Search Publications

Global-scale magnetosphere convection driven by dayside magnetic reconnection
DOI: 10.1038/s41467-024-44992-y Bibcode: 2024NatCo..15..639D

Branduardi-Raymont, Graziella; Wang, Chi; Dai, Lei +8 more

Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state convection within the closed part of the magnetosphere relies on magnetic reconnection in the nightside magnetospheric tail. Nevertheless, time-dependent models of the Dungey cycle suggest an alternative scenario whe…

2024 Nature Communications
Cluster 16
The variable source of the plasma sheet during a geomagnetic storm
DOI: 10.1038/s41467-023-41735-3 Bibcode: 2023NatCo..14.6143K

Asamura, K.; Kistler, L. M.; Mouikis, C. G. +8 more

Both solar wind and ionospheric sources contribute to the magnetotail plasma sheet, but how their contribution changes during a geomagnetic storm is an open question. The source is critical because the plasma sheet properties control the enhancement and decay rate of the ring current, the main cause of the geomagnetic field perturbations that defi…

2023 Nature Communications
Cluster 6
Earth's magnetosphere and outer radiation belt under sub-Alfvénic solar wind
DOI: 10.1038/ncomms13001 Bibcode: 2016NatCo...713001L

Lugaz, Noé; Farrugia, Charles J.; Schwadron, Nathan A. +3 more

The interaction between Earth's magnetic field and the solar wind results in the formation of a collisionless bow shock 60,000-100,000 km upstream of our planet, as long as the solar wind fast magnetosonic Mach (hereafter Mach) number exceeds unity. Here, we present one of those extremely rare instances, when the solar wind Mach number reached ste…

2016 Nature Communications
Cluster 24
Observations of discrete harmonics emerging from equatorial noise
DOI: 10.1038/ncomms8703 Bibcode: 2015NatCo...6.7703B

Dandouras, Iannis; Walker, Simon N.; Balikhin, Michael A. +7 more

A number of modes of oscillations of particles and fields can exist in space plasmas. Since the early 1970s, space missions have observed noise-like plasma waves near the geomagnetic equator known as `equatorial noise'. Several theories were suggested, but clear observational evidence supported by realistic modelling has not been provided. Here we…

2015 Nature Communications
Cluster 99
Wave energy budget analysis in the Earth's radiation belts uncovers a missing energy
DOI: 10.1038/ncomms8143 Bibcode: 2015NatCo...6.8143A

Artemyev, A. V.; Agapitov, O. V.; Mozer, F. S. +2 more

Whistler-mode emissions are important electromagnetic waves pervasive in the Earth's magnetosphere, where they continuously remove or energize electrons trapped by the geomagnetic field, controlling radiation hazards to satellites and astronauts and the upper-atmosphere ionization or chemical composition. Here, we report an analysis of 10-year Clu…

2015 Nature Communications
Cluster 58
Solar wind entry into the high-latitude terrestrial magnetosphere during geomagnetically quiet times
DOI: 10.1038/ncomms2476 Bibcode: 2013NatCo...4.1466S

Wei, Y.; Zhang, H.; Zong, Q. -G. +14 more

An understanding of the transport of solar wind plasma into and throughout the terrestrial magnetosphere is crucial to space science and space weather. For non-active periods, there is little agreement on where and how plasma entry into the magnetosphere might occur. Moreover, behaviour in the high-latitude region behind the magnetospheric cusps, …

2013 Nature Communications
Cluster 62