[IGSMAIL-2879]: new <P1-C1> pseudorange bias corrections
Jim Ray (USNO 202-762-1444)
jimr at maia.usno.navy.mil
Fri Jun 9 05:53:41 PDT 2000
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IGS Electronic Mail 09 Jun 05:53:25 PDT 2000 Message Number 2879
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Author: Jim Ray
Dear Colleagues,
With reference to the <P1-C1> pseudorange bias values distributed in IGS
Mail #2744 (15 Mar 2000), David Jefferson (JPL) has computed an updated set
of biases using the same procedures as Ron Muellerschoen did for the
previous set; see the attached e-mail below. These biases are based on
Ashtech Z-12 data only, collected after the launch of the new Block IIR
satellite PRN20/SVN51, which has been added, and the decommissioning of
PRN14, which as been dropped. As before, the biases have been renormalized
to zero mean across the constellation in order to leave the net receiver
clock bias unaffected.
The following set of new <P1-C1> bias values is recommended for use by all
IGS Analysis Centers and users of IGS clock products, preferably starting
with data collected on 18 June 2000 (beginning of GPS week 1067):
average <P1-C1> biases (mm) in PRN order:
-76 -261 74 508 -174 209 -272 -157 124 -464 PRN01-10
-11 549 -316 -185 -228 83 81 -256 PRN11-20
-137 -450 -148 180 206 463 4 281 560 PRN21-30
-187 PRN31-40
As described by David (see below), these new biases differ from the previous
set by 34 mm (RMS), with minimum and maximum changes of -73 and 89 mm,
respectively.
The RINEX converter utility, cc2noncc, has been updated accordingly. This
utility can be used to transform AOA TurboRogue, AOA ICS-4000Z, and Trimble
4000 RINEX files to be compatible with modern receiver types. The Fortran
code is available at ftp://maia.usno.navy.mil/pub/biases/cc2noncc.f
(version 1.4, 08 Jun 2000).
--Jim Ray
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Date: Thu, 8 Jun 2000 15:11:57 -0700 (PDT)
From: David C Jefferson <djeff at cobra.jpl.nasa.gov>
To: jimr at maia.usno.navy.mil
Subject: Latest C1-P1 results
Cc: David.Jefferson at jpl.nasa.gov, James.F.Zumberge at jpl.nasa.gov,
Ronald.J.Muellerschoen at jpl.nasa.gov, Yoaz.Bar-Sever at jpl.nasa.gov,
gpetit at si.bipm.fr, tim.springer at aiub.unibe.ch
I have been assisting Ron Muellerschoen in reviewing our P1-C1 estimates.
My comparisons involve our original estimates based on Ashtechs only, new
estimates based on Ashtechs only, new esimates based on Benchmarks only,
and Ashtech/Benchmark estimates from Y. Gao at the University of Calgary.
After adjusting each of the sets of satellite-dependent pseduorange biases
to make them consistent (w.r.t. sense, zero-means, satellites used, and
reference used), the following statistics have been realized using 25 GPS
satellites (units are mm):
n mean sd min max RMS med
GB-GA: 25 0 82 -177 140 80 25
JA-JA0: 25 -1 35 -73 89 34 1
JB-JA0: 25 0 96 -241 195 94 11
JB-JA: 25 1 96 -238 157 94 14
JA-GA: 25 -1 38 -99 68 37 7
JB-GB: 25 0 57 -131 104 56 2
KEY: GA = Gao Benchmark estimates
GB = Gao Ashtech estimates
JA0 = original JPL Ashtech estimates
JA = recent JPL Ashtech estimates
JB = recent JPL Benchmark estimates
Our results are consistent with those from Gao, in that:
a) Ashtech then/now agreement is about 3 cm (Gao = 1 cm).
b) RMS difference between Ashtechs vs. Benchmarks is about 9 cm (Gao = 8 cm).
We also now have (Ashtech) estimates for newly-lauched PRN20/GPS51. A full
full of new estimates, which we expect to incorporate into our processing
shortly, is shown below:
-76 -261 74 508 -174 209 -272 -157 124 -464 PRN01-10
-11 549 -316 -185 -228 83 81 -256 PRN11-20
-137 -450 -148 180 206 463 4 281 560 PRN21-30
-187 PRN31-40
We also intend to asses the effects of using our Benchmark estimates, alone
as well as with the Ashtech ones, on our global network orbit analyses.
Please forward this message as appropriate.
Regards,
David
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