|Mission Type:||Earth's magnetic field observation|
|Website:||ESA Swarm homepage|
|Cospar Id:||SWARM A: 2013-067B|
SWARM B: 2013-067A
SWARM C: 2013-067C
|Satcat:||SWARM A: 39452|
SWARM B: 39451
SWARM C: 39453
|Mission Duration:||4 years (planned)|
|Dry Mass:||369 kg|
|Launch Mass:||468 kg|
|Dimensions:||9.1 m × 1.5 m × 0.85 m|
|Launch Date:||22 November 2013,|
|Launch Site:||Plesetsk, Site 133/3|
|Orbit Regime:||Polar orbit|
|Orbit Periapsis:||Swarm A: ≤|
Swarm C: ≤
Swarm B: ≤
|Orbit Apoapsis:||Swarm A: ≤|
Swarm C: ≤
Swarm B: ≤
|Orbit Inclination:||Swarm A: 87.4°|
Swarm C: 87.4°
Swarm B: 88.0°
|Orbit Mean Motion:||15|
|Instruments:||VFM: Vector Field Magnetometer|
ASM: Absolute Scalar Magnetometer
EFI: Electric Field Instrument
LRR: Laser Range Reflector
|Trans Band:||S Band|
|Trans Frequency:||2 GHz|
|Trans Bandwidth:||6Mbit/s download|
|Programme:||Living Planet Programme|
Swarm is a European Space Agency (ESA) mission to study the Earth's magnetic field. High-precision and high-resolution measurements of the strength, direction and variations of the Earth's magnetic field, complemented by precise navigation, accelerometer and electric field measurements, will provide data for modelling the geomagnetic field and its interaction with other physical aspects of the Earth system. The results offer a view of the inside of the Earth from space, enabling the composition and processes of the interior to be studied in detail and increase our knowledge of atmospheric processes and ocean circulation patterns that affect climate and weather.
The overall objective of the Swarm mission is to build on the experience from the Ørsted and CHAMP missions and to provide the best ever survey of the geomagnetic field (multi-point measurements) and its temporal evolution, to gain new insights into the Earth system by improving our understanding of the Earth's interior and climate.
The Swarm constellation consists of three satellites (Alpha, Bravo and Charlie) placed in two different polar orbits, two flying side by side at an altitude of and a third at an altitude of .  The launch was delayed and rescheduled to 12:02:29 UTC on 22 November 2013, from Plesetsk Cosmodrome, Russia. ESA contracted Astrium to develop and build the three orbiters, while Eurockot provided the launch services.
Through a Canadian-European partnership, the Canadian Space Agency's CASSIOPE satellite's e-POP instrument suite was formally integrated as the fourth satellite in the Swarm constellation in 2018, joining Alpha, Bravo, and Charlie as Echo.
The payload of the three spacecraft consists of the following instruments:
The constellation is controlled by the European Space Operations Centre in Darmstadt, Germany. By the beginning of May 2014, Swarm had finished its in-orbit commissioning. Preliminary data indicates that the constellation is performing well as data received closely matches that from a previous German mission, CHAMP.
During the commissioning stage problems were discovered with the backup Magnetometer on the "Charlie" satellite, which led to "Bravo" satellite being placed in the lone high altitude orbit (510 km) and "Charlie" joining "Alpha" in the lower tandem orbit (462 km) to improve the resilience of the constellation. Commissioning data also indicated greater noise in data when a satellite was in view of the sun; the current theory is this is caused by differential heating in the satellite, but this has not been confirmed. Overall, the constellation is in good health and, due to accurate orbital insertion, has significant fuel reserves remaining.
In September 2016, scientists published a study that revealed a direct link between GPS blackouts of low-Earth-orbiting satellites and "thunderstorms" in the ionosphere. During the first two years of Swarm's operation their GPS connection was broken 166 times. The high-resolution observations from the satellite helped to link these outages to ionospheric thunderstorms 300–600 km in the Earth's atmosphere.
In December 2016, scientists announced that, by using data from the Swarm satellites, they had discovered a new feature in the Earth's outer core, a jet-stream of rapidly moving liquid iron moving at around 50 km per year. 
In April 2017, Swarm's data was used to confirm that Steve was a previously unrecognized atmospheric phenomenon.
In May 2020, Swarm revealed that Earth's magnetic field is gradually weakening in an area stretching from Africa to South America, which might cause technical disturbances in satellites orbiting Earth.