We study the internal waves as the evolution of the interface between two immiscible, inviscid, incompressible, irrotational fluids of different density in three dimensions. Motion of the interface and fluids is driven by the action of gravity, surface tension, and/or a prescribed far-field pressure gradient. The model includes derived equations for the evolution of the interface and surfaces density. Presence of the surface tension introduces high order derivatives into the evolution equations. This makes the considered problem stiff and the application of the standard explicit time-integration methods suffers strong time-step stability constraints.
Our proposed numerical method employes a special interface parameterization that enables the use of implicit time-integration methods via a small-scale decomposition. This approach allows us to capture the nonlinear growth of normal modes for the case of Rayleigh-Taylor instability with the heavier fluid on the top. In addition, in the given test problem with the prescribed initial disturbance to a flat interface under an action of the surface tension dominating the gravity, the surface relaxes to a flat interface. Linear stability analysis is performed and the numerical results are validated by comparison to the obtained analytic solution of the linearized problem for a short time. The developed model and numerical method can be efficiently applied to study the motion of internal waves for doubly periodic interfacial flows with surface tension.
We study the internal waves as the evolution of the interface between two immiscible, inviscid, incompressible, irrotational fluids of different density in three dimensions. Motion of the interface and fluids is driven by the action of gravity, surface tension, and/or a prescribed far-field pressure gradient. The model includes derived equations for the evolution of the interface and surfaces density. Presence of the surface tension introduces high order derivatives into the evolution equations. This makes the considered problem stiff and the application of the standard explicit time-integration methods suffers strong time-step stability constraints.
Our proposed numerical method employes a special interface parameterization that enables the use of implicit time-integration methods via a small-scale decomposition. This approach allows us to capture the nonlinear growth of normal modes for the case of Rayleigh-Taylor instability with the heavier fluid on the top. In addition, in the given test problem with the prescribed initial disturbance to a flat interface under an action of the surface tension dominating the gravity, the surface relaxes to a flat interface. Linear stability analysis is performed and the numerical results are validated by comparison to the obtained analytic solution of the linearized problem for a short time. The developed model and numerical method can be efficiently applied to study the motion of internal waves for doubly periodic interfacial flows with surface tension.
Model Selection with Piecewise Regular GaugesGabriel Peyré
Talk given at Sampta 2013.
The corresponding paper is :
Model Selection with Piecewise Regular Gauges (S. Vaiter, M. Golbabaee, J. Fadili, G. Peyré), Technical report, Preprint hal-00842603, 2013.
http://hal.archives-ouvertes.fr/hal-00842603/
Integration is a part of Calculus.
This is just a short presentation on Integration.
It may help you out to complete your academic presentation.
Thank You
Efficient Analysis of high-dimensional data in tensor formatsAlexander Litvinenko
We solve a PDE with uncertain coefficients. The solution is approximated in the Karhunen Loeve/PCE basis. How to compute maximum ? frequency? probability density function? with almost linear complexity? We offer various methods.
We have implemented a multiple precision ODE solver based on high-order fully implicit Runge-Kutta(IRK) methods. This ODE solver uses any order Gauss type formulas, and can be accelerated by using (1) MPFR as multiple precision floating-point arithmetic library, (2) real tridiagonalization supported in SPARK3, of linear equations to be solved in simplified Newton method as inner iteration, (3) mixed precision iterative refinement method\cite{mixed_prec_iterative_ref}, (4) parallelization with OpenMP, and (5) embedded formulas for IRK methods. In this talk, we describe the reason why we adopt such accelerations, and show the efficiency of the ODE solver through numerical experiments such as Kuramoto-Sivashinsky equation.
Model Selection with Piecewise Regular GaugesGabriel Peyré
Talk given at Sampta 2013.
