Title |
Primary Author |
Preliminary estimation of the atmospheric nonlinear
frequency dispersion and absorption effects on the pulse SLR accuracy |
Yuri Galkin |
Moscow State Forest University
Mytischi-5, MGUL
141005, Moscow Region
RUSSIA
Voice: +7-095-586-9134
Fax: +7-095-586-9134
Email: galkin@mgul.ac.ru
Ruben A. Tatevian
Central Scientific Research Institute of Geodesy, Aero-Survey
and Cartography
RUSSIA
It is known, that the nonlinearity of the frequency-dependent
refraction and absorption of air can evoke in additional errors
of SLR, because of changes of the received ranging signal parameters
are relatively of the standard calculation methods. Additional
group delays, shift of a carrying frequency and her change in
a receiving point of the Gaussian laser pulse for SLR are estimated.
The estimation is made for "smooth" dispersion curve
(just effective UV resonances) without effects of the atmospheric
local resonances. It is noted that the shown effects are most
important of the multi color SLR for Marini-Murray atmospheric
model correction because of the effects depend on a laser ray
elevation angle.
Poster paper; received August 6, 2002
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Biaxial Rayleigh- and Raman-LIDAR for applications
in atmospheric sounding and SLR |
Ulrich Schreiber |
Technical University of Munich
Fundamentalstation Wettzell
D-93444 Koetzting
GERMANY
Voice: +49 9941 603113
Fax: +49 9941 603222
Email: schreiber@wettzell.ifag.de
Florian Seitz, Franz Meyer
Technical University of Munich
Nikolaus Brandl
Bundesamt fuer Kartographie und Geodaesie
Fundmentalstation Wettzell
D-93444 Koetzting
GERMANY
Precise orbit determinations in SLR and LLR require corrections
for the contribution of the atmosphere to the effective index
of refraction. Despite the fact that the range measurements are
obtained consistently, there is a discrepancy of approximately
4cm reported in the comparison between optical and microwave based
range measurements for the same GPS satellite target. As a conclusion
from earlier work, the knowledge of the water vapor content of
the atmosphere at least for some selections of the operation wavelength
seems important. To overcome the lack of sensitivity for the measurement
of water vapour profiles in the Earth's troposphere by means of
remote sensing a biaxial Rayleigh- and Raman LIDAR has been set
up on the Fundamentalstation Wettzell, making use of the still
existing equipment of a former SLR facility. By operating the
station as a Rayleigh-LIDAR its geometrical characteristics and
the overall sensitivity of this setup as a LIDAR system could
be established and optimized. Observations in the spectral range
of 607 nm and 660 nm are probing the troposphere for nitrogen
and water molecules. By combining this information water vapor
profiles of the lower troposphere were obtained.
Oral paper; received August 14, 2002
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Wavelength Dependence of Range Correction |
David Arnold |
94 Pierce Road
Watertown, MA 02472-3035
USA
Voice: 617-924-3811
Fax:
Email:
The diffraction pattern of a retroreflector depends on the wavelength
of the incident light. As a result, the range correction for an
array with retroreflectors at different orientation angles will
be different at each wavelength. This paper shows range correction
matrices for LAGEOS at various wavelengths such as 355, 423.5,
847, and 1064 nanometers
Oral paper; received August 22, 2002
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Atmospheric Contribution to the Laser Ranging Jitter |
Ivan Prochazka |
Czech Technical University
Brehova 7
115 19 Prague 1
CZECH REPUBLIC
Voice: +420 2 21912246
Fax: +420 2 21912252
Email: prochazk@mbox.cesnet.cz
L. Kral
Czech Technical University
Brehova 7
115 19 Prague 1
CZECH REPUBLIC
The contribution of the atmospheric fluctuation - the seeing
- to the laser ranging has been investigated. The beam propagation
has been modeled using two independent approaches and models.
The random component of the atmospheric propagation correction
has been found to be well below 10 um for all seeing conditions,
beam path geometry and wavelength.
Oral paper; received August 22, 2002
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Validation of Mapping Functions |
Stefan Riepl |
Bundesamt fuer Kartographie und Geodaesie
D-93444 Koetzting,
GERMANY
Email: riepl@wettzell.ifag.de
David Ramirez, Cesar Guitano
Universidad de Concepcion
Concepcion
CHILE
The present paper focuses on techniques, both numerical and experimental,
which are currently used to validate mapping functions relating
the zenith path delay correction to other angles of elevation.
The paper concentrates on the application of two-color laser ranging
data taken with the TIGO SLR module, aiming on a determination
of the zenith path delay, as well as the utilization of numerical
weather prediction data, which is applied to the estimation of
horizontal refractivity gradients. Moreover a comparison of mapping
functions with respect to their applicable spectrum of wavelengths
is given using raytracing techniques.
