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    “Global” Global PositioningSystem Measurements

    Prof. Thomas HerringDepartment of Earth, Atmosphere and

    Planetary Sciences

    http://www-gpsg.mit.edu/~tah

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    Overview

    • Review of the development of the GPS

    system and basics of its use and operation

    • Selected regional applications

    • Character of global measurements

    • Origin of systematic effects in global results

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    GPS Original Design

    • Started development in the late 1960s as

    NAVY/USAF project to replace Doppler

    positioning system• Aim: Real-time positioning to < 10 meters,

    capable of being used on fast moving

    vehicles.• Limit civilian (“non-authorized”) users to

    100 meter positioning.

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    GPS Design

    • Innovations:

    – Use multiple satellites (originally 21, now ~28)

    – All satellites transmit at same frequency– Signals encoded with unique “bi-phase, quadrature

    code” generated by pseudo-random sequence

    (designated by PRN, PR number): Spread-spectrum

    transmission.– Dual frequency band transmission:

    • L1 ~1.575 GHz, L2 ~1.227 GHz

    • Corresponding wavelengths are 190 mm and 244 mm

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    Latest Block IIR satellite

    (1,100 kg)° Transmission array is

    made up of 12 helical

    antenna in two rings of43.8 cm (8 antennas) and

    16,2 cm (4 antennas) radii

    ° Total diameter is 87 cm

    ° Solar panels lead to

    large solar radiation

    pressure effects.

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    Measurements

    • Measurements:– Time difference between signal transmission from

    satellite and its arrival at ground station (called“pseudo-range”, precise to 0.1–10 m)

    – Carrier phase difference between transmitter andreceiver (precise to a few millimeters) but initial valuesunknown (ie., measures change in range to satellites).

    – In some case, the integer values of the initial phaseambiguities can be determined (bias fixing)

    • All measurements relative to “clocks” in groundreceiver and satellites (potentially posesproblems).

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    Measurement usage

    • “Spread-spectrum” transmission: Multiple

    satellites can be measured at same time.

    • Since measurements can be made at same

    time, ground receiver clock error can be

    determined (along with position).

    • Signal

     

    V (t ,   x)=V osin[2π ( ft − k.   x)+πC(t )]

    C(t ) is code of zeros and ones (bi

    Varies discretely at 1.023 or 10.

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    Measurements

    • Since the C(t) code changes the sign of the

    signal, satellite can be only be detected if the

    code is known (PRN code)• Multiple satellites can be separated by

    “correlating” with different codes (only the

    correct code will produce a signal)• The time delay of the code is the pseudo-

    range measurement.

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    Position

    Determination(perfect

    clocks).

    • Three satellites

    are needed for 3-D

    position with

    perfect clocks.

    • Two satellites

    are OK if height is

    known)

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    Positiondetermination:

    with clock

    errors: 2-D case• Receiver clock is

    fast in this case, so

    all pseudo-ranges are

    short

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    Positioning

    • For pseudo-range to be used for positioningneed:

    – Knowledge of errors in satellite clocks

    – Knowledge of positions of satellites

    • This information is transmitted by satellite

    in “broadcast ephemeris”

    • “Differential” positioning (DGPS)eliminates need for accurate satellite clock

    knowledge.

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    GPS Security systems

    • Selective availability (SA) is no longer active butprior to 2000 “denied” civilian accuracy better

    than 100 m• Antispoofing (AS) active since 1992, addsadditional encryption to P-code on L1 and L2.

    • Makes civilian GPS receivers more expensive and

    more sensitive to radio interference• Impact of AS and SA small on results presented

    here.

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    Satellite constellation

    • Since multiple satellites need to be seen at

    same time (four or more):

    – Many satellites (original 21 but now 28)

    – High altitude so that large portion of Earth can

    be seen (20,000 km altitude —MEO)

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    Current constellation

    • Relative sizes

    correct (inertial

    space view)

    • “Fuzzy” linesnot due to orbit

    perturbations,

    but due to

    satellites beingin 6-planes at

    55o inclination.

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    Global GPS analysis• GPS phase measurements at L1 and L2 from a global

    distribution of station used

    • Analysis here is “un-constrained”

    – All site positions estimated– Atmospheric delay parameters estimated

    – “Real” bias parameters for each satellite global, integervalues for regional site combinations (

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    Global GPS analysis

    • Data used between 1992-2001

    • Full analysis has ~600 stations (analysis

    here restricted to ~100 sites that have morethan 5 years of data

    • Large density of sites (~300) in California

    • Total data set has > 2 billion phasemeasurements

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    GPS Antennas (for precise positioning)

    • Rings are

    called

    choke-rings

    (used to

    suppressmulti-path)

    Nearly all antennas are patch antennas (conductingpatch mounted in insulating ceramic).

