Research news on Solar corona

The solar corona as a research area focuses on the physical processes governing the Sun’s outer atmosphere, characterized by low densities, high temperatures (∼10⁶ K), and complex magnetic structures. It integrates observational solar physics, plasma astrophysics, and magnetohydrodynamics to study coronal heating, magnetic reconnection, wave propagation, flares, and coronal mass ejections. Research emphasizes multi-wavelength diagnostics (EUV, X-ray, radio), spectropolarimetry, and numerical modeling to infer coronal magnetic fields, energy transport, and particle acceleration. This domain is central to understanding space weather, heliospheric conditions, and the coupling between the photosphere, chromosphere, and interplanetary medium.

NASA probe data suggests a more complex sun's magnetic engine

A Southwest Research Institute-led study found that protons and heavy ions react differently to solar magnetic reconnection events, revealing a more complex magnetic engine powering the solar wind. Magnetic reconnection converts ...

'Miracle': Europe reconnects with lost spacecraft

The European Space Agency announced Thursday it has re-established communication with a spacecraft that is part of its Proba-3 mission, after losing contact with the satellite a month ago.

Eclipse research finds turbulent times in the sun's corona

Researchers at the University of Hawaiʻi have uncovered new clues about how energy moves through the sun's outer atmosphere, using one of nature's rarest events as their window: total solar eclipses. Drawing on more than ...

Kissing the sun: Unraveling mysteries of the solar wind

Using data collected by NASA's Parker Solar Probe during its closest approach to the sun, a University of Arizona-led research team has measured the dynamics and ever-changing "shell" of hot gas from where the solar wind ...

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