HR: 0800h
AN: G31A-0783 [Abstracts]
TI: Power Spectral Analysis of Simultaneous VLBI and GPS Tropospheric Estimates
AU: * Ray, J
EM: jimr@ngs.noaa.gov
AF: National Geodetic Survey, NOAA
1315 East-West Hwy, Silver Spring, MD 20910
United States
AU: Boehm, J
EM: johannes.boehm@tuwien.ac.at
AF: Institute of Geodesy and Geophysics, TU Vienna
Gusshausstrasse 27-29, Vienna, A-1040
Austria
AB:
Observations by space geodetic techniques experience refraction and signal
delay due to passage through the Earth's atmosphere. For high-accuracy
positioning results, data analysts must account for these effects. Since
independent path delay values of sufficient accuracy are not usually
available, nuisance parameters are commonly added in the geodetic analysis.
The general validity of such zenith path delay (ZPD) estimates as true
atmospheric measures has been confirmed by comparison of results from
independent radiometric and other techniques over many years. Biases and
standard deviations in the sub-cm range are normally found, which is
expected to be adequate as inputs to improve the forecast performance of
numerical weather models. To better understand the noise characteristics of
ZPD estimates from VLBI and GPS, we have examined the power spectra of
simultaneous observations during a 15-day period in October 2002. The
official combined ZPD products from the technique services have been used
primarily, but series from individual analysis centers have also been
included. For the seven sites studied, the power-law spectral indices over
sub-daily intervals are close to -8/3, consistent with fully developed
Kolmogorov turbulence, and flatten over longer periods. The VLBI series,
sampled hourly, show white noise at levels of 0.7 to 1.5 mm for
frequencies above 5 cycles per day. The simultaneous GPS series, sampled
every 2 hours, display no indication of white noise except for one receiver
with poor data analysis. The spectra of VLBI-GPS differences are generally
flat but show possible signs of excess noise in some spectral bands. Based
on these results, estimating VLBI ZPD values more often than every few hours
should be reconsidered, especially if changes would strengthen other
parameters. On the other hand, GPS-based ZPD estimates should be determined
more frequently, at least hourly. Considering the greater reliability of
the VLBI scale and the corresponding weakness of GPS (mostly due to
uncertainties in the phase patterns of the satellite transmit and tracking
station antennas), an optimal combination of ZPD results should rely on the
VLBI estimates for its absolute long-term accuracy and weight GPS heavily
for its high-frequency precision.
DE: 1200 GEODESY AND GRAVITY
DE: 1244 Standards and absolute measurements
DE: 1294 Instruments and techniques
DE: 0360 Transmission and scattering of radiation
DE: 0365 Troposphere--composition and chemistry
SC: Geodesy [G]
MN: 2004 AGU Fall Meeting