The corresponding paper is :
Model Selection with Piecewise Regular Gauges (S. Vaiter, M. Golbabaee, J. Fadili, G. Peyré), Technical report, Preprint hal-00842603, 2013.
http://hal.archives-ouvertes.fr/hal-00842603/
Integration is a part of Calculus.
This is just a short presentation on Integration.
It may help you out to complete your academic presentation.
Thank You
Efficient Analysis of high-dimensional data in tensor formatsAlexander Litvinenko
We solve a PDE with uncertain coefficients. The solution is approximated in the Karhunen Loeve/PCE basis. How to compute maximum ? frequency? probability density function? with almost linear complexity? We offer various methods.
We have implemented a multiple precision ODE solver based on high-order fully implicit Runge-Kutta(IRK) methods. This ODE solver uses any order Gauss type formulas, and can be accelerated by using (1) MPFR as multiple precision floating-point arithmetic library, (2) real tridiagonalization supported in SPARK3, of linear equations to be solved in simplified Newton method as inner iteration, (3) mixed precision iterative refinement method\cite{mixed_prec_iterative_ref}, (4) parallelization with OpenMP, and (5) embedded formulas for IRK methods. In this talk, we describe the reason why we adopt such accelerations, and show the efficiency of the ODE solver through numerical experiments such as Kuramoto-Sivashinsky equation.
Response Surface in Tensor Train format for Uncertainty QuantificationAlexander Litvinenko
We apply low-rank Tensor Train format to solve PDEs with uncertain coefficients. First, we approximate uncertain permeability coefficient in TT format, then the operator and then apply iterations to solve stochastic Galerkin system.
Robust Control of Uncertain Switched Linear Systems based on Stochastic Reach...Leo Asselborn
This presentation proposes an approach to algorithmically synthesize control strategies for
set-to-set transitions of uncertain discrete-time switched linear systems based on a combination
of tree search and reachable set computations in a stochastic setting. For given Gaussian
distributions of the initial states and disturbances, state sets wich are reachable to a chosen
confidence level under the effect of time-variant hybrid control laws are computed by using
principles of the ellipsoidal calculus. The proposed algorithm iterates over sequences of the
discrete states and LMI-constrained semi-definite programming (SDP) problems to compute
stabilizing controllers, while polytopic input constraints are considered. An example for illustration is included.
We study an elliptic eigenvalue problem, with a random coefficient that can be parametrised by infinitely-many stochastic parameters. The physical motivation is the criticality problem for a nuclear reactor: in steady state the fission reaction can be modeled by an elliptic eigenvalue
problem, and the smallest eigenvalue provides a measure of how close the reaction is to equilibrium -- in terms of production/absorption of neutrons. The coefficients are allowed to be random to model the uncertainty of the composition of materials inside the reactor, e.g., the
control rods, reactor structure, fuel rods etc.
The randomness in the coefficient also results in randomness in the eigenvalues and corresponding eigenfunctions. As such, our quantity of interest is the expected value, with
respect to the stochastic parameters, of the smallest eigenvalue, which we formulate as an integral over the infinite-dimensional parameter domain. Our approximation involves three steps: truncating the stochastic dimension, discretizing the spatial domain using finite elements and approximating the now finite but still high-dimensional integral.
To approximate the high-dimensional integral we use quasi-Monte Carlo (QMC) methods. These are deterministic or quasi-random quadrature rules that can be proven to be very efficient for the numerical integration of certain classes of high-dimensional functions. QMC methods have previously been applied to linear functionals of the solution of a similar elliptic source problem; however, because of the nonlinearity of eigenvalues the existing analysis of the integration error
does not hold in our case.
We show that the minimal eigenvalue belongs to the spaces required for QMC theory, outline the approximation algorithm and provide numerical results.
