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observations_of_gnss-satellites_on_the_hobart-ceduna_baseline
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observations_of_gnss-satellites_on_the_hobart-ceduna_baseline [2016/11/01 02:41] Lucia McCallum |
observations_of_gnss-satellites_on_the_hobart-ceduna_baseline [2016/11/01 03:00] (current) Lucia McCallum [near field model comparison] |
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| First results were presented during the IVS GM in South Africa [[http://events.saip.org.za/getFile.py/access?contribId=55&sessionId=6&resId=0&materialId=slides&confId=56|Hellerschmied et al.]] and the VLBI WS for nera field targets in Bonn ([[http://www3.mpifr-bonn.mpg.de/div/meetings/vonft/pdf-files/talks/Hellerschmied_Bonn_2016.pdf|scheduling]], [[http://www3.mpifr-bonn.mpg.de/div/meetings/vonft/pdf-files/talks/2016_Bonn_Plank.pdf|observations]], [[http://www3.mpifr-bonn.mpg.de/div/meetings/vonft/pdf-files/talks/McCallum.WS2016.pdf|technical challenges]]). | First results were presented during the IVS GM in South Africa [[http://events.saip.org.za/getFile.py/access?contribId=55&sessionId=6&resId=0&materialId=slides&confId=56|Hellerschmied et al.]] and the VLBI WS for nera field targets in Bonn ([[http://www3.mpifr-bonn.mpg.de/div/meetings/vonft/pdf-files/talks/Hellerschmied_Bonn_2016.pdf|scheduling]], [[http://www3.mpifr-bonn.mpg.de/div/meetings/vonft/pdf-files/talks/2016_Bonn_Plank.pdf|observations]], [[http://www3.mpifr-bonn.mpg.de/div/meetings/vonft/pdf-files/talks/McCallum.WS2016.pdf|technical challenges]]). | ||
| - | **We have a series (6 hours) of measured delays on the Ho-Cd baseline. If interested, we are happy to share our experience and provide data for comparisons.** | + | <note>We have a series (6 hours) of measured delays of multiple GNSS-satellites on the Ho-Cd baseline. If interested, we are happy to share our experience and provide data for comparisons.</note> |
| ===== near field model comparison ===== | ===== near field model comparison ===== | ||
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| + | M. Rothacher from ETH was interested to compare the modelled delays. [[http://fourier.phys.utas.edu.au/wg7/|131a_vievs.dat]] is a file containing the theoretical delyas calculated with VieVS. Values are in seconds. Time reference is time of signal reception (UT) at station 1. The delay includes the a priori hydrostatic delay as well as the antenna axis offset which is up to 8m for the Hobart26 antenna. | ||
/home/www/auscope/opswiki/data/attic/observations_of_gnss-satellites_on_the_hobart-ceduna_baseline.1477968062.txt.gz · Last modified: 2016/11/01 02:41 by Lucia McCallum
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