Earth's magnetic field, or magnetosphere, stretches from the planet's core out into space, where it meets the solar wind, a stream of charged particles emitted by the Sun.
For the most part, the magnetosphere acts as a shield to protect Earth from this high-energy solar activity.
But when this field comes into contact with the Sun's magnetic field - a process called "magnetic reconnection" - powerful electrical currents from the Sun can stream into Earth's atmosphere, whipping up geomagnetic storms and space weather phenomena that can affect high-altitude aircraft, as well as astronauts on the International Space Station.
By combining observations from the ground and in space, the team observed a plume of low-energy plasma particles that essentially hitches a ride along magnetic field lines - streaming from Earth's lower atmosphere up to the point, tens of thousands of kilometres above the surface, where the planet's magnetic field connects with that of the Sun.
In this region, which the scientists call the "merging point", the presence of cold, dense plasma slows magnetic reconnection, blunting the Sun's effects on Earth.
"Reconnection strips away some of our magnetic shield and lets energy leak in, giving us large, violent storms. These plasmas get pulled into space and slow down the reconnection process, so the impact of the Sun on the Earth is less violent," Foster said.
Foster approached Brian Walsh at NASA's Goddard Space Flight Center with data showing a plasma plume emanating from Earth's surface, and extending up into the lower layers of the magnetosphere, during a moderate solar storm in January 2013.
As it turns out, all three spacecraft crossed the point in the magnetosphere at which Foster had detected a plasma plume from the ground.
The team analysed data from each spacecraft and found that the same cold, dense plasma plume stretched up to where the solar storm made contact with Earth's magnetic field.
Foster said the observations from space validate measurements from the ground. The combination of space- and ground-based data give a highly detailed picture of a natural defensive mechanism in Earth's magnetosphere.
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