Control of Discrete-Time Piecewise Affine Probabilistic Systems using Reachab...Leo Asselborn
This presentation proposes an algorithmic approach to
synthesize stabilizing control laws for discrete-time piecewise
affine probabilistic (PWAP) systems based on computations of
probabilistic reachable sets. The considered class of systems
contains probabilistic components (with Gaussian distribution)
modeling additive disturbances and state initialization. The
probabilistic reachable state sets contain all states that are
reachable with a given confidence level under the effect of
time-variant control laws. The control synthesis uses principles
of the ellipsoidal calculus, and it considers that the system
parametrization depends on the partition of the state space. The
proposed algorithm uses LMI-constrained semi-definite programming
(SDP) problems to compute stabilizing controllers,
while polytopic input constraints and transitions between regions
of the state space are considered. The formulation of
the SDP is adopted from a previous work in [1] for switched
systems, in which the switching of the continuous dynamics
is triggered by a discrete input variable. Here, as opposed
to [1], the switching occurs autonomously and an algorithmic
procedure is suggested to synthesis a stabilizing controller. An
example for illustration is included.
Probabilistic Control of Uncertain Linear Systems Using Stochastic ReachabilityLeo Asselborn
This presentation proposes an approach to algorithmically synthesize control strategies for
set-to-set transitions of discrete-time uncertain systems based on reachable set computations in
a stochastic setting. For given Gaussian distributions of the initial states and disturbances, state
sets wich are reachable to a chosen confidence level under the effect of time-variant control laws
are computed by using principles of the ellipsoidal calculus. The proposed algorithm iterates over
LMI-constrained semi-definite programming problems to compute probabilistically stabilizing
controllers, while ellipsoidal input constraints are considered. An example for illustration is included.
constant strain triangular which is used in analysis of triangular in finite element method with the help of shape function and natural coordinate system.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...Ana Luísa Pinho
Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
In silico drugs analogue design: novobiocin analogues.pptx
cheb_conf_aksenov.pdf
1. Acquiring elastic properties of thin composite
structure from vibrational testing data
P. Chebyshev Mathematical Ideas and Their Applications to
Natural Sciences International Conference
V. Aksenov, A. Vasyukov, K. Beklemysheva
May 15, 2021
Moscow Institute of Physics and Technology
4. Problem overview
Figure 1: Example of the vibrational
testing stand
• Setup:
• Non-destructive testing of
thin composite structures
• Amplitutde-frequency
characteristic is measured
• Motivation:
• Lack of reliable data from
the manufacturers
• Elastic properties may
change during production
• Effective model with coarser
geometry
2
5. Governing equations
The model describes linear anisotropic elastic medium with viscous
damping. The transient load with constant frequency is applied on the
border
ρwtt + γ0wt − (D66wxx + D55wyy ) = 0 (x, y) ∈ G
w(x, y, t) = g(x, y) · eiωt
(x, y) ∈ ΓD
σn = (D66wx nx + D55wy ny ) = 0 (x, y) ∈ ΓN (ΓN ∪ ΓD = ∂G)
Variables
