1,229 research outputs found
MHD simulations of the solar photosphere
We briefly review the observations of the solar photosphere and pinpoint some
open questions related to the magnetohydrodynamics of this layer of the Sun. We
then discuss the current modelling efforts, addressing among other problems,
that of the origin of supergranulation.Comment: 10 pages, 6 figures; 4th French-Chinese Meeting on Solar Physics
Understanding Solar Activity: Advances and Challenges, 4th French-Chinese,
Nice, Franc
Mesoscale dynamics on the Sun's surface from HINODE observations
Aims: The interactions of velocity scales on the Sun's surface, from
granulation to supergranulation are still not understood, nor are their
interaction with magnetic fields. We thus aim at giving a better description of
dynamics in the mesoscale range which lies between the two scales mentioned
above. Method: We analyse a 48h high-resolution time sequence of the quiet Sun
photosphere at the disk center obtained with the Solar Optical Telescope
onboard Hinode. The observations, which have a field of view of 100
\arcsec 100 \arcsec, typically contain four supergranules. We monitor
in detail the motion and evolution of granules as well as those of the radial
magnetic field. Results: This analysis allows us to better characterize Trees
of Fragmenting Granules issued from repeated fragmentation of granules,
especially their lifetime statistics. Using floating corks advected by measured
velocity fields, we show their crucial role in the advection of the magnetic
field and in the build up of the network. Finally, thanks to the long duration
of the time series, we estimate that the turbulent diffusion coefficient
induced by horizontal motion is approximately . Conclusions: These results demonstrate that the long living
families contribute to the formation of the magnetic network and suggest that
supergranulation could be an emergent length scale building up as small
magnetic elements are advected and concentrated by TFG flows. Our estimate for
the magnetic diffusion associated with this horizontal motion might provide a
useful input for mean-field dynamo models.Comment: to appear in A&A - 8 pages, 13 figures (degraded quality) - Full
resolution version available @
http://www.ast.obs-mip.fr/users/rincon/hinode_roudier_aa09.pd
Heavy flavor in relativistic heavy-ion collisions
We study charm production in ultra-relativistic heavy-ion collisions by using
the Parton-Hadron-String Dynamics (PHSD) transport approach. The initial charm
quarks are produced by the PYTHIA event generator tuned to fit the transverse
momentum spectrum and rapidity distribution of charm quarks from Fixed-Order
Next-to-Leading Logarithm (FONLL) calculations. The produced charm quarks
scatter in the quark-gluon plasma (QGP) with the off-shell partons whose masses
and widths are given by the Dynamical Quasi-Particle Model (DQPM), which
reproduces the lattice QCD equation-of-state in thermal equilibrium. The
relevant cross sections are calculated in a consistent way by employing the
effective propagators and couplings from the DQPM. Close to the critical energy
density of the phase transition, the charm quarks are hadronized into
mesons through coalescence and/or fragmentation. The hadronized mesons then
interact with the various hadrons in the hadronic phase with cross sections
calculated in an effective lagrangian approach with heavy-quark spin symmetry.
The nuclear modification factor and the elliptic flow of
mesons from PHSD are compared with the experimental data from the STAR
Collaboration for Au+Au collisions at =200 GeV and to the ALICE
data for Pb+Pb collisions at =2.76 TeV. We find that in the
PHSD the energy loss of mesons at high can be dominantly attributed
to partonic scattering while the actual shape of versus reflects
the heavy-quark hadronization scenario, i.e. coalescence versus fragmentation.
Also the hadronic rescattering is important for the at low and
enhances the -meson elliptic flow .Comment: 8 pages, 3 figures, to be published in the Proceedings of the 15th
International Conference on Strangeness in Quark Matter (SQM2015), 6-11 July
2015, JINR, Dubna, Russi
Al Partitioning Patterns and Root Growth as Related to Al Sensitivity and Al Tolerance in Wheat
Abundance and Diversity of Dockerin-Containing Proteins in the Fiber-Degrading Rumen Bacterium, Ruminococcus flavefaciens FD-1
Peer reviewedPublisher PD
Development of the ECOSAR P-Band Synthetic Aperture Radar
This paper describes objectives and recent progress on the development of the EcoSAR, a new P-band airborne radar instrument being developed at the NASA/ Goddard Space Flight Center (GSFC) for the polarimetric and interferometric measurements of ecosystem structure and biomass. These measurements support science requirements for the study of the carbon cycle and its relationship to climate change. The instrument is scheduled to be completed and flight tested in 2013. Index Terms SAR, Digital Beamforming, Interferometry
Next-generation muscle-directed gene therapy by in silico vector design
There is an urgent need to develop the next-generation vectors for gene therapy of muscle disorders, given the relatively modest advances in clinical trials. These vectors should express substantially higher levels of the therapeutic transgene, enabling the use of lower and safer vector doses. In the current study, we identify potent muscle-specific transcriptional cisregulatory modules (CRMs), containing clusters of transcription factor binding sites, using a genome-wide data-mining strategy. These novel muscle-specific CRMs result in a substantial increase in muscle-specific gene transcription (up to 400-fold) when delivered using adeno-associated viral vectors in mice. Significantly higher and sustained human micro-dystrophin and follistatin expression levels are attained than when conventional promoters are used. This results in robust phenotypic correction in dystrophic mice, without triggering apoptosis or evoking an immune response. This multidisciplinary approach has potentially broad implications for augmenting the efficacy and safety of muscle-directed gene therapy
Towards a SAR System for Personalized Cardiac Rehabilitation: A Patient with PCI
Physical activity has been shown to have multiple benefits, such as reducing mortality rate caused by cardiovascular diseases and providing an optimal health status, making it one of the most important components of cardiac rehabilitation (CR) programs. However, the adherence to the program is low, and finding strategies to motivate people to perform physical training is a priority. This work proposes the introduction of a socially assistive robotics system in order to provide monitoring and motivation to patients within a CR program. A study was carried out with one patient accompanied by the robot during a conventional phase II, namely 16 sessions of the cardiac rehabilitation program. The results show the reliability of the system to provide information to assess the patient's performance during the activity. Additionally, the patient was able to improve his posture patterns along the sessions due to the continuous monitoring provided by the robot
YAG thermal barrier coatings deposited by suspension and solution precursor thermal spray
Yttrium aluminium garnet (YAG) is a promising topcoat material for thermal barrier coatings due to its high temperature stability and better CMAS (calcium-magnesium-alumino-silicate) resistance. YAG topcoats were deposited by suspension and solution precursor high-velocity oxy-fuel (HVOF) thermal spray. The relationships between processing, microstructure and final properties were studied through a range of characterization techniques and thermal cycling tests. The microstructure of the as-sprayed YAG topcoat from stoichiometric solution precursor (SP-YAG) had distributed pores and inter-splat boundaries, while the as-sprayed topcoat produced from suspension (S-YAG) had vertical and branched micro cracks, pores, and inter-splat boundaries. Both as-sprayed coatings were composed of amorphous phase, hexagonal yttrium aluminium perovskite (YAP) and cubic YAG. In thermal cycling tests, 20% of SP-YAG failure was reached after the 10th cycle; whereas, S-YAG reached the failure criteria between the 60th and 70th cycle. The failure of both the SP-YAG and the S-YAG topcoats occurred due to thermal stresses during the thermal cycling
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