Almost Invariant Sets and Transport in the Solar System

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University of Paderborn Applied Mathematics Michael Dellnitz Department of Mathematics University of Paderborn Almost Invariant Sets and Transport in the Solar System

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Almost Invariant Sets and Transport in the Solar System. Michael Dellnitz Department of Mathematics University of Paderborn. Overview. invariant sets (mission design; zero finding). statistics (molecular dynamics; transport problems). GAIO. invariant manifolds. global attractors. - PowerPoint PPT Presentation

Transcript of Almost Invariant Sets and Transport in the Solar System

Page 1: Almost Invariant Sets and Transport in the Solar System

University of Paderborn

Applied Mathematics

Michael DellnitzDepartment of Mathematics

University of Paderborn

Almost Invariant Sets andTransport in the Solar System

Page 2: Almost Invariant Sets and Transport in the Solar System

University of Paderborn

Applied Mathematics

Overview

almost invariant sets

invariant measures

global attractorsinvariant manifolds

invariant sets(mission design; zero finding)

statistics(molecular dynamics;transport problems)

set orientednumerical

methods

Page 3: Almost Invariant Sets and Transport in the Solar System

University of Paderborn

Applied Mathematics

Simulation of Chua´s Circuit

yz

zyxy

xm

xmyx

)3

( 310

Page 4: Almost Invariant Sets and Transport in the Solar System

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Numerical Strategy

1. Approximation of the invariant set A

2. Approximation of the dynamical behavior on A

A

Page 5: Almost Invariant Sets and Transport in the Solar System

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The Multilevel Approachfor the Lorenz System

Page 6: Almost Invariant Sets and Transport in the Solar System

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Relative Global Attractors

nnjj RRfxfx :),(1

define compact For nRQ

0

)(

j

jQ QfA

Relative Global Attractor

.QAQ inside sets invariant the all contains

Page 7: Almost Invariant Sets and Transport in the Solar System

University of Paderborn

Applied Mathematics

The Subdivision Algorithm

. covering boxes

of collection a be Let

Q

k

A

C 1

Subdivision

).diam( )diam( and

that such Construct

ˆ

ˆ

1

kkCBCB

k

CCBB

C

kk

Selection Set

BBfCBCBC kkkˆ)(ˆˆ:ˆ 1 s.t.

Page 8: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Example: Hénon Map

parameters and babxyaxyxf ),,1(),( 2

Page 9: Almost Invariant Sets and Transport in the Solar System

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distance Hausdorff the

Then Define

),(

.

h

BQkCB

k

0),(lim kQ

kQAh

A Convergence Result

Proposition [D.-Hohmann 1997]:

Remark:

Results on the speed of convergence can be obtained if possesses a hyperbolic structure.QA

Page 10: Almost Invariant Sets and Transport in the Solar System

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Realization of the Subdivision Step

},,1:{),( nircyRyrcR iiin for

Boxes are indeed boxes

Subdivision by bisection

Data structure

Page 11: Almost Invariant Sets and Transport in the Solar System

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Realization of the Selection Step

Standard choice of test points:

• For low dimensions: equidistant distribution on edges of boxes.• For higher dimensions: stochastic distribution inside the boxes.

.,)(1 jiBBf ji whethercheck to have We

Use test points:

? points test all for ji ByByf )(

Page 12: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Global Attractor in Chua´s Circuit

Page 13: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Subdivision

Simulation

Global Attractor in Chua´s Circuit

Page 14: Almost Invariant Sets and Transport in the Solar System

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Invariant Manifolds

. i.e. , of point fixed a be Let ppffp )(

jpxfxpW

jpxfxpWju

js

for

for

)(:)(

)(:)(

Stable and unstable manifold of p

)( pW s

)( pW u

p

Page 15: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Example: Pendulum

Page 16: Almost Invariant Sets and Transport in the Solar System

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Computing Local Invariant Manifolds

Idea:

)( pWA

pN

ulocN

of odneighborho small a for

Let p be a hyperbolic fixed point

N

p )( pW uAN

Page 17: Almost Invariant Sets and Transport in the Solar System

University of Paderborn

Applied MathematicsInitializationSubdivisionContinuation 1Continuation 2Continuation 3

Covering of an Unstable Manifold for a Fixed Point of the Hénon Map

Page 18: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Discussion

• The algorithm is in principle applicable to manifolds of arbitrary dimension.

• The numerical effort essentially depends on the dimension of the invariant manifold (and not on the dimension of state space).

• The algorithm works for general invariant sets.

