Improving the Resilience to Interference of a GNSS Reference Station

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Improving the Resilience to Interference of a GNSS Reference Station Dr. Youssef Tawk Product Application Specialist Leica Geosystems

Outline What is Interference for GNSS Reference Station? Interference Sources Leica Geosystems ITK Test Case Examples Summary 2

What is Interference for GNSS Reference Station Interference is a phenomenon where undesired signals enter the GNSS reference station receiver and mix with the satellite navigation signals to disrupt the operation of the receiver, causing: Partial or total loss of lock Reduced and/or noisy SNR Reduced ability of the receiver to properly operate to provide reliable raw observation data, corrections, and compute a position. 3

Interference Sources Increasing amount of sources of GNSS interference In-Band: Within band of GNSS signal. Intentional jammers, other RF spectrum users (legal or not) Near-Band: Close to band of GNSS signal. Includes legal transmissions such as Globalstar and long-range air traffic control radar Out of band Harmonics: Far removed transmitters that may have spurious harmonic emissions overlapping GNSS band ARSR-4 Radar Self Interference: Electronics integration often requires solving in-band, near-band and out of band harmonics from within the product itself 4

Leica Geosystems ITK ITK stands for Interference Tool Kit A software upgrade on Leica s GR30/50 reference station receivers: Allows the user to visualize the frequency spectrum: Easily detects interference by visual inspection Automatic Interference detection Adaptive interference rejection technologies for strong interference situations using three methods: HDR mode - High dynamic range mode performing a wideband mitigation Band pass filter Adaptive notch filter 5

Test case examples: In band Continuous Wave (1582.5 MHz, -44 dbm) Out of band Narrowband (1625 MHz, 1.2288 MHz CDMA, -14 dbm) Out of band Wideband (1625 MHz, 10 MHz, LTE, -28 dbm) Receiver performance before and after mitigation: Average GPS L1 C/No, over all satellites tracked for each epoch Number of Satellites tracked RTK position accuracy 6

In Band Continuous Wave Normal/Healthy GPS L1 Spectrum 7

In Band Continuous Wave In Band Continuous Wave Interferer 8

In Band Continuous Wave Mitigated In Band CW Interferer (HDR mode & Notch filter applied) 9

In Band Continuous Wave Before Mitigation After Mitigation Average C/No (db-hz) Satellites Tracked 10 3D RTK Position Error (m)

Out of Band Narrowband Out of Band Narrowband Interferer (e.g. GlobalStar) 11

Out of Band Narrowband Mitigated Out of Band Narrowband Interferer (HDR Mode) 12

Out of Band Narrowband Before Mitigation After Mitigation Average C/No (db-hz) Satellites Tracked 13 3D RTK Position Error (m)

Out of Band Wideband 10 MHz LTE Centred at 1625 MHz 14

Out of Band Wideband Mitigated OOB WB Interferer (HDR Mode) 15

Out of Band Wideband Before Mitigation After Mitigation Average C/No (db-hz) Satellites Tracked No Position 16 3D RTK Position Error (m)

Summary Interference Tool Kit (ITK) Power Spectrum Visualisation and Mitigation technologies for Leica s GR30 / GR50 reference station receivers Demonstrated and will become available as future software upgrades Efficient interference rejection of strong interferers becomes possible In-Band Continuous Wave Out of Band Narrow band Out of Band Wide band Satellite tracking and signal quality can be largely preserved High quality Precise Positioning remains possible 17

THANK YOU FOR YOUR ATTENTION! The best answers combine the smartest solutions The Leica Spider family of products provide all you need for smart solutions. From single base stations to comprehensive infrastructure RTK networks. GNSS Networks and Reference Stations Smart Solutions from Leica Geosystems