Upload
others
View
3
Download
0
Embed Size (px)
Citation preview
Realization of ETRS89:Alternatives, future concepts
Werner GurtnerJ h IhdJohannes IhdeJens Luthardt
EUREF Symposium, Brussels, June 18-20, 2008
AIUBAstronomisches Institut der Universität Bern
ETRS89 Definition
Resolution No 1, Firenze 1990
"recommends that the system to be adopted by EUREF will be coincident with ITRS at the epoch 1989.0 and fixed to the stable part of the Eurasian Plate and will be
20, 2
008
fixed to the stable part of the Eurasian Plate and will be known as European Terrestrial Reference System 89 (ETRS89)"
s, Ju
ne 1
8-2
"accepts that … for most applications, the coordinates will have no time variation"
um, B
russ
el
Resolution No 1, Bern 1992
ie 2
REF
Sym
posi
"recommends that this solution (Bernese solution of EUREF GPS 1989 campaign) be accepted as the current realiastion of the ETRS89 under the name of EUREF89"
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Conclusions from the definition
"fixed to the stable part" implies that the ETRS is rotating "somehow" with the Eurasian plate"no time variation" implies the desire to avoid
20, 2
008
no time variation implies the desire to avoid changes in time of the positions of European stations within the stable part
s, Ju
ne 1
8-2
The definition does not say anything about the realizations nor the reference epoch of the realizations
um, B
russ
el realizations
The first realization (EUREF89) was based on
ie 3
REF
Sym
posi The first realization (EUREF89) was based on SLR/VLBI-derived "fiducial stations" given in ITRF89 at epoch 1989.0
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
First realization of ETRS89
ITRF892000
20, 2
008 1995
s, Ju
ne 1
8-2
ETRF89 1989 0
um, B
russ
el ETRF89EUREF89
1989.0
ie 4
REF
Sym
posi
z =z
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR z89=z89
Most simple realization based on a ITRFyy
Just fulfilling the requirement "fixed to the stable part":Just fulfilling the requirement fixed to the stable part :
Take a realization of ITRS ITRFyy
20, 2
008
yyDetermine "somehow" rotation pole and rotation rate dr/dt of the Eurasian plate from this solution
s, Ju
ne 1
8-2
Select a reference epoch for the realizationMove all European reference stations into the reference epoch by their ITRFyy velocities
um, B
russ
el reference epoch by their ITRFyy-velocitiesRotate them by the rotation angle
d /d * ( 1989 0)
ie 5
REF
Sym
posi r = dr/dt * (tref-1989.0)
into the ETRS89 ETRFyy
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Later Realizations of ETRS89
ITRF89 ~ ITRF2000 ~ ITRF2005 ETRF2005
ETRFyy = f(ITRFyy)
20, 2
008 ETRF2000
z2005
s, Ju
ne 1
8-2
ETRF89
EPN
um, B
russ
el ETRF89 z2005z2000
ie 6
REF
Sym
posi
z89=z89
z2000
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Remarks to the Most simple realization
Each realization is completely independent from earlier realizations (unless the ITRFyy datum depends on earlier datums)
20, 2
008 In the early days the applied rotation was based on plate
motion models
s, Ju
ne 1
8-2
Changes/uncertainties in the applied rotation rate will become more disturbing with time
um, B
russ
el
more disturbing with time
Changes/uncertainties related to the datum realizations of subsequent ITRFyy may also lead to significant variations of
ie 7
REF
Sym
posi subsequent ITRFyy may also lead to significant variations of
positions in the ETRFyy counterpart
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Improvements (1)
Include additional parameters into the ptransformation ITRFyy ETRFyy
20, 2
008 E.g., to attenuate effects from changes in the datum
Mainly translations, Zuheir also includes translation rates
s, Ju
ne 1
8-2
Various ways how to determine such additional parameters
um, B
russ
el parameters
Proposal by Zuheir to base these additional parameters on
ie 8
REF
Sym
posi the values determined in the "memo", i.e. based on global analysis
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Improvements (2)
R f ll b t li ti ETRF tRefer all subsequent realizations ETRFyy to a reference realization, e.g., ETRF2000, i.e. extract and combine parameters from the memo in a way
20, 2
008
and combine parameters from the memo in a way that they take into account the datum differences to ETRF2000 (actually between ITRFyy and ITRF2000)
s, Ju
ne 1
8-2 y yy
um, B
russ
el Remark: The "memo values" are results from the global analysis, they are not specifically
ti i d f E
ie 9
REF
Sym
posi optimized for Europe
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Alternative Realization of ETRS89
ITRF..2005rz ~ (z2005- z1989) / (t2005-1989.0) 2005005 989 005
~ (z2005- z2000) / (t2005-1989.0)~ ...
