Estimation and validation of receiver antenna codephase variations for multi GNSS signals

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dc.identifier.uri http://dx.doi.org/10.15488/5233
dc.identifier.uri https://www.repo.uni-hannover.de/handle/123456789/5280
dc.contributor.author Breva, Yannick ger
dc.contributor.author Kröger, Johannes ger
dc.contributor.author Kersten, Tobias ger
dc.contributor.author Schön, Steffen ger
dc.contributor.editor European Space Agency (ESA)
dc.date.accessioned 2019-08-26T08:55:00Z
dc.date.available 2019-09-04T22:05:02Z
dc.date.issued 2019-09-04
dc.identifier.citation Breva, Y. et al.: Estimation and validation of receiver antenna codephase variations for multi GNSS signals. 7th International Colloquium on Scientific and Fundamental Aspects of GNSS, September 4-6, 2019, ETH Zürich, Switzerland ger
dc.description.abstract Besides antenna phase center corrections (PCC) for carrier phase measurements, which have to be considered for precise GNSS application, also codephase variations (CPV) exist. These are antenna dependent delays of the code which vary with azimuth and elevation. Such variations are not provided operationally in the antenna exchange format (ANTEX) at the moment. Previous studies in our working group show, that CPV should be taken into account when using code-carrier combination. Depending on the antenna type they can amount up to some dm. At Institut für Erdmessung (IfE), a concept to determine the CPV has been established. This procedure uses a robot that rotates and tilts the antenna under test precisely in the field. Real world modulated signals from the satellites are used, which is challenging in anechoic chamber procedures. Time differenced single differences are used to estimate PCC and CPV as spherical harmonics (8,8) in a post-processing approach. In this contribution we present the concept CPV of Galileo signals for several kinds of receiving antennas (mass market and high grade). In addition, we discuss the repeatability and stability of CPV for those antenna. Typical values of the CPV reaches up to 500 mm. The RMS of patterns resulting from multiple calibrations are 80 mm for Galileo C1X and 48 mm for GPS C1C. ger
dc.language.iso eng ger
dc.publisher Zürich : European Space Agency (ESA) and ETH Zürich
dc.relation.ispartof 7th International Colloquium on Scientific and Fundamental Aspects of GNSS ger
dc.rights CC BY-NC-ND 3.0 DE ger
dc.rights.uri http://creativecommons.org/licenses/by-nc-nd/3.0/de/ ger
dc.subject GNSS eng
dc.subject electromagnetics eng
dc.subject GPS/GNSS antennas eng
dc.subject GNSS receiver antenna calibration eng
dc.subject geodesy eng
dc.subject GNSS ger
dc.subject Elektromagnetik ger
dc.subject GPS/GNSS-Antennen ger
dc.subject GPS/GNSS-Antennenkalibrierung ger
dc.subject Geodäsie ger
dc.subject.ddc 550 | Geowissenschaften ger
dc.subject.ddc 624 | Ingenieurbau und Umwelttechnik ger
dc.subject.ddc 520 | Astronomie, Kartographie ger
dc.title Estimation and validation of receiver antenna codephase variations for multi GNSS signals eng
dc.type ConferenceObject ger
dc.type Text ger
dc.description.version publishedVersion ger
tib.accessRights frei zug�nglich


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