0011 for the apparent oblateness of the atmosphere near the 8 km altitude
Meteor Detection from the Fireball Moroccan Network: First Orbital Results and Links to Parent Bodies
International audienceA network of meteor stations is being deployed in Morocco with the aim to determine meteor trajectories and their relationships with possible parent bodies. Several meteor showers may be related to known parent bodies, such as the the comet 109P/Swift-Tuttle, which is associated to Perseids. Two stations of meteor observations with Watec cameras were recently installed in Morocco as part of this network, one at the Oukaimeden Observatory and the other at Marrakech. This paper presents the implementation of a software to determine the orientation of the camera, and the preliminary results obtained with the two stations
Meteor Detection from the Fireball Moroccan Network: First Orbital Results and Links to Parent Bodies
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