ITS 20-meter parabolic antenna, Table Mountain, Colorado, USA
GIOVE-B on the Air
Understanding Galileo's New Signals
Following up on their earlier work analyzing and decoding new GNSS signals, researchers from Stanford University and the University of Colorado confirm that GIOVE-B transmits on L1, E5a, and E5b bands with MBOC modulation in L1, and finds the PRN generators in all bands to be 13- or 14-stage Gold codes, not the memory codes specified in the Galileo ICD.
Europe’s second Galileo In-Orbit Validation Element (GIOVE-B) test satellite was launched on April 27, 2008, at 22:16 UTC and began transmissions on May 7.
On the same day, we observed signals in the L1, E5a, and E5b bands, with the L1 spectrum showing multiplexed binary offset carrier (MBOC) modulation. We then identified the generators for the PRN codes in each band, using the approach described in our previous Institute of Navigation (ION) conference papers listed in the Additional Resources section at the end of this article. We revealed these codes to be 13- or 14-stage Gold codes, different from the memory codes in the Galileo Interface Control Document (ICD).
Our results were validated by acquiring the transmitted signals with these codes. In the following discussion, we elaborate on our data collection apparatus, the observed signal spectra, and the revealed PRN code generators of GIOVE-B.
As in previous observations described in a May/June 2006 article in Inside GNSS, both antennas were connected to an vector signal analyzer that enabled the capture of extended data records of multiple seconds of 36 MHz bandwidth at the various frequency bands of interest. We used data from the SGMS to determine the codes associated with the GIOVE-B L1 transmission, while data collected with the larger-aperture antenna was used to study the GIOVE-B E5 code generation.
The 20-meter parabolic antenna shown in the photo above is located at Table Mountain in Colorado and owned by the Institute for Telecommunication Sciences (ITS). The institute is the research and engineering branch of the National Telecommunications and Information Administration (NTIA). Until recently, the facility had sat dormant but has now undergone a renovation bringing it to operational status, thanks in part to a joint effort involving ITS, the volunteer Deep Space Exploration Society <http://deep-space.org/index.shtml>, and the University of Colorado.
Precise tracking files were generated based on the publicly available Two Line Orbital Elements (TLEs) obtained from Dr. T.S. Kelso’s Celestrack webpage <www.celestrak.com/NORAD/elements>, which provided sufficient accuracy to track GIOVE-B. (Note: The page is part of Center for Space Standards and Innovation /Analytical Graphics Inc.)
Observations were taken on May 7 during a pass over Boulder, Colorado. During this time, we observed the expected spectral signatures on the L1 and E5 frequencies; however, no signal was observed on the allocated E6 frequency.
The middle part of the L1 spectrum displays the MBOC modulation for the Galileo Open Service (OS) signals, while the two side lobes 15 MHz from the center frequency show BOC(15, 2.5) modulation for Galileo’s Public Regulated Service (PRS) signals. The E5 spectrum indicates AltBOC(15, 10) modulation.
We assume the asymmetry of the L1 or E5 spectrum is due to early stage components (filters and amplifiers) in the RF chain and not directly representative of the satellite signal. The issue probably arises from the filter connected to the antenna, not the filter in the software receiver. In other words, the asymmetry is from capturing the data, not processing the data.
Time domain data was collected independently at E5a and E5b for PRN code determination at those frequencies. The data were also used for L1 PRN code validation. . .
(For the complete article, including figures, graphs, and
ManufacturersIn our analysis, we used the 89600 Vector Signal Analyzer from Agilent Technologies, Palo Alto, California, USA.
Copyright © 2017 Gibbons Media & Research LLC, all rights reserved.