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    Global IGS Network (~150 stations)

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    Specific sites analyzed

    • Total of 100 sites analyzed of which 50 were used

    to realize coordinate system

    • Since analysis has little constraint, it is:– Free to rotate

    – Possibly free to translate (explicit estimation)

    – Possibly free to change scale (explicit estimation)

    • Latter too effects should not be present but these

    we will explore here.

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    Network used in analysis

    Black: Frame sites; Red other sites

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    Results from analysis

    • Examples of time series for some sites

    – “Common Mode” error, example of regional

    frame definition

    • Satellite phase center positions

    • Scale and Center of Mass (CoM) variations

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    Example of motions measured in

    Pacific/Asia region• Fastest motions are

    >100 mm/yr

    • Note convergencenear Japan

    More at http://www-gpsg.mit.edu/~fresh/index2.html

    http://bowie.mit.edu/~fresh/index2.htmlhttp://bowie.mit.edu/~fresh/index2.html

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    Αϖεραγε ΡΜΣ 5 µµ-40

    -20

    0

    20

    40

    1994 1995 1996 1997 1998 1999 2000 2001 2002

    ∆ΧΑΤ1 Εαστ (µµ) −40.1 µµ/ψρ

    ∆ΧΗΙΛ Εαστ (µµ) −36.1 µµ/ψρ

    ∆ΗΟΛΧ Εαστ (µµ) −31.5 µµ/ψρ

    ∆ϑΠΛ Εαστ (µµ) −36.7 µµ/ψρ

    ∆ΥΣΧ1 Εαστ (µµ) −38.3 µµ/ψρ

     

    California East residuals (trends removed)

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    -30

    -20

    -10

    0

    10

    20

    30

    1994 1995 1996 1997 1998 1999 2000 2001 2002

    ∆ΧΑΤ1 Εαστ (µµ)

    ∆ΧΗΙΛ Εαστ (µµ)

    ∆ΗΟΛΧ Εαστ (µµ)

    ∆ϑΠΛ Εαστ (µµ)

    ∆ΥΣΧ1 Εαστ (µµ)

     

    East position residuals (California)

    E l f “ i l” f d fi i i

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    Example from “regional” frame definition

    Ψεαρ

    Ηεχτορ Μινε Εαρτηθυακε

    -10

    -5

    0

    5

    10

    1995 1996 1997 1998 1999 2000 2001

    ∆ΧΑΤ1 Ρεγ (µµ) ΡΜΣ 0.9 µµ

    ∆ϑΠΛΜ Ρεγ (µµ) ΡΜΣ 1.4 µµ

     

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    “Desert” California site

    Year

    RMS

    0.7 mm

    0.6 mm

    2.9 mm

    -30

    -25

    -20

    -15

    -10

    -5

    0

    5

    2000 2000.2 2000.4 2000.6 2000.8 2001

    BULL North (mm)BULL East (mm)BULL Height (mm)

     

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    Origin of “common” mode errors

    • Unknown at the moment, but clearly scaleswith distance (172 of 500 sites in

    S.California have sub-mm daily horizontalscatter, 2-3 mm vertical)

    • Possible effects from satellite transmissionsystem.

    • Example of estimating corrections to phasecenter position (wrt CoM) of satellites

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    Phase center offsets

    a

    δρ = dh cos γ  ; sin γ  = (R/a) sin ψ  ; (R/a) = 0.24

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    Elevation angle dependence

    Ελεϖατιον ανγλε (δεγ)

    -0.005

    0

    0.005

    0.01

    0.015

    0.02

    0.025

    0.03

    0.035

    0 20 40 60 80

    δρ − 1

    0.03 Ηειγητ ερρορ

    Full estimation effects

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    Full estimation effects

    TextEnd

    0

    5

    10

    15

    20 6065

    7075

    8085 90

    0.015

    0.02

    0.025

    0.03

    0.035

    0.04

    0.045

    Max ElevMin Elev

     

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    Effects of phase center position

    changes• A unit change in the radial phase center

    position will change the range to the

    satellite by a constant plus up to 0.03 units.• For 1 meter change; range change about 5

    parts-per-billion

    • If different models of satellites havedifference phase center positions, scalecould change with time.