Oral paper; received August 23, 2002
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Zimmerwald Dual-wavelength Operation: First Experiences |
Werner Gurtner |
Astronomical Institute
University of Bern
Sidlerstrasse 5
CH-3012 Bern
SWITZERLAND
Voice: 0041 31 6318591
Fax: 0041 31 6313869
Email: werner.gurtner@aiub.unibe.ch
Eugen Pop, Johannes Utzinger
Astronomical Institute
University of Bern
Sidlerstrasse 5
CH-3012 Bern
SWITZERLAND
On August 14, 2002 Zimmerwald started to submit dual-wavelength
SLR data collected on 423 and 846 nm using two Hamamatsu photomultipliers.
The paper discusses the special hard- und software installations
needed for the dual-wavelength operation and presents first results
of acquired passes.
Oral paper; received August 29, 2002
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A Database of Atmospheric Refractivities from GPS
Radio Occultations |
Manuel de la Torre Juárez |
Jet Propulsion Laboratory/Caltech
M/S 238-600, 4800 Oak Grove Dr.
Pasadena, CA 91109-8099
USA
Phone: 818 354-4548
Fax: 818 393-4965
Email: mtj@jpl.nasa.gov
George A. Hajj, Byron I Iijima, Chi O Ao, Anthony J. Mannucci,
Tom P. Yunck
Jet Propulsion Laboratory/Caltech
M/S 238-600, 4800 Oak Grove Dr.
Pasadena, CA 91109-8099
USA
The launches of the CHAMP, SAC-C, and GRACE spacecraft have started
a campaign of dense remote sensing of atmospheric refractivity
profiles using GPS radio-occultations of the Earth's atmosphere.
These data provide high resolution profiles of refractivities,
up to the stratopause, which can be converted into geopotential
heights, and atmospheric pressure and temperature as a function
of geometric heights.
These data are been made available to the community interested
in operational applications. The characteristics and quality,
of the data will be described.
Oral paper; received September 03, 2002
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Modification of Laser Ranging Equation |
Xiong Yaoheng |
Yunnan Observatory, Chinese Academy of Sciences
P.O. Box 110
Kunming 650011
CHINA
Voice: 86-871-3911347
Fax: 86-871-3911845
Email: yozsx@public.km.yn.cn
Feng Hesheng
Yunnan Observatory, Chinese Academy of Sciences
P.O. Box 110
Kunming 650011
CHINA
The goal of this paper is to discuss the atmospheric turbulent
effects on the laser beam of the laser ranging, especially for
the lunar laser ranging. Considering the laser beam wander and
spread caused by the atmospheric turbulence and the distribution
of the laser beam, a new form of the laser ranging equation is
given. That will guide us to do the real-time tilt compensation
for the LLR.
Oral paper; received September 11, 2002
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Two-color laser ranging with the MLRO system |
Giuseppe Bianco |
Agenzia Spaziale Italiana
Centro di Geodesia Spaziale "G. Colombo"
P.O. Box 11
75100 Matera (MT)
ITALY
Voice: +39-0835-377209
Fax: +39-0835-339005
Email: giuseppe.bianco@asi.it
T. Oldham, M. Bieneman, C. Clarke, V. Husson
Honeywell-TSI
7515 Mission Drive
Lanham, MD 20706
USA
The Matera Laser Ranging Observatory (MLRO) has been developed
and installed by Honeywell Technology Solutions Inc. at the Center
for Space Geodesy "Giuseppe Colombo" (CGS) of the Italian
Space Agency (ASI). The MLRO has built-in two-color ranging capability
at 532 nm and 355 nm wavelengths with two receiving configurations:
either a dual microchannel plate photomultiplier chain or a Hamamatsu
streak camera. This presentation briefly outlines the system setup
for two color ranging, and describes the first observational results
obtained so far on ground targets and satellites.
Oral paper; received September 17, 2002
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Atmospheric Refraction at Optical Wavelengths:
Problems and Solutions |
Virgilio Mendes |
Faculdade de Ciências da Universidade de Lisboa, Dep. de
Matemática
Ernesto de Vasconcelos
Bloco C1 - PISO 3
1749-016 Lisboa
PORTUGAL
Voice: +351 21 7500842
Fax: +351 21 750 0072
Email: vmendes@fc.ul.pt
Presented by: Erricos C. Pavlis
Atmospheric refraction is an important accuracy-limiting factor
in the application of satellite laser ranging (SLR) to high-accuracy
applications. The modeling of that source of error in the analysis
of SLR data comprises the determination of the delay in the zenith
direction and subsequent projection to a given elevation angle,
using a mapping function. Standard data analyses practices use
the Marini-Murray model for both zenith delay determination and
mapping. This model was tailored for a particular wavelength and
is not suitable for all the wavelengths used in modern SLR systems.
Using ray tracing though a large database of radiosonde data,
we assess the zenith delay models and mapping functions currently
available, we discuss the effect of using different types of input
data to drive those models and the sensitivity of models and functions
to changes in the wavelength and we give some recommendations
towards a unification of practices and procedures in SLR data
analysis.
Oral paper; received September 17, 2002
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