Simple testing of multi-frequency, multi-constellation GNSS receivers

The R&S®SMBV100B vector signal generator can be turned into a multi-frequency, multi‑constellation GNSS simulator for receiver tests in the lab.

SMBV100B vector signal generator

Su misión

All available global navigation satellite systems (GNSS), including modernized GPS, GLONASS, Galileo and BeiDou, already offer, or at least have planned, positioning services on multiple frequencies in the L-band. Using various signals on different carriers helps significantly improve a receiver’s position estimation (navigation solution) in terms of accuracy, reliability and resilience to interference. This is because receivers working on L1, L2 and L5 signals are able to calculate the ionospheric delay and, as a result, remove the corresponding position error. Considering all available GNSS, there are more than 120 navigation satellites in space. On average, around 30 satellites are visible from most locations around the world. Cada uno de estos vehículos espaciales (SV) proporciona múltiples servicios de posicionamiento en distintas frecuencias. The signals of the visible satellites are not only received via line of sight (LOS), but are also reflected from nearby buildings or other obstacles.

Naturalmente, los requisitos en el lado del receptor aumentan con la evolución en las constelaciones de los GNSS, y hacer simulaciones realistas se hace más complejo, además de costoso en el aspecto computacional.

Engineers developing new receivers capable of multiconstellation signal processing require a highly accurate and versatile simulator to validate functionality and performance. The simulator must be able to provide extremely realistic signals for any combination of GNSS (e.g. GPS, Galileo, GLONASS, BeiDou) and frequencies. Por lo tanto, su presupuesto para canales debe ser lo suficientemente amplio para cubrir todos los vehículos espaciales visibles, el elevado número de servicios de posicionamiento (como el L1 C/A o el E1 OS) y también los ecos reflejados. And engineers must be able to take into account signal propagation characteristics such as tropospheric and ionospheric effects, system characteristics such as orbit and clock errors and the user environment, e.g. shadowing or other impairments.

The SMBV100B can generate GNSS signals for all frequency bands at once, simplifying multi-frequency test setups.
The R&S®SMBV100B can generate GNSS signals for all frequency bands at once, simplifying multi-frequency test setups.

Solución Rohde & Schwarz

Thanks to its flexible option concept, the R&S®SMBV100B can be used for a wide variety of test cases. Starting with single-frequency signals for receiver development and production testing, the GNSS simulator can be upgraded by software to support multi-constellation, multi-frequency scenarios, which allows advanced receiver characterization and performance testing.

Se pueden generar multitud de distintos escenarios con señales GPS, Galileo, GLONASS y BeiDou en tiempo real con hasta 102 canales. For the receiver, the simulated location can be static, but users can also import waypoint files to set up dynamic scenarios. De este modo, es posible simular incluso cambios de posición del vehículo. The antenna pattern can be changed individually and the installation location of the antenna can be set. Potential shadowing caused by the antenna housing can be modeled using vehicle body mask files.

Multi-constellation, multi-frequency scenarios can be configured with the GNSS simulator of the R&S®SMBV100B
Fig. 2: Multi-constellation, multi-frequency scenarios can be configured in an easy, user-friendly and efficient way with the GNSS simulator of the R&S®SMBV100B.

Aplicación

Configuración de escenarios multifrecuencia

Thanks to the high modulation bandwidth of the R&S®SMBV100B, it is possible to simultaneously generate signals for all important GNSS frequency bands such as L1, L2 and L5 on only one RF output without the need for additional equipment such as external combiners. This makes testing multi-frequency receivers much simpler.

To evaluate the error mitigation capabilities of multi-frequency receivers, different ionospheric models can be applied. Standard models such as the Klobuchar model used by GPS or the NeQuick model proposed by Galileo are available, but historical models can also be loaded.

Utilización de múltiples constelaciones de GNSS

The R&S®SMBV100B can generate signals for up to 102 channels from different GNSS to support receiver tests with complex test signals. This makes it easy to set up realistic scenarios where SVs from multiple GNSS are present. Por ejemplo:

Sistema N.º de vehículos espaciales Señales N.º de canales
GPS 8 L1 C/A, L5 8 × 2 = 16
Galileo 8 E1 OS, E5a, E5b 8 × 3 = 24
GLONASS 7 L1 C/A, L2 C/A 7 × 2 = 14
Total 23 54

If the test case requires a mixed GNSS signal with a predefined minimum and maximum number of satellites, these limits can be set per GNSS. All satellites can be manually switched on or off on-the-fly, i.e. the simulation is not interrupted.

It is also possible to vary the individual power levels or assign pseudorange errors to each satellite without recalculating the scenario – ideal for testing the receiver autonomous integrity monitoring (RAIM) capabilities of a receiver. The real-world situation of disappearance and reappearance of satellites can be observed on the built-in simulation monitor (see Fig. 3).

GNSS constellations and satellite power levels can be observed on the built-in simulation monitor.
Fig. 3: GNSS constellations and satellite power levels can be observed on the built-in simulation monitor.

Características y ventajas

The R&S®SMBV100B is the perfect solution for testing multi-constellation receivers. Este ofrece condiciones de prueba realistas y reproducibles en un entorno controlado de laboratorio con las siguientes características clave:

  • Compatible con escenarios multiconstelación con hasta 102 canales
  • Support of all important global navigation satellite systems (GNSS)
  • GPS L1/L2 (C/A and P code), L2C, L5
  • GLONASS L1/L2 C/A code
  • Galileo E1, E5a, E5b
  • BeiDou B1I/B2I
  • QZSS/SBAS L1 C/A
  • Easy configuration of multi-frequency scenarios