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8/22/2019 Ashby GPS Relativity http://slidepdf.com/reader/full/ashby-gps-relativity 1/35 July 20, 2006 AAPT workshop 1 Relativity in the Global Positioning System Neil Ashby Department of Physics,UCB 390 University of Colorado, Boulder, CO 80309-00390 NIST Affiliate Email: [email protected]

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July 20, 2006 AAPT workshop 1

Relativity in the Global Positioning System

Neil Ashby

Department of Physics,UCB 390

University of Colorado, Boulder, CO 80309-00390

NIST Affiliate

Email: [email protected]

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July 20, 2006 AAPT workshop 2

Fundamental Principles

• Principle of Inertia– The laws of physics are the same in all inertial frames of reference.

• Constancy of the speed of light– The speed of light, c, is a constant independent of the motion of the

source (or of the observer); (it is c in all inertial frames).

• Principle of Equivalence (“weak form”)– Over a small region of space and time, the fictitious gravitational field

induced by acceleration cannot be distinguished from a realgravitational field due to mass.

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July 20, 2006 AAPT workshop 3

Changes in point of view (reference frames)

In studying relativity, one must be willing to adopt different points of view--

that is, different reference frames. The physical phenomena

don’t change, but our description of them does change.

Example 1: the gulf stream curves toward the east as it flows north. For an

observer fixed on the rotating earth, this is due to the “Coriolis force.”

To an observer in a local, freely falling non-rotating frame attachedto earth’s center, this is due to conservation of angular momentum.

Example 2: A pendulum in an accelerating car points backwards. From the

point of view of someone in the car, the force of gravity points slightly

downwards and slightly backwards.

From the point of view of someone on the ground, the pendulum bob

is accelerated forwards by a component of tension in the string that

points slightly forwards and upwards.

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July 20, 2006 AAPT workshop 4

Question.

In an accelerating vehicle, if up is indicated by the direction of the string

that holds down a helium balloon, what direction is “up”?

Up?Up?

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July 20, 2006 AAPT workshop 5

Relativity of Simultaneity

To an observer on the ground, let two lightning

strokes at the front and back of the train

be simultaneous.

The “moving” observer at the train’s midpoint findsthe event at front occurs first.

2'

vxt t 

c≈ −

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July 20, 2006 AAPT workshop 6

Notation--”Lab” and “Moving” Frames

*

Event

In Lab Frame: { t, x ,y, z }

In Moving Frame: { t’, x’, y’, z’ }

 x,x’

 y y’

 z z’

Origins pass by each other at t = t’ = 0.

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July 20, 2006 AAPT workshop 7

Breakdown of simultaneity

In a given inertial frame, it’s OK to take differences of velocities and obtain a

velocity difference greater than c.

Example: Let a rod of length L=x move in the positive x-direction with speed v.

Light emitted at t=0 from the left end of the rod travels to the right end.v

vc 

In Lab, arrival time at the rod end:

2;

( ) (1 / )

 L L L vLt 

c v c v c c c= = +

− −≃

L

In the moving frame:

2 2' ; '

 L vL vxt t t t  

c c c= = − = −

event at t=t’=0

signal propagating with speed c

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July 20, 2006 AAPT workshop 8

Breakdown of simultaneity

 x,x’

 y y’

 z z’ 

*

Event

2'

vxt t 

c−≃

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July 20, 2006 AAPT workshop 9

Relation Between Doppler Effect

and Relativity of Simultaneity

0 2 3 ....... ... x nλ λ λ λ  =

2'

vnt 

c

λ = −

0t =

Wavefronts are marked

simultaneously by the

“non-moving” observer:

Moving observer says the wavefronts are marked differently:

So the wavefront at ( 1) x nλ = =

before it gets into the right position to be marked at t’ = 0. To the moving observer,

the wavelength is:

2

v vc

c c

λ λ =

' (1 ) .v v

c cλ λ λ λ  = + = +

 c

needs to move an additional distance

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July 20, 2006 AAPT workshop 10

Doppler frequency shift

, ln ln ln .c f c f  λ λ = = +

So when lambda increases, the frequency decreases. Taking the

differential of the logarithm function gives

. f v

 f c

λ 

λ 

∆ ∆= − = −

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July 20, 2006 AAPT workshop 11

Equivalence Principle and Gravitational Frequency Shifts

Over a small region of space and time,a fictitious gravity field induced by

acceleration cannot be distinguished

From a gravity field produced by mass.

