EGU23-3621
https://doi.org/10.5194/egusphere-egu23-3621
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Review of coordinated measurements with Swarm and Cluster : multi-scale magnetospheric and ground currents

Malcolm Dunlop1,2, Xiangcheng Dong3, Xin Tan2, Junying Yang2, Dong Wei4, and Chao Xiong5
Malcolm Dunlop et al.
  • 1RAL Space, STFC, DIDCOT, Oxfordshire, OX11 0QX, United Kingdom of Great Britain – England, Scotland, Wales (m.w.dunlop@rl.ac.uk)
  • 2School of Space and Environment, Beihang University, 100191, Beijing, China
  • 3Department of Geophysics, Yunnan University, Kunming, China
  • 4Department of Earth and Space Sciences, Southern University of Science and Technology, Shenzhen, China
  • 5Department of Space Physics Wuhan University, Wuhan, 430072, China

We review a number of studies, undertaken during the 10 years of Swarm, using distributed, multi-scale measurements arising from the combination with Cluster, MMS and ground based arrays. The scaling, coherence and correlation of field-aligned current sheets (FACs) connecting different regions of the magnetosphere have been explored with associated analysis techniques using these multi-point measurements at both low (LEO) and high altitudes, and in relation to (R1/R2) auroral boundaries. Individual events can map to conjugate current density distributions at the magnetopause and ring current and regions in between; as well as to associated  ground signatures, driven by the external conditions. Large and small-scale (MLT) trends in FAC orientation can be inferred from dual-spacecraft (e.g. the Swarm A&C spacecraft). Conjugate effects seen in ground (dH/dt), ionospheric and magnetospheric magnetic signals show that intense, coherent FA currents can take place in the polar cusp during the main phase of a geomagnetic storm and at near tail local times during substorm activity, at different altitudes. In the former event the mesoscale FACs show vertical scaling and a corresponding geomagnetic disturbance, driven by unsteady magnetic reconnection at the magnetopause. In the latter event, the most intense dH/dt is shown to be associated with FACs driven into the ionosphere by the arrival of bursty bulk flows BBFs at geosynchronous orbit (linked via a modified sub-storm current wedge, SCW). In situ ring current morphology can also be investigated by MMS, THEMIS and Cluster during the Swarm era, and can be compared to distributions of R2-FACs.

How to cite: Dunlop, M., Dong, X., Tan, X., Yang, J., Wei, D., and Xiong, C.: Review of coordinated measurements with Swarm and Cluster : multi-scale magnetospheric and ground currents, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-3621, https://doi.org/10.5194/egusphere-egu23-3621, 2023.