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magnetic reconnection

magnetic-reconnection-fuels-slow-solar-winds
Posted inResearch Spotlights

Spotting the Source of Slow Solar Wind

Kate Wheeling, freelance science writer by Kate Wheeling 24 August 201618 July 2023

A new study suggests that magnetic reconnection may fuel slow solar winds, which top out at speeds below 500 kilometers per second.

Posted inEditors' Vox

First Results from NASA’s Magnetospheric Multiscale Mission

by Andrew Yau 18 August 201618 July 2023

Understanding magnetic reconnection is important in the context of Sun-Earth Connection, because of the resulting exchange of mass and energy, and the large amount of energy involved.

Solar wind interacts with Venus's ionosphere to produce magnetotail.
Posted inResearch Spotlights

Solar Wind Disconnects Venus’s Magnetotail

by A. K. Higginson 27 June 201618 July 2023

Polarity reversals in the solar wind magnetic field disconnect the magnetic field trailing behind Venus, allowing ions from the atmosphere to escape.

Posted inEditors' Vox

Chasing Down the Slow Solar Wind

by L. E. Kepko 20 June 201618 July 2023

The Sun's plasma blasts Earth’s magnetosphere at more than a million miles per hour. The fastest pours from holes in the corona, but until recently the source of the "slow" solar wind was a mystery.

Posted inResearch Spotlights

Electrons Thrown Off Course in Near-Earth Magnetic Reconnection

by A. K. Higginson 26 April 201618 July 2023

NASA Magnetospheric Multiscale (MMS) mission detects energy differences in electrons scattered by magnetic reconnection.

Interactions between the Sun’s and Earth’s magnetic fields (shown here as white lines) result in geomagnetic activity and auroras that are visible from Earth’s surface.
Posted inScience Updates

Exploring New Knowledge on Magnetospheric Interactions

by J. R. Kan and J. L. Burch 6 April 201618 July 2023

AGU Chapman Conference on Magnetospheric Dynamics; Fairbanks, Alaska, 27 September to 2 October 2015

Dipolarization fronts (DFs), bursty bulk flows (BBFs), flux transfer events (FTEs), and Kelvin-Helmholtz instability (KHI) in a high-resolution simulation of an idealized substorm.
Posted inScience Updates

Great Mysteries of the Earth's Magnetotail

by M. I. Sitnov, V. G. Merkin and J. Raeder 21 March 201618 July 2023

Workshop on Magnetotail Reconnection Onset and Dipolarization Fronts; Laurel, Maryland, 16–18 September 2015

Posted inResearch Spotlights

Satellites Test Theory of Magnetic Reconnection

by Mark Zastrow 2 February 201618 July 2023

A quartet of satellites flying through Earth's magnetic field measures its interaction with the Sun's and puts a theory about their reconnection to the test.

Posted inResearch Spotlights

X Marks the Spot of Magnetic Islands in Space

by Mark Zastrow 17 June 201518 July 2023

At the edge of Earth's magnetic field, satellites have found X-shaped fields and fast-moving "islands" of magnetism that could shed light on the physics of solar storms.

Posted inFeatures

Why Does the Aurora Flare Up?

by S.-I. Akasofu 14 April 201518 July 2023

The spectacular auroras that circle Earth's geomagnetic poles and burst with colorful displays during geomagnetic storms have mystified humanity for millennia. Now scientists are uncovering their secrets.

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