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July 20, 2006 AAPT workshop 12

Gravitational Frequency Shift

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July 20, 2006 AAPT workshop 13

2 2

2

1

2

 / 

;

.

(1 )2

t L c

gL

v gt  c

 f v gL

 f c c c

 J GM GM  r a f 

 f c

=

= =

∆ ∆Φ= − = − = −

− − − +

∆ = −

Gravitational Frequency Shift

The situation in the rocket is static. The fractional

frequency difference between the clocks is

2.

 f 

 f c

∆ ∆Φ= +

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July 20, 2006 AAPT workshop 14

Frequency shifts due to Gravitational Potential Differences

Let be the gravitational potential on earth’s geoid--at mean sea level,

and r be the radius of a GPS satellite.0Φ

0 E GM 

r ∆Φ = − − Φ

0Φ includes contributions from earth’s oblateness as well as its mass:

0 2

1

1(1 ),

2

GM  J 

a

Φ = − +

where: a1 is the equatorial radius of the earth;

2 .001086 J  ≃ is earth’s quadrupole moment coefficient.

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July 20, 2006 AAPT workshop 15

How big are gravitational frequency shifts in the GPS?

2

1

1( )

 f GM GM 

 f c a a ∆

= − − −

To get a rough estimate, assume the satellite orbit is circular and

the reference clock is on earth’s equator.

where

105 10 ; ( 13km navigation error per day) f 

 f 

−∆× ≈≃

14 3 2

1

3.986 10 m /s ;

26,562km;

6,378km

GM 

a

a

= ×

=

=

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July 20, 2006 AAPT workshop 16

Best IIR Rbs

Navs 51, 54

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July 20, 2006 AAPT workshop 17

Question:

If a clock makes an error in one day of 1 part in 10^14, how far

would light travel in this amount of time?

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July 20, 2006 AAPT workshop 18

Question:

If a clock makes an error in one day of 1 part in 10^14, how far

would light travel in this amount of time?

In one day, the error is:

14 10

10 86400sec 8.64 10 sec.− −

× = ×

In this amount of time, light travels a distance

10 10(8.64 10 sec) 299792458m/sec (8.64 10 sec)

0.26 m

d c− −

= × × = × ×

=

Answer:

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July 20, 2006 AAPT workshop 19

Constancy of c

( ) ,

1,2,3,4

 j jc t t 

 j

= −

=

r - r

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July 20, 2006 AAPT workshop 20

Sample data

20959777.407-8705178.66813799439.29437239.929 346 353 94

3486595.54615908390.24520982631.27037239.

925 307 870 03

-4436309.87516360459.35820450127.56637239.

920 713 391 82

13246718.72118997823.89513004579.64237239.924 422 365 61

Transmitter

Position z i (m)

Transmitter

Position y i (m)

Transmitter

Position x i (m)

Transmission

Epoch t i (s)SV #

Question: Where is the receiver and what is the time at the receiver?

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July 20, 2006 AAPT workshop 21

Reciprocity

( ) j jc t t = −r - r

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July 20, 2006 AAPT workshop 22

The constancy of the speed of light implies time dilation

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July 20, 2006 AAPT workshop 23

Einstein’s Light Clock 

2 2c v−

2 2

2 2

2 2

 /  / ;

1 / 

' / 1 /  

 L ct L c v

v c

t L c v c t  

= − =

= = −

This is just Euclidean geometry and the constancy of c.

