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ASEN 5070 Statistical Orbit determination I Fall 2012 Professor George H. Born

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ASEN 5070 Statistical Orbit determination I Fall 2012 Professor George H. Born Professor Jeffrey S. Parker Lecture 8: Stat OD Processes. Announcements. Homework 1 Graded Comments included on D2L Any questions, talk with us this week Homework 2 CAETE due Today Graded soon after - PowerPoint PPT Presentation
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CCAR Colorado Center for Astrodynamics Research University of Colorado Boulder ASEN 5070 Statistical Orbit determination I Fall 2012 Professor George H. Born Professor Jeffrey S. Parker Lecture 8: Stat OD Processes 1
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Page 1: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 1

ASEN 5070Statistical Orbit determination I

Fall 2012

Professor George H. BornProfessor Jeffrey S. Parker

Lecture 8: Stat OD Processes

Page 2: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 2

Homework 1 Graded◦ Comments included on D2L◦ Any questions, talk with us this week

Homework 2 CAETE due Today◦ Graded soon after

Homework 3 due Today

Homework 4 due next week

Announcements

Page 3: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 3

A few questions on Problem 4’s Laplace Transform.

There’s one Transform missing from the table:

Note: This has been posted in the HW3 discussions on D2L for a few days now. Check there if you have a commonly-asked question!

Homework 3

Page 4: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 4

What does the joint density function MEAN?

Page 5: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 5

Quiz Results

Page 6: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 6

Quiz Results

Page 7: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 7

Quiz Results

Page 8: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 8

Quiz Results

Page 9: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 9

Quiz Results

Page 10: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 10

Quiz Results

Page 11: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 11

Quiz Results

Page 12: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 12

Quiz Results

Page 13: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 13

Truth Reference Best Estimate

Observations are functions of state parameters, but usually NOT state parameters.

Mismodeled dynamics

Underdetermined system.

Stat OD in a Nutshell

Page 14: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 14

We have noisy observations of certain aspects of the system.

We need some way to relate each observation to the trajectory that we’re estimating.

Stat OD in a Nutshell

Observed RangeComputed Range

True Range = ???

X*

Page 15: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 15

We have noisy observations of certain aspects of the system.

We need some way to relate each observation to the trajectory that we’re estimating.

Stat OD in a Nutshell

Observed RangeComputed Range

True Range = ???ε = O-C = “Residual”

X*

Page 16: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 16

Assumptions:

◦ The reference/nominal trajectory is near the truth trajectory. Linear approximations are decent

◦ Force models are good approximations for the duration of the measurement arc.

◦ The filter that we’re using is unbiased: The filter’s best estimate is consistent with the true

trajectory.

Stat OD in a Nutshell

Page 17: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 17

How do we best fit the data?

Fitting the data

Residuals = ε = O-C

Page 18: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 18

How do we best fit the data?

Fitting the data

Residuals = ε = O-C

Page 19: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 19

How do we best fit the data?

Fitting the data

Residuals = ε = O-C

No

Page 20: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 20

How do we best fit the data?

Fitting the data

Residuals = ε = O-C

No

No

Page 21: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 21

How do we best fit the data?

Fitting the data

Residuals = ε = O-C

No

No

Not bad

Page 22: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 22

How do we best fit the data?

Fitting the data

Residuals = ε = O-C

No

No

Not bad

Page 23: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 23

How do we best fit the data?

A good solution, and one easy to code up, is the least-squares solution

Fitting the data

Page 24: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 24

How do we map an observation to the trajectory?

Mapping an observation

Observed RangeComputed Range

ε = O-C = “Residual”

X*

Page 25: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 25

How do we map an observation to the trajectory?

Mapping an observation

Page 26: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 26

How do we map an observation to the trajectory?

Very non-linear relationships! Need to linearize to make a practical

algorithm.

Mapping an observation

Page 27: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 27

Linearization Introduce the state deviation vector

If the reference/nominal trajectory is close to the truth trajectory, then a linear approximation is reasonable.

State Deviation and Linearization

Page 28: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 28

Goal of the Stat OD process:

Find a new state/trajectory that best fits the observations:

If the reference is near the truth, then we can assume:

State Deviation and Linearization

Page 29: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 29

Goal of the Stat OD process:

The best fit trajectory

is represented by

State Deviation and Linearization

This is what we want

Page 30: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 30

How do we map the state deviation vector from one time to another?

State Deviation Mapping

X*

Page 31: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 31

How do we map the state deviation vector from one time to another?

The state transition matrix.

State Deviation Mapping

Page 32: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 32

How do we map the state deviation vector from one time to another?

The state transition matrix.

It permits:

State Deviation Mapping

Page 33: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 33

The state transition matrix maps a deviation in the state from one epoch to another.

It is constructed via numerical integration, in parallel with the trajectory itself.

State Transition Matrix

Page 34: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 34

The “A” Matrix:

The A Matrix

Page 35: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 35

Still need to know how to map measurements from one time to a state at another time!

Measurement Mapping

Page 36: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 36

Still need to know how to map measurements from one time to a state at another time!

Would like this:

Measurement Mapping

Page 37: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 37

Still need to know how to map measurements from one time to a state at another time!

Measurement Mapping

Page 38: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 38

Still need to know how to map measurements from one time to a state at another time!

Define:

Measurement Mapping

Page 39: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 39

The Mapping Matrix

Measurement Mapping Matrix

Page 40: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 40

Now we can map an observation to the state at an epoch.

Mapping an observation

Observed RangeComputed Range

ε = O-C = “Residual”

X*

Page 41: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

We have the method of least squares

How do we solve the problem?

Page 42: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

We have the method of least squares

How do we solve the problem?

Page 43: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

We have the method of least squares

How do we solve the problem?

Page 44: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

We have the method of least squares

How do we solve the problem?

Page 45: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 45

Example 4.2.1

Page 46: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

Example 4.2.1

Or in component form:

Expressed in first order form:

Page 47: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

Example 4.2.1

Page 48: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

Example 4.2.1

Page 49: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder

Example 4.2.1

Page 50: ASEN 5070 Statistical Orbit determination I Fall  2012 Professor George H.  Born

CCARColorado Center for

Astrodynamics Research

University of ColoradoBoulder 50

Homework 1 Graded◦ Comments included on D2L◦ Any questions, talk with us this week

Homework 2 CAETE due Today◦ Graded soon after

Homework 3 due Today

Homework 4 due next week

Announcements


Recommended