54 research outputs found
Rosetta photoelectron emission and solar ultraviolet flux at comet 67P
The Langmuir Probe instrument on Rosetta monitored the photoelectron emission
cur- rent of the probes during the Rosetta mission at comet
67P/Churyumov-Gerasimenko, in essence acting as a photodiode monitoring the
solar ultraviolet radiation at wave- lengths below 250 nm. We have used three
methods of extracting the photoelectron saturation current from the Langmuir
probe measurements. The resulting dataset can be used as an index of the solar
far and extreme ultraviolet at the Rosetta spacecraft position, including
flares, in wavelengths that are important for photoionisation of the cometary
neutral gas. Comparing the photoemission current to data measurements by
MAVEN/EUVM and TIMED/SEE, we find good correlation when 67P was at large
heliocentric distances early and late in the mission, but up to 50 percent
decrease of the expected photoelectron current at perihelion. We discuss
possible reasons for the photoemission decrease, including scattering and
absorption by nanograins created by disintegration of cometary dust far away
from the nucleus.Comment: 11 pages, 8 figures, accepted for publication in MNRA
Distribution dependent SDEs driven by additive fractional Brownian motion
We study distribution dependent stochastic differential equations with irregular, possibly distributional drift, driven by an additive fractional Brownian motion of Hurst parameter . We establish strong well-posedness under a variety of assumptions on the drift; these include the choice B(·,μ)=(f∗μ)(·)+g(·),f,g∈B∞,∞α,α>1-12H,thus extending the results by Catellier and Gubinelli (Stochast Process Appl 126(8):2323–2366, 2016) to the distribution dependent case. The proofs rely on some novel stability estimates for singular SDEs driven by fractional Brownian motion and the use of Wasserstein distances
Distribution dependent SDEs driven by additive continuous noise
We study distribution dependent stochastic differential equation driven by a continuous process, without any specification on its law, following the approach initiated in [17]. We provide several criteria for existence and uniqueness of solutions which go beyond the classical globally Lipschitz setting. In particular we show well-posedness of the equation, as well as almost sure convergence of the associated particle system, for drifts satisfying either Osgood-continuity, monotonicity, local Lipschitz or Sobolev differentiability type assumptions
The control of brain network dynamics across diverse scales of space and time
The human brain is composed of distinct regions that are each associated with
particular functions and distinct propensities for the control of neural
dynamics. However, the relation between these functions and control profiles is
poorly understood, as is the variation in this relation across diverse scales
of space and time. Here we probe the relation between control and dynamics in
brain networks constructed from diffusion tensor imaging data in a large
community based sample of young adults. Specifically, we probe the control
properties of each brain region and investigate their relationship with
dynamics across various spatial scales using the Laplacian eigenspectrum. In
addition, through analysis of regional modal controllability and partitioning
of modes, we determine whether the associated dynamics are fast or slow, as
well as whether they are alternating or monotone. We find that brain regions
that facilitate the control of energetically easy transitions are associated
with activity on short length scales and slow time scales. Conversely, brain
regions that facilitate control of difficult transitions are associated with
activity on long length scales and fast time scales. Built on linear dynamical
models, our results offer parsimonious explanations for the activity
propagation and network control profiles supported by regions of differing
neuroanatomical structure.Comment: 12 pages, 7 figures. arXiv admin note: text overlap with
arXiv:1607.0101
Kelvin-Helmholtz instability in the presence of variable viscosity for mudflow resuspension in estuaries
The temporal stability of a parallel shear flow of miscible fluid layers of dif- ferent density and viscosity is investigated through a linear stability analysis and direct numerical simulations. The geometry and rheology of this Newto- nian fluid mixing can be viewed as a simplified model of the behavior of mud- flow at the bottom of estuaries for suspension studies. In this study, focus is on the stability and transition to turbulence of an initially laminar configuration. A parametric analysis is performed by varying the values of three control pa- rameters, namely the viscosity ratio, the Richardson and Reynolds numbers, in the case of initially identical thickness of the velocity, density and viscosity profiles. The range of parameters has been chosen so as to mimic a wide variety of real configurations. This study shows that the Kelvin-Helmholtz instability is controlled by the local Reynolds and Richardson numbers of the inflection point. In addition, at moderate Reynolds number, viscosity strat- ification has a strong influence on the onset of instability, the latter being enhanced at high viscosity ratio, while at high Reynolds number, the influ- ence is less pronounced. In all cases, we show that the thickness of the mixing layer (and thus resuspension) is increased by high viscosity stratification, in particular during the non-linear development of the instability and especially pairing processes. This study suggests that mud viscosity has to be taken into account for resuspension parameterizations because of its impact on the inflec- tion point Reynolds number and the viscosity ratio, which are key parameters for shear instabilities
Ground-based and Polar spacecraft observations of a giant (Pg) pulsation and its associated source mechanism
The emerging landscape of health research based on biobanks linked to electronic health records: Existing resources, statistical challenges, and potential opportunities
Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/154448/1/sim8445_am.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/154448/2/sim8445.pd
Observations of Enhanced Radiation in the kc/s-Band (5 and 8 kc/s) During Auroral and Geomagnetic Disturbances
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