CRFS Arrays have been helping the European Space Agency stay in control of the RF spectrum at their Deep Space Antenna sites across the world. They perform a key role throughout the mission duration, protecting the huge sums invested in deep space missions by ensuring uninterrupted control of and communication with spacecraft millions of kilometers from Earth.

DSA-2, Cebreros (©The European Space Agency)

The challenge

Initially founded in 1975, the European Space Agency comprises 22 member countries, and is dedicated to space exploration and research. Current and recent high-profile missions include Gaia, which is mapping the structure of our own galaxy, the Milky Way, and Rosetta, the first mission to land on and study a comet.

The 35-meter Deep Space Antennas (DSA-1, outside Perth in Western Australia, DSA-2, outside Madrid in Spain and DSA-3, outside Malargüe in Argentina) are used to send commands and information from and to these interplanetary deep space missions. These antennas operate in the S-, X-, K- and Ka-band frequencies, and can be subject to interference from terrestrial sources – airfields, military bases, WiMAX etc. ESA is also in the process of expanding the capability of supporting spacecraft launch and early orbit phases (LEOP) by means of smaller aperture antennas from the Deep Space Antennas sites. To ensure that interference was not affecting these communications (particularly during mission critical times like launch and maneuvering), ESA needed a way to monitor RF spectrum activity around the Deep Space Antenna sites.

CRFS Array in situ at DSA-2 (©The European Space Agency)

The solution

ESA chose to deploy RFeye Array 300s at the DSA-1 and DSA-2 sites, which are controlled remotely from ESA Mission Control in Darmstadt. These Arrays provide spectrum monitoring and geolocation capabilities, both of which are key to their use at the antenna sites. Highly sensitive receivers allow for detailed and comprehensive surveys of the RF environment around the arrays. Geolocation can be carried out by both angle of arrival (AoA) and time difference of arrival (TDOA) techniques, depending on the number of arrays deployed. A single array can calculate a line of bearing to the source of a signal, while a second array can generate a second line of bearing that crosses the first at the source location. A third array adds the possibility of using TDOA in addition.

Close-up of CRFS Array at DSA-2 (©The European Space Agency)

The results


During the initial stages of mission planning, the arrays allow engineers to carry out extensive surveys of the RF spectrum in the area surrounding the antennas. Any potential sources of interference can then be investigated and steps taken to mitigate their impact (by, say, requesting that local military/airfield operators avoid transmissions in the required bands during mission launches).

Monitoring during launches

During the launch itself, it is absolutely critical to maintain uninterrupted communication. The Deep Space Antenna sites will be used to control the craft as well as receive information from it, so any interference at this stage could have a significant impact on the success of the mission. CRFS arrays allow not only a successful planning stage in order to eliminate potential sources of interference, but also real-time monitoring throughout the launch to ensure that this is the case, and allow for rapid geolocation of any unexpected sources that might occur.

Monitoring during missions

ESA missions frequently take months or years to complete, during which time the RF environment around the antennas may significantly change (as, for example, nearby cities grow, or telecoms technologies advance). CRFS arrays allow for ongoing monitoring of the situation, to ensure that information can continue to be both sent to and received from the spacecraft throughout the mission.


The 24/7 monitoring that CRFS Arrays provide ensures complete peace of mind, protecting missions with budgets reaching billions of euros from being disrupted by external interference. Piermario Besso, Head of the Antenna and Infrastructure section at ESA’s European Space Operations Centre in Darmstadt, summarizes: “The CRFS Array 300 is what we needed at ESA to monitor the Deep Space Antenna sites. With one Array at each site we are able to perform accurate Angle of Arrival identification of potential ground interference in order to electromagnetically safeguard our most critical frequency bands”.

Array 100

Vehicle-mounted, transportable or ground-fixed installations

Array 300

Outdoor ground-fixed or vehicle-mounted installation complete with IP65-rated radome

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