However, there’s a catch. Before electrons can be accelerated by these shock waves, they need to contain a certain amount of energy to begin with. Nobody knows how electrons gain this initial energy.

During this event, electrons in Earth's foreshock region—an area where the solar wind is predisturbed by its interaction with the bow shock—reached unprecedented energy levels, surpassing 500 keV.

The magnetosheath, the region downstream of the Earth's bow shock, is one of the most typical turbulent environments and is very suitable for studying turbulence dissipation. By analyzing ...

During this event, electrons in Earth's foreshock region -- an area where the solar wind is predisturbed by its interaction with the bow shock -- reached unprecedented energy levels, surpassing ...

An example effect is the bow shock created as the magnetosphere passes ... an encounter with a magnetic reconnection site in the Earth’s magnetosphere.

China’s Tiangong space station and ambitious lunar and Mars exploration programs signal its intent to dominate beyond Earth’s ...