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Top-class technology that inspires


© EADS Astrium

The Galileo navigation system will comprise 30 satellites in total, plus the associated ground infrastructure. Twenty-seven satellites will be required to operate, while three others will be kept on stand-by as reserves. The satellites will circle the Earth on three orbital planes at an altitude of approximately 23,300 km. They will transmit time signals and the co-ordinates of their orbital position to the ground receivers, which use the signal propagation time to determine their distance from the satellite and therefore their position relative to the surface of the globe. To calculate its exact position, a ground receiver needs to receive signals from at least four satellites. The ability to determine a position accurately worldwide to within one metre calls for technology that has not previously existed in space. The in-orbit validation (IOV) phase is an important milestone in setting up the system and is laying the foundations for Galileo. The Giove-B test satellite is the transition to IOV and will perform pioneering work in space.

Giove-B is equipped with top-class technology. In addition to conventional rubidium clocks, a space passive hydrogen maser (S-PHM) will be used for the first time. This atomic clock will be the most precise timekeeper ever to have been used in space and is the key to the greater accuracy that Europe’s navigation system will offer compared to the American GPS. “The satellite is carrying the same type of leading-edge technology that will be used in the current system,” says Dr Oliver Juckenhöfel, head of future projects at Astrium. “This will provide a concrete basis for Galileo, making it possible for the structures, applications and services involved to be planned at an early stage.”

The hydrogen maser
The hydrogen maser
© EADS Astrium / Raoul Kieffer

Trying to explain atomic clocks in a way that everyone can understand is at least as difficult as trying to grasp how they actually function. For thousands of years, humankind has used natural constants to structure their lives according to time. Initially, the focus was on establishing the best days for sowing and harvesting. Later, it shifted to general curiosity about the world. The natural constants used by humans to measure time soon faded into the background. In 1736, a maritime clock developed by John Harrison laid the basis for the navigation principle still used today. The measurements made with his ‘H1’ and its follow-up models made it possible very early on to determine the East–West position of ships on their journeys in addition to their North–South position, which was determined using star maps. Ever since then, the accuracy of clocks has also been a gauge of position, not only on ships. Some time later the atom, along with its properties in different states, was discovered as a constant for measuring temporal cycles. This led to the development of a hydrogen atom clock in the mid-20th century that measures time a thousand times more accurately than even the most precise atomic clock in the world. Such a ‘hydrogen maser’ will also be applied in the Galileo programme. In theory, this maser only errs by one second every million years.

This atomic clock is the ideal companion for any navigation satellite when it comes to ensuring the best possible positioning accuracy. Car drivers who have so far relied on GPS to guide them can now look forward to even more reliable navigation systems. The more accurately satellites and ground stations are temporally coordinated with one another, the more precise the maps and directions become. A deviation of just one millisecond, i.e. one thousandth of a second, in space results in an error of 300 metres on Earth.

Securing the Galileo signals
Securing the Galileo signals
© ESA / Image P. Carril

Galileo will be the first set of satellites to be sent by Europe into a medium earth orbit (MEO). Although this orbit is particularly stable, it entails a greater exposure to radiation than a traditional geostationary orbit. In order to determine the extent of this burden, Giove-B will also carry radiation gauges. At the heart of Giove-B’s navigation payload, and that of the subsequent Galileo satellites, is a signal generator (NSGU) which will produce the navigation signals required to seize and use the reserved transmission frequencies – the satellites’ main task. This will guarantee an uninterrupted signal up until the in-orbit validation phase, even after the Giove-A satellite launched in 2005 as a pure frequency holder has reached the end of its service life. Galileo will use the frequency bands L1, E5 and E6. Giove-B already possesses full broadcasting ability for the signals that are actually applicable to the complete system. The MBOC code, in particular, which was agreed upon by the USA and the European Union as recently as last year, is already being implemented by Giove-B today. This code will form the overall basis for ensuring the interoperability and compatibility of the Galileo system with the next generation of GPS satellites.

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