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July 20, 2006 AAPT workshop 24

How Big is Time Dilation in the GPS?

22 2

2

211

2

11 / 1 ;2

4000m/s;1

3.5 102

vv cc

vv

c

− ≈ −

=

− = − ×

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July 20, 2006 AAPT workshop 25

Accounting For Relativistic Effects

Example: Time Dilation:

( )

2 2

1/ 22 2

2

2

2

2

path

1 / ;

1 / 

1

1 .2

11

2

d v c dt  

dt v c d  

v

d c

vt d 

c

τ  

τ  

τ  

τ  

= −

= −

+

∆ = +

Elapsed Coordinate time:

Observed Proper Time

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July 20, 2006 AAPT workshop 26

GPS Satellite in a circular earth-bound orbit

3;

GmM m

− =r rɺɺ

Newton’s law of motion: Force toward the earth is gravitational.

The mass of the satellite cancels out (a consequence of the

Principle of Equivalence). The orbit is nearly a Kepler ellipse.

Solution of the above equation shows that the energy is constant:

21

2 2

GM GM  v

r a− = −

where a is the semimajor axis.

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July 20, 2006 AAPT workshop 27

Frequency shift of GPS satellite clocks

relative to reference clock on equator

( )22

10

2 2 2

1 1

2 2

 E a f v

 f c c c

ω  Φ − Φ∆= − − −

( )2

2 12

1

10

2

31 1 1 12 (1 / 2)

2 22 1 1

4.4647 10 .

 E E  E E 

 E 

GM GM   f GM J a

 f c a r a aGM 

c a r 

ω 

∆ = − − − + + +

= − − + ×

Putting in everything that is known about these quantities and addingand subtracting some terms,

The first term depends on orbital eccentricity and gives rise to a periodic timeerror that is ( E is the eccentric anomaly)

2

2sin( ) .

rel E  

et GM a E const  

c∆ = − +

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July 20, 2006 AAPT workshop 28

Clocks on earth’s geoid beat at equal rates

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July 20, 2006 AAPT workshop 29

Orbit adjustments in GPS

2 2

3 3;

2 2

 E E GM GM   f a

 f c a c a a

δ δ   ∆ = ∆ − =

For an increase in altitude of 20 km, the change in frequency is

131.88 10 . f  f 

δ   −∆ ×≃

This effect is now understood and the clock frequency is adjustedwhen the orbit is changed. (Back-of-the-envelope calculation!)

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July 20, 2006 AAPT workshop 30

END

Further development--introduce the metric

2 2 2 2 2

2

2(1 )( ) ;ds c dt dx dy dz

c

Φ= − + + + +

Discuss proper time, coordinate time; show how the effects can be

obtained from the metric…..

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July 20, 2006 AAPT workshop 31

Sagnac effect

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July 20, 2006 AAPT workshop 32

Sagnac Effect on Synchronization

in a Rotating System

Sagnac Correction =2

2 z A

c

ω 

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July 20, 2006 AAPT workshop 33

Principle of Equivalence

V

V+∆∆∆∆V

Acceleration

Local Inertial

Frame

r

2

2 2

22

2

2 2 2

Induced potential difference/c ;

Gravitational potential difference/c ;

1Net potential difference/c = 0;

c Tc

c

c T c c

∆= =

∇Φ=

+ ∇Φ ∆ ∇Φ= + =

A r V r

r

A r r V r r

i i

i

i i i i

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July 20, 2006 AAPT workshop 34

Common-view time transfer

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July 20, 2006 AAPT workshop 35

Why are atomic clocks needed?

To reduce the effect of clock error to < 2 meters,

the clock error must be less than 2/c = 6.7 x 10-9 sec.

Half a day = 43200 seconds, so the fractional clock

error must be less than:

(2 m)/(43200 s x c) = 1.5 x 10-13.

Only atomic clocks can achieve such stability.