20, 2
008 ETRF2000
s, Ju
ne 1
8-2
ETRF89
um, B
russ
el ETRF89 z2005z2000
ie 1
0
REF
Sym
posi
z89
ITRF2005 European Realization:Determine best-fitting transformation parameters between
ITRF2005 and previous ETRS89 realization, e.g., ETRF2000
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR p , g ,
Rigorous Solution
Select a reference realization ETRF00, e.g., ETRF2000Select max number of European stations that
are present in both ETRF2000 and ITRFyy with sufficiently long history
20, 2
008
historylie in the "stable part" of Europe
Move the stations into common reference epoch using
s, Ju
ne 1
8-2 Move the stations into common reference epoch using
respective velocities (ETRF2000 and ITRFyy)Determine Helmert transformation parameters between
um, B
russ
el
pthe two sets of coordinates (least squares adjustment)Introduce the smallest possible number of parameters,
ie 1
1
REF
Sym
posi e.g., 3 translations, 3 rotations and r.rates and
Include additional derivatives, if necessary
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Least-squares estimation of transformation parametes
31 defining points used for the estimation of
20, 2
008
for the estimation of transformation parameters between ITRF and ETRF
s, Ju
ne 1
8-2 ITRF and ETRF
i.e . withoutHOFN on Island
um, B
russ
el HOFN on IslandKELY and THU1 on GreenlandNYAL on Spitsbergen
ie 1
2
REF
Sym
posi
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Transformation parameters from ITRF2005 Ep. 2000.0 to ETRF2000 Ep. 2000.0
Tx mm
Ty mm
Tz mm
D 10-9
Rx mas
Ry mas
Rz mas
sigma0mm
20, 2
008
mm mm mm 10 mas mas mas mm43 ±3
46 ±6
-46 ±3
1.0 ±0.5
0.7 ±0.2
5.8 ±0.1
-8.8 ±0.1
2.5
s, Ju
ne 1
8-2
δTx mm/y
δTz mm/y
δTz mm/y
δD 10-9/y
δRx mas/y
δRy mas/y
δRz mas/y
sigma0mm/y
um, B
russ
el -0.28±0.03
+0.05±0.02
+0.52±0.01
-0.80±0.03
0.93
ie 1
3
REF
Sym
posi
31 stations used
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
ETRFyyITRFyy 70 + 41 / 152
2005 ETRF2005ITRF2005 (00.0)
ETRFyyITRFyy Memo Vers. 6 / 770 + 41 / 152 stations
70 stationsworldwide 31 stations
TTTSRRRPxxxx000
Gurtner / Ihde
Jumps31 stations stable part of Europe
Rxxxx000
TTTSRRRPxxxxxxx
2000 ETRF2000
R---xxxx
ITRF2000 (97 0)
ITRF2000 (00.0)
1997 ITRF1997 (97.0)TTTSRRR
Memo Vers. 5ITRF2000 (97.0)
Altamimi
?? stations
1996TTTSRRRPxxxxxxxRxxxxxxxITRF1996 (97.0)
M B h / Alt i i S ifi ti f f f fi i i th l i f EUREF GPS iMemo: Boucher / Altamimi, Specification for reference frame fixing in the analysis of EUREF GPS campaign
Residuals ???2005-ETRF2000
mm
20, 2
008
s, Ju
ne 1
8-2
um, B
russ
el
Z.Altamimi
ie 1
5
REF
Sym
posi
Least squares transformation
Proposal by Altamimi
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR Proposal by Altamimi
Remarks to Rigorous Solution
Rotation angles divided by (reference epoch – 1989.0) approximate rotation rate of Euroasian plateapproximate rotation rate of Euroasian plateThey also contain contributions of systematic errorsAll the parameters soak up systematic errors of datum realizations and errors of regional nature
20, 2
008
realizations and errors of regional nature
Parameters are mathematical transformation parameters and
s, Ju
ne 1
8-2 don't have to be physically interpreted Formal errors are
unimportant.
um, B
russ
el Maintains full internal accuracy of the original ITRFyy solutionYields the smallest possible residuals/jumps w/r to the reference solution (vtPv = min) closest to the users' needs
ie 1
6
REF
Sym
posi reference solution (v Pv min) closest to the users needs
Could be further improved by using densified reference network
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR network
Current situation
S f ETRS89 li ti f ll b d ITRFSo far ETRS89 realizations are fully based on ITRFyy solutions
20, 2
008 Contribution by EUREF:
European IGS stations and SLR/VLBI being part of ITRFyy
s, Ju
ne 1
8-2 European IGS stations and SLR/VLBI being part of ITRFyy
2000: Inclusion of EPN into ITRF2000 solution
um, B
russ
el
So far, ETRS89 realizations have not been optimized for maximum consistency between subsequent
ie 1
7
REF
Sym
posi realizations
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR
Further improvements, future concepts
European Permanent Network:200 permanent stations availableTime series of weekly solutionsAccumulated solutions
Use EPN for the maintenance of the ETRS89
20, 2
008 Excellent internal accuracy
Time resolution, spatial densityVelocity field
s, Ju
ne 1
8-2 Velocity field
EPN processing based on ITRF/IGSyy ( orbits, ERPs,..., SLR,...)ETRS89 realizations „independent“ from ITRFyy:
D i
um, B
russ
el DensityFrequency...
ie 1
8
REF
Sym
posi Optimized for long-term consistency between subsequent
realizationsITRFyy ETRFyy: Availability of positions/velocities of
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR yy yy y p /
reference stations and of transformation parameters
Open questions (1)
How to make use of EPN? In detail?How often will there be updates to the parameters and reference coordinates?Based on which solutions? Based on which reference?
20, 2
008
Based on which solutions? Based on which reference?How do the mathematical models of the optimization function and the transformations look like? What to do with “scale” diff ?
s, Ju
ne 1
8-2 differences?
What to do with annual (or other) variations of ITRFyy/IGSyy-based positions?
um, B
russ
el
pEPN positionsCampaign-based positions
How to refer user results to the respective realization (naming
ie 1
9
REF
Sym
posi How to refer user results to the respective realization (naming,
traceability, citation, uniqueness)?
l k d
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR New special working group proposed
Open questions (2)
Do we need to modify the definition of ETRS89?
20, 2
008 I don't think so!
Definition is simpleS ff l
s, Ju
ne 1
8-2 Sufficiently vague
um, B
russ
el
Need to modify/extend specifications for the realization/maintenance of ETRS89
ie 2
0
REF
Sym
posi realization/maintenance of ETRS89
e.g., quantification of the “stable part”
AIUB
Foli
Astronomisches Institut der Universität Bern
EUR