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    Block IIR

    -2.0 -1.5 -1.0 -0.5 0.0 0.5

    1

    23

    45

    6

    7

    8

    910

    13

    1415

    16

    17

    18

    1921

    22

    23

    2425

    26

    27

    2930

    31

    GPS Satellite Antenna Phase Center offsets

    X Offset (m)

    Y Offset (m)

    Z Offset (m)

    Offset (m)-2.0 -1.5 -1.0 -0.5 0.0 0.5

    1

    23

    45

    6

    7

    8

    910

    13

    1415

    16

    17

    18

    1921

    22

    23

    2425

    26

    27

    2930

    31

    GPS Satellite Phase Center Adjustments

    Offset (m)

    Total phase center position and adjustment to specified values

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    Scale variations with time

    Ψεαρ

    Σχαλε ρατε οφ χηανγε −0.25 ππβ/ψρ

    Γλοβαλ Ηειγητσ −1.6 µµ/ψρ

    -10

    -5

    0

    5

    10

    1992 1994 1996 1998 2000 2002

    ∆σχαλε (ππβ)

     

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    Center of mass variations as well

    Ψεαρ

    Μεαν οφφσετ −120 µµ

    -300

    -200

    -100

    0

    100

    200

    300

    1994 1995 1996 1997 1998 1999 2000 2001 2002

    ∆Ζ (µµ) Σχαλε εστιµατεδδΖ (µµ) Σχαλεδ νοτ εστιµατεδ

     

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    Conclusion• Regional GPS (e.g., California) yields sub-

    millimeter results for “good” stations• Globally RMS increase to 2-3 mm for reasons that

    are not clear

    • Secular scale change -1.6 mm/yr in height

    (Reference sites have 0.8 mm/yr average)• In GAMIT: -120 mm Z-offset in CoM for unknown

    reasons

    • Differences between generations of satellites might

    explain some of these results.• Systematic nature suggests we might be able to

    resolve

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    Relativistic Corrections terms

    • Propagation path curvature due to Earth’spotential (a few centimeters)

    • Clock effects due to changing potential

    • For e=0.02 effect is 47 ns (14 m)

    "τ=2GM

    c3

    ln  R

    r +R

    s+ρ

    Rr +Rs−ρ

     

    $%

    '(

    "τ=−   GM

    c2  e asinE

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    Relativistic Effects

    Time (hrs)

    -50

    -25

    0

    25

    50

    0 4 8 12 16 20 24

    PRN 03 Detrended; e=0.02

    Clock - trend (ns)GR Effect (ns)

     

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    Tectonic Deformation Results

    • “Fixed GPS” stations operate continuously

    and by determining their positions each day

    we can monitor their motions relative to aglobal coordinate system

    • Temporary GPS sites can be deployed on

    well defined marks in the Earth and themotions of these sites can be monitored

    (campaign GPS)

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    Motion after Earthquakes. Example from

    Hector Mine, CA 

    Year

    Hector Mine Earthquake(166 mm removed)

    LDES Site Mojave Desert

    -10

    0

    10

    20

    30

    40

    1999 1999.5 2000 2000.5 2001

    Continued motion tells us about material characteristics

    and how stress is re-distributed after earthquake

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    Relativistic effects

    • General relativity affects GPS in three ways– Equations of motions of satellite

    – Rates at which clock run– Signal propagation

    • In our GPS analysis we account for the

    second two items• Orbits only integrated for 1-3 days andequation of motion term is considered small

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    Clock effects

    • GPS is controlled by 10.23 MHz oscillators

    • On the Earth’s surface these oscillators are set to

    10.23x(1-4.4647x10-10

    ) MHz (39,000 ns/day ratedifference)

    • This offset accounts for the change in potentialand average velocity once the satellite is launched.

    • The first GPS satellites had a switch to turn thiseffect on. They were launched with “Newtonian”clocks

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    Propagation and clock effects

    • Our theoretical delay calculations are made

    in an Earth centered, non-rotating frame

    using a “light-time” iteration i.e., thesatellite position at transmit time is

    differenced from ground station position at

    receive time.• Two corrections are then applied to this

    calculation

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    Effects of Selective Availability

    Time (hrs)

    -200

    0

    200

    400

    600

    800

    0 4 8 12 16 20 24

    PRN 03 (June 14)

    Clock SA (ns) 1999Clock NoSA (ns) 2000

     

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    Conclusions• GPS dual-use technology: Applications in civilian world

    widespread– Geophysical studies (mm accuracy)

    – Engineering positioning (