Since the intensity of solar activity is currently lower than anticipated, the original plan of where to place the satellites at the beginning of science operations has been reviewed recently by the scientific community and experts in ESA.
Low solar activity means the satellites experience lower atmospheric drag, as clearly demonstrated by ESA’s GOCE mission.
Earth's protective shield
Swarm is tasked with measuring and untangling the different magnetic signals that stem from Earth’s core, mantle, crust, oceans, ionosphere and magnetosphere.
Launched together, the three identical Swarm satellites were released into adjacent orbits at an altitude of 490 km.
The satellites may be identical, but to optimise sampling in space and time their orbits are different – a key aspect of the mission.
The data acquired from different locations can be used to distinguish between the changes in the magnetic field caused by the Sun’s activity and those signals that originate from inside Earth.
The result for Swarm is a slightly different orbit configuration that will save satellite fuel at the beginning of the mission and offer a better return for science at a later stage.
Two satellites are now being lowered to an altitude of about 462 km and an inclination of 87.35°. They will orbit almost side by side, about 150 km apart as they pass over the equator. Over the life of the mission they will both descend to about 300 km.
The third satellite is being placed in a higher orbit of 510 km and at a different inclination of 87.75°, slightly closer to the pole.
The difference in inclination will cause a slow drift of the upper satellite relative to the path of the lower two at increasing angles. After three years, the fuel saved can be used to slow down the relative orbital drift.
Swarm continues to acquire excellent science data. Satellite constellation maintenance operations are proceeding, this is particularly relevant and important to achieving the bestpossible estimate of all contributors to the total magnetic field. Last year, early mission data were used to derive candidate solutions for the 2015 International Geomagnetic Reference Field (IGRF) model. The IGRF is a main field model that (by convention) is updated every five years, and which is used by practically all applications communities and services in need of geomagnetic data. IGRF-12, as the final 2015 model is called, is based on a combination of Swarm, historical satellite data and ground-based observatory data. In addition, a Swarm Initial Field Model, which includes also the computation of the crustal magnetic field at high spatial resolution, has been producedand made available to the community.
With the aim of making the best possible use of existing satellites, ESA and Canada have made a deal that turns Swarm into a four-satellite mission to shed even more light on space weather and features such as the aurora borealis.
In orbit since 2013, ESA’s three identical Swarm satellites have been returning a wealth of information about how our magnetic field is generated and how it protects us from dangerous electrically charged atomic particles in the solar wind.
Canada’s Cassiope satellite carries three instrument packages, one of which is e-POP. It delivers information on space weather which complements that provided by Swarm. Therefore, the mission teams began looking into how they could work together to make the most of the two missions.
To make life easier, it also just so happens that Cassiope’s orbit is ideal to improve Swarm’s readings.
And now, thanks to this international cooperation and formalised through ESA’s Third Party Mission programme, e-POP has effectively become a fourth element of the Swarm mission. It joins Swarm’s Alpha, Bravo and Charlie satellites as Echo.
Unlike our geographic North Pole, which is in a fixed location, magnetic north wanders. This has been known since it was first measured in 1831, and subsequently mapped drifting slowly from the Canadian Arctic towards Siberia.
One of the practical consequences of this is that the World Magnetic Model has to be updated periodically with the pole’s current location. The model is vital for many navigation systems used by ships, Google maps and smartphones, for example.
One of the many areas of research using information from Swarm focuses on explaining why the pole has picked up such a pace – and a subject being discussed at this week’s Living Planet Symposium.
Between 1990 and 2005 magnetic north accelerated from its historic speed of 0–15 km a year, to its present speed of 50–60 km a year. In late October 2017, it crossed the international date line, passing within 390 km of the geographic pole, and is now heading south.
In fact, recently, the World Magnetic Model had to be updated urgently because of the speed at which the pole is moving.
ESA’s Swarm mission is not only being used to keep track of magnetic north, but scientists are using its data to measure and untangle the different magnetic fields that stem from Earth’s core, mantle, crust, oceans, ionosphere and magnetosphere.
Our magnetic field exists because of an ocean of superheated, swirling liquid iron that makes up the outer core. Like a spinning conductor in a bicycle dynamo, this moving iron creates electrical currents, which in turn generate our continuously changing magnetic field.
Tracking changes in the magnetic field can, therefore, tell researchers how the iron in the core moves.
Research is showing that changes in the pattern of core flow between 1970 and 1999 elongated the Canadian lobe, significantly weakening its signature on Earth's surface, causing the pole to accelerate towards Siberia.
Simple models taking account of this process and describing future geomagnetic change predict that over the next decade the north magnetic pole will continue on its current trajectory and will travel a further 390–660 km towards Siberia.
What’s worse than dealing with deadly #SpaceDebris and violent #SpaceWeather?
Dealing with both at the same time!
@esa_swarm has dodged a potential collision at short notice, right in the middle of its 10-week climb to escape the Sun’s wrath:
https://esa.int/Space_Safety/Swarm_dodges_collision_during_climb_to_escape_Sun_s_wrath

"Collision avoided! 💥 In the wee small hours this morning Swarm-Alpha was moved out of harm's way - space debris in the form of a rocket body 🚀 that has been threatening our inner duo 🫣 Thanks to the hard work of the @esaoperations Space Debris Office for guiding us clear!
Collision avoided! 💥 No fireworks for Swarm Charlie this weekend thanks to the timely work of the space debris office, flight dynamics team & more @esaoperations, who swerved us out of the way of a small spacecraft early on Sunday morning 🚀 It’s busy up there!
It's getting busier. This is the 6th time we’ve had to move one of the Swarm satellites out of harm’s way this year, and the 22nd time we’ve had to call in a collision avoidance manoeuvre operation 🫣 That’s compared to 13 in the whole of 2021.