A dual linear polarization fringe fitting method for VLBI observation
In this paper, we propose a dual linear polarization fringe fitting method which can be used in the next generation VLBI system (VLBI global observing system, VGOS). The legacy geodetic VLBI observation mode is dedicated to the right circular polarization (RCP), which differs from the dual linear po...
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doaj-cc211fd6ca9b42b1a682a5b978e6c7742020-11-25T03:26:25ZzhoSurveying and Mapping PressActa Geodaetica et Cartographica Sinica1001-15951001-15952020-04-0149442343110.11947/j.AGCS.2020.2019008320200403A dual linear polarization fringe fitting method for VLBI observationHUANG Yidan0LIU Lei1SHU Fengchun2ZHENG Weimin3Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;In this paper, we propose a dual linear polarization fringe fitting method which can be used in the next generation VLBI system (VLBI global observing system, VGOS). The legacy geodetic VLBI observation mode is dedicated to the right circular polarization (RCP), which differs from the dual linear polarization adopted in the VGOS system. The algorithm presented in this work consists of the calibration part and combined fringe fitting part. In the calibration part, we derive the intermediate frequency (IF) delay and phase calibration information from each polarization product by carrying out fringe fitting on a strong reference source. Then this information is applied to the target sources. In the combined fringe fitting part, we combine 4 polarization products into the Pseudo-Stokes Intensity and in the meanwhile search for the appropriate differential parallactic angle, so as to maximize the amplitude of the intensity and therefore derive the delay as observable. Compared with single polarization, the combined product yields higher signal-to-noise ratio (SNR) and smaller fringe phase scatter.http://html.rhhz.net/CHXB/html/2020-4-423.htmvlbi global observing systemdual linear polarizationfringe fittingsignal-to-noise ratiodelay observationphase scatter |
collection |
DOAJ |
language |
zho |
format |
Article |
sources |
DOAJ |
author |
HUANG Yidan LIU Lei SHU Fengchun ZHENG Weimin |
spellingShingle |
HUANG Yidan LIU Lei SHU Fengchun ZHENG Weimin A dual linear polarization fringe fitting method for VLBI observation Acta Geodaetica et Cartographica Sinica vlbi global observing system dual linear polarization fringe fitting signal-to-noise ratio delay observation phase scatter |
author_facet |
HUANG Yidan LIU Lei SHU Fengchun ZHENG Weimin |
author_sort |
HUANG Yidan |
title |
A dual linear polarization fringe fitting method for VLBI observation |
title_short |
A dual linear polarization fringe fitting method for VLBI observation |
title_full |
A dual linear polarization fringe fitting method for VLBI observation |
title_fullStr |
A dual linear polarization fringe fitting method for VLBI observation |
title_full_unstemmed |
A dual linear polarization fringe fitting method for VLBI observation |
title_sort |
dual linear polarization fringe fitting method for vlbi observation |
publisher |
Surveying and Mapping Press |
series |
Acta Geodaetica et Cartographica Sinica |
issn |
1001-1595 1001-1595 |
publishDate |
2020-04-01 |
description |
In this paper, we propose a dual linear polarization fringe fitting method which can be used in the next generation VLBI system (VLBI global observing system, VGOS). The legacy geodetic VLBI observation mode is dedicated to the right circular polarization (RCP), which differs from the dual linear polarization adopted in the VGOS system. The algorithm presented in this work consists of the calibration part and combined fringe fitting part. In the calibration part, we derive the intermediate frequency (IF) delay and phase calibration information from each polarization product by carrying out fringe fitting on a strong reference source. Then this information is applied to the target sources. In the combined fringe fitting part, we combine 4 polarization products into the Pseudo-Stokes Intensity and in the meanwhile search for the appropriate differential parallactic angle, so as to maximize the amplitude of the intensity and therefore derive the delay as observable. Compared with single polarization, the combined product yields higher signal-to-noise ratio (SNR) and smaller fringe phase scatter. |
topic |
vlbi global observing system dual linear polarization fringe fitting signal-to-noise ratio delay observation phase scatter |
url |
http://html.rhhz.net/CHXB/html/2020-4-423.htm |
work_keys_str_mv |
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1724592943149350912 |