HelioSwarm is a NASA heliophysics mission that will launch a constellation of 9 spacecraft to investigate the fundamental properties of plasma turbulence.  The HelioSwarm spacecraft will fly in formation through the solar wind – the cloud of charged particles that flow from the Sun.   One central hub spacecraft will gather data from eight smaller node spacecraft, characterising collisionless plasma turbulence in 3 dimensions, on multiple scales, for the first time. 

Each spacecraft will fly a magnetometer (a magnetic field instrument) designed and built at Imperial College London.   

Facts

  • Launch Readiness date: 2029 
  • Orbit: Lunar resonance orbit around Earth (approximately 60 by 11 Earth radii) 
  • Mission Duration: nominal 1 year 
  • Imperial College involvement: Lead, magnetometer instrument (MAG) 
  • MAG: Fluxgate sensor; electronics box and power supply developed in the Space
  • Magnetometer Laboratory 
  • Science Lead: Prof. Tim Horbury, Imperial College London 
  • Instrument Manager: Helen O'Brien, Imperial College London 
  • Funding Agency: UKSA 

External Links

UNH HelioSwarm | NASA HelioSwarm | UK Space Agency