• w(x, y, t) – displacement in normal direction
• ρ – known density
• θ = (γ0, D55, D66) – unknown parameters
3
6. Governing equations
w = wpart +
∞
X
i=0
Ci wi
We suggest that due to damping, the terms describing free vibrations
fade exponentially, thus only consider the term
wpart = u(x, y) · eiωt
We arrive at the BVP for u:
(−ρω2
+ iγ0ω)u − (D66uxx + D55uyy ) = 0 (x, y) ∈ G
(1.1)
u(x, y) = g(x, y) (x, y) ∈ ΓD
(1.2)
σn = (D66ux nx + D55uy ny ) = 0 (x, y) ∈ ΓN (ΓN ∪ ΓD = ∂G)
(1.3)
4
8. FEM formulation of the direct problem
Equivalent form of the equation (1.1)
cω
Z
G
uv d x d y + D66
Z
G
ux vx d x d y + D55
Z
G
uy vy d x d y =
=
Z
ΓD
vσn d Γ +
Z
ΓN
vσn d Γ
for arbitrary continous function v(x, y). We solve it approximately with
Finite Element method on a triangular grid
u =
X
i∈I
ui hi +
X
k∈D
gk hk , v ∈ {hi , i ∈ I}
where hi are 1-st degree basis polynomials, hi (xi ) = 1, D – grid vertices
on ΓD, I – all other vertices, gk = g(xk , yk )
5
9. FEM formulation of the direct problem
Numerical solution of the direct problem
K̃(ω, θ)u = ˜
f (ω, θ) (2.1)
K̃(ω, θ) = cωK0 + D66Kx + D55Ky
[K0]ij =
Z
G
hi hj d x d y
[Kx ]ij =
Z
G
hi,x hj,x d x d y
[Ky ]ij =
Z
G
hi,y hj,y d x d y
˜
f (ω, θ) = cωf0 + D66fx + D55fy
[f0]i = −
X
k∈D
gk
Z
G
hi hk d x d y
[fx ]i = −
X
k∈D
gk
Z
G
hi,x hk,x d x d y
[fy ]i = −
X
k∈D
gk
Z
G
hi,y hk,y d x d y
cω = −ρω2
+ iγ0ω
6
10. Inverse problem
In the experiment, the amplitude u is sampled at a test point (xt, yt) for
different frequencies ωk . Thus we obtain the amplitude-frequency
characteristic uexp(ωk )
Figure 2: Sample AFC
The goal is to obtain values of the parameters from these data 7
11. Inverse problem
We propose the following optimization problem:
min
θ
L(θ) =
Nω
X
k=1
k[u(θ, ωk )]t − uexp(ωk )k
2
(2.2)
s.t. θi > 0
Here u(θ, ωk ) is the solution of K̃(θ, ωk )u = ˜
f (θ, ωk )
The evaluation of L(θ) requires only standard linear algebra, thus we can
use fast automatic differentiation to obtain derivatives efficiently
8
12. Trust-region method
Trust-region subproblem
pk = arg min
p
fk + gT
k p +
1
2
pT
Bk p (2.3)
s.t. kpk k ≤ ∆k
(fk = f (xk ), gk = ∇f (xk ))
Newton-Gauss method:
Bk = ∇2
f (xk )
BFGS:
y = gk+1 − gk
s = xk+1 − xk
Bk+1 = Bk +
yyT
sT y
−
sT
BT
k Bk s
sT Bk s
9
13. Trust-region method
Algorithm 1 Trust-region method
Require: x0 — initial guess, ∆max > 0, ∆0 ∈ (0, ∆max ), η ∈ [0, 1
4
)
1: repeat
2: Evaluate pk as the solution of (2.3)
3: ρk = f (xk )−f (xk +pk )
mk (0)−mk (pk )
{relative improvement}
4: if ρk < 1
4
then
5: ∆k+1 = 1
4
∆k
6: else
7: if ρk > 3
4
and kpk k = ∆k then
8: ∆k+1 = min(2∆k , ∆max )
9: else
10: ∆k+1 = ∆k
11: if ρk > η then
12: xk+1 = xk + pk
13: Update the quadratic model
14: else
15: xk+1 = xk
16: until checkStopCondition() or k ≥ kmax 10
15. Setup
(a) (b)
Figure 3: Two experimental geometries, used for calculations
• Simple geometry, ∼ 300 vertices, 201 frequencies
• Reference AFC is evaluated for some θbase. Initial guess θ0 with
every value about 30% different 11
21. Discussion of the results
Results:
• Possibility to use both first
and second order methods
• Code is just-in-time compiled
for GPU
• Fast convergence achieved for
a rather decent perturbation
(30%)
Problems:
• Global convergence only to
local minimum, which are
possibly multiple
• Convergence in D55 is by
order of magnitude worse
• Geometries with larger
number of DOF might
exhaust GPU memory
17
22. Thank you for your attention!
aksenov.vv@phystech.edu
17