vlbi2010 reference antenna for antenna deformations and site ties east coast geodetic vlbi meeting...
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![Page 1: VLBI2010 Reference antenna for antenna deformations and site ties East Coast Geodetic VLBI Meeting 23-24 Feb, 2011, Haystack Observatory Bill Petrachenko](https://reader036.vdocument.in/reader036/viewer/2022082621/56649e985503460f94b9b754/html5/thumbnails/1.jpg)
VLBI2010 Reference antenna for antenna deformations and site ties
East Coast Geodetic VLBI Meeting
23-24 Feb, 2011, Haystack Observatory
Bill Petrachenko
![Page 2: VLBI2010 Reference antenna for antenna deformations and site ties East Coast Geodetic VLBI Meeting 23-24 Feb, 2011, Haystack Observatory Bill Petrachenko](https://reader036.vdocument.in/reader036/viewer/2022082621/56649e985503460f94b9b754/html5/thumbnails/2.jpg)
Using a small reference antenna for antenna deformations and site ties
Small reference antenna
Use connected element interferometryto a small nearby antenna to measurethe “effective” reference point of the
VLBI2010 antenna- and to measure the effect of
VLBI2010 antenna deformations
Observe GNSS satellites with the samesmall antenna and measure
the “effective” reference point of the GNSS antenna
The intersection of axes of the smallantenna becomes the reference point forboth VLBI & GPS and ties the techniques
VLBI2010 antenna
GPS antenna
![Page 3: VLBI2010 Reference antenna for antenna deformations and site ties East Coast Geodetic VLBI Meeting 23-24 Feb, 2011, Haystack Observatory Bill Petrachenko](https://reader036.vdocument.in/reader036/viewer/2022082621/56649e985503460f94b9b754/html5/thumbnails/3.jpg)
Question 1: Are there enough strong sources to correlated with a small reference antenna?
System parameters Ref. antenna: D = 2-, 2.5, or 3-m; eff = 0.5; Tsys = 80-K Centre freq = 8.5-GHz BW = 1-GHz TINT = 60-s Single-polarization SNRmin = 10
Sources selected from the Bordeaux Image Gallery 834 candidate VLBI sources Each oberved 1 to ~40 times in S-, X-, K-, and/or Q-band Parameters in the data base
Total flux (ST) Median correlated flux (Sm) over UV-plane Delay error, median for UV-plane
I used median values for ensemble of sessions observed
![Page 4: VLBI2010 Reference antenna for antenna deformations and site ties East Coast Geodetic VLBI Meeting 23-24 Feb, 2011, Haystack Observatory Bill Petrachenko](https://reader036.vdocument.in/reader036/viewer/2022082621/56649e985503460f94b9b754/html5/thumbnails/4.jpg)
3-m 2.5-m 2-m
Number of sources available for a2-, 2.5-, or 3-m reference antenna
correlated with a 12-m VLBI2010 antenna
![Page 5: VLBI2010 Reference antenna for antenna deformations and site ties East Coast Geodetic VLBI Meeting 23-24 Feb, 2011, Haystack Observatory Bill Petrachenko](https://reader036.vdocument.in/reader036/viewer/2022082621/56649e985503460f94b9b754/html5/thumbnails/5.jpg)
Question 2: Is GPS multipath small enough using a small parabolic reference antenna?
Worst case assumptions Multipath reflector is horizontal with 100% reflection
coefficient Sidelobe gain for the ref. antenna is according to the
ITU equation: Gi = 32-25*log10(θ) The multipath signal phase is offset by 90 deg from the
direct signal.
![Page 6: VLBI2010 Reference antenna for antenna deformations and site ties East Coast Geodetic VLBI Meeting 23-24 Feb, 2011, Haystack Observatory Bill Petrachenko](https://reader036.vdocument.in/reader036/viewer/2022082621/56649e985503460f94b9b754/html5/thumbnails/6.jpg)
Worst Case GPS Multipath
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0 5 10 15 20
Elevation angle (deg)
Ran
ge
erro
r (m
m)
f=1.2 GHz,D=2.0
f=1.2 GHz,D=2.5
f=1.2 GHz,D=3.0
f=1.6 GHz,D=2.0
f=1.6 GHz,D=2.5
f=1.6 GHz,D=3.0