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magnetic reconnection

An X4.9 class solar flare erupts from the Sun.
Posted inNews

Scientists Claim a More Accurate Method of Predicting Solar Flares

Tim Hornyak, Science Writer by Tim Hornyak 5 October 202018 July 2023

Supercomputer 3D modeling of magnetic fields could help mitigate damage from geomagnetic storms.

Artist’s illustration of the Magnetospheric Multiscale mission spacecraft traveling through Earth’s magnetic field
Posted inResearch Spotlights

Deciphering Electron Signatures in Earth’s Magnetic Tail

by Mark Zastrow 21 February 202018 July 2023

A new analysis of spacecraft data collected near the tip of Earth’s magnetotail sheds light on how geomagnetic activity affects the motion of electrons in this region.

Posted inEditors' Highlights

Measuring the Magnetic Reconnection Rate in the Magnetotail

by Y. Wang 7 December 201818 July 2023

Both simulations and observations are used to measure the magnetic reconnection rate in the Earth’s magnetotail, suggesting that the rate is correlated with the intensity of a magnetic substorm.

Posted inEditors' Highlights

Evidence That Earth’s Forehead Controls the Wagging of its Tail

by Michael W. Liemohn 23 March 201818 July 2023

Yes, Earth has a tail, a magnetotail, and there is debate about how much Earth’s upper atmosphere plays a role in the controlling the dynamics of this region of space.

Researchers find new evidence suggesting lower energy particles may play an outsized role in space weather near Earth
Posted inResearch Spotlights

Jets of Ionospheric Cold Plasma Discovered at the Magnetopause

by David Shultz 24 October 201718 July 2023

The lower-energy particles may play a larger role in magnetic reconnection than previously believed, influencing space weather near Earth.

Four identical MMS spacecraft—one of which is pictured in this illustration—were launched in 2015 to study the process of magnetic reconnection.
Posted inResearch Spotlights

New Explanation for “Meandering” Electrons Orbiting Earth

by Mark Zastrow 11 May 201718 July 2023

A new study proposes a simpler theory to explain a class of electrons zipping around Earth, propelled by magnetic explosions.

Artist’s illustration of events on the Sun changing the conditions in near-Earth space.
Posted inResearch Spotlights

For Magnetic Reconnection Energy, O—not X—Might Mark the Spot

by Mark Zastrow 10 April 201718 July 2023

A new analysis of satellite data could upend conventional wisdom about how solar storms produce their dangerous radiation—not from X-shaped mergers of magnetic field lines but from swirling vortices.

The Sun’s magnetic field lines, shown here using a model, can further twist and loop after they encounter near-Earth space.
Posted inResearch Spotlights

Explaining Unexpected Twists in the Sun's Magnetic Field

by Mark Zastrow 4 April 201718 July 2023

New research shows how the Sun's magnetic field can shift when it approaches Earth, which can throw off space weather forecasts.

Researchers spot the cause of poleward boundary intensifications in Earth’s aurora
Posted inResearch Spotlights

Polar Interlopers in the Aurora

Leah Crane by L. Crane 9 March 201718 July 2023

A new study suggests that poleward boundary intensifications in the aurora are caused by fast flows of plasma from the poles into the auroral oval.

Researchers identify the role of plasma waves where the magnetic fields of Earth and the Sun interact.
Posted inResearch Spotlights

Plasma Waves Pinpointed at the Site of Magnetic Reconnection

by Mark Zastrow 17 February 201718 July 2023

When the Earth's and the Sun's magnetic fields meet, they realign in explosive and mysterious reconnections. Data suggest that plasma waves called kinetic Alfvén waves play a key role.

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