Page 19: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

GENESIS Trajectory

Page 20: Almost Invariant Sets and Transport in the Solar System

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Invariant Manifolds

Stable manifold

Unstable manifold

Halo orbit

Page 21: Almost Invariant Sets and Transport in the Solar System

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Earth

Halo orbit

Unstable Manifoldof the Halo Orbit

Page 22: Almost Invariant Sets and Transport in the Solar System

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Unstable Manifoldof the Halo Orbit

Flight along the manifold

Computation with GAIO, University of Paderborn

Page 23: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

)(

))((

)(1

l

lkkl

kld

Bm

BBfmp

pP

with chain Markov eApproximat

Invariant Measures:Discretization of the Problem

Galerkin approximation using the functions

dihiBi ,,1

dBB ,,1 coveringBox

)stochastic measure; Lebesgue ( dPm

Page 24: Almost Invariant Sets and Transport in the Solar System

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Invariant Measure for Chua´s Circuit

Computation by GAIO; visualization with GRAPE

Page 25: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Invariant Measurefor the Lorenz System

Page 26: Almost Invariant Sets and Transport in the Solar System

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Typical Spectrum of the Markov Chain

Invariant measure

„Almost invariant set“

We consider the simplest situation...

Page 27: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Analyzing Maps with IsolatedEigenvalues (D.-Froyland-Sertl 2000)

Page 28: Almost Invariant Sets and Transport in the Solar System

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At the Other End

This map has norelevant eigenvalue

except for theeigenvalue 1

(using a result fromBaladi 1995).

Let‘s pick amap between

the two extremes

Page 29: Almost Invariant Sets and Transport in the Solar System

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A Map with a Nontrivialrelevant Eigenvalue

This map has arelevant eigenvalue

of modulus less than one.

Essential spectrumof continuous problem

(Keller ´84)

Page 30: Almost Invariant Sets and Transport in the Solar System

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Corresponding Eigenfunctions

Eigenfunction forthe eigenvalue 1

Eigenfunction forthe eigenvalue < 1

positive on (0,0.5) andnegative on (0.5,1)

Page 31: Almost Invariant Sets and Transport in the Solar System

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Almost Invariant Sets

and if measure the to respect

withinvariant almost- is :Definition

).())((

0)(

1 AAAf

A

XA

.

1

MP

PP d

for

that such operator transfer

the of eigenvalue an be letNow

Page 32: Almost Invariant Sets and Transport in the Solar System

University of Paderborn

Applied Mathematics

Almost Invariance and Eigenvalues

. to respect withinvariant almost- is if

Then withset a be Let

A

AXA

2

1

.5.0)(

Proposition:

Page 33: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Example

796.02/)592.01(]5.0,0[ and A

Second eigenfunction of the 1D-map:

Page 34: Almost Invariant Sets and Transport in the Solar System

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Almost Invariant Setsin Chua´s Circuit

Computation by GAIO; Visualization with GRAPE

Page 35: Almost Invariant Sets and Transport in the Solar System

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Transport in the Solar System(Computations by Hessel, 2002)

Idea: Concatenate the CR3BPs for

• Neptune• Uranus• Saturn• Jupiter• Mars

and compute the probabilities for transitionsthrough the planet regions.

Page 36: Almost Invariant Sets and Transport in the Solar System

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Spectrum for Jupiter

Detemine the secondlargest real positiveeigenvalue:

Page 37: Almost Invariant Sets and Transport in the Solar System

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Transport for Jupiter

Eigenvalue: 0.9998

Eigenvalue: 0.9982

Page 38: Almost Invariant Sets and Transport in the Solar System

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Transport for Neptune

Eigenvalue: 0.999947

Page 39: Almost Invariant Sets and Transport in the Solar System

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Quantitative Results

For the Jacobian constant C = 3.004 we obtain for the probability to pass each planet within ten years:

• Neptune: 0.0002• Uranus: 0.0003• Saturn: 0.011• Jupiter: 0.074

Page 40: Almost Invariant Sets and Transport in the Solar System

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Using the Underlying Graph(Froyland-D. 2001, D.-Preis 2001)

Boxes are verticesCoarse dynamics represented by edges

Use graph theoretic algorithms incombination with the multilevel structure

Page 41: Almost Invariant Sets and Transport in the Solar System

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Applied Mathematics

Using Graph Partitioningfor Jupiter (Preis 2001–)

Green – green: 0.9997Red – red: 0.9997

Yellow – yellow: 0.8733

Green – yellow: 0.065Red – yellow: 0.062

T: approx. 58 days

Page 42: Almost Invariant Sets and Transport in the Solar System

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4BP for Jupiter / Saturn

Invariant measure

Page 43: Almost Invariant Sets and Transport in the Solar System

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4BP for Jupiter / Saturn

Almost invariant sets

Page 44: Almost Invariant Sets and Transport in the Solar System

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4BP for Saturn / Uranus

Almost invariant sets

Page 45: Almost Invariant Sets and Transport in the Solar System

University of Paderborn

Applied Mathematics

Contact

http://www.upb.de/math/~agdellnitz

Papers and software at