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.
Day will briefly turn into night across a swath of northern Spain on Aug. 12, when the moon will completely cover the sun during a rare total solar eclipse.
Space Exploration
Jul 8, 2026
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A researcher at The University of Alabama in Huntsville (UAH), a part of The University of Alabama System, has published a new study in The Astrophysical Journal suggesting that tiny charged dust grains near the sun may significantly ...
Astronomy
Jul 1, 2026
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The solar atmosphere is a turbulent and magnetized environment, with the release of magnetic energy readily manifesting as emission across the electromagnetic spectrum. Solar radio emission dominates the radio sky, with the ...
Astronomy
Jun 17, 2026
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Solar flares are the most explosive energy-release events in the solar corona, leading to intense particle acceleration, plasma heating and bulk plasma motions on short timescales. Core questions during solar flares remain ...
Astronomy
Jun 9, 2026
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Close to 100 scientists from all over Europe, the United States, and Japan are gathering this week at the Institute for Solar Physics (KIS) in Freiburg to present and discuss the first scientific results from the successful ...
Planetary Sciences
Jun 3, 2026
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When NASA scientists first observed a particular radio burst from the sun in August 2025, there was nothing unusual about it. But then the radio burst kept going. Typically, solar radio bursts like these last a few hours ...
Astronomy
May 15, 2026
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Solar radio bursts are intrinsically linked to the motion of their emitting source through the coronal and heliospheric plasma. Electron transport is mostly confined to magnetic field lines. These electrons move at a substantial ...
Astronomy
May 2, 2026
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It has been a dream of astronomers and solar scientists for ages. A new mission gives solar researchers a powerful new tool in their arsenal: on-demand, total solar eclipses. Launched in 2024, The European Space Agency's ...
Space Exploration
Apr 30, 2026
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At more than one million degrees, the sun's atmosphere—the corona—is incredibly hot; but not everywhere. Time and again, huge structures of significantly cooler solar plasma—about 10,000 degrees—appear within the corona. ...
Astronomy
Apr 22, 2026
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Since July 2025, the European Space Agency's pair of Proba-3 satellites has already created 57 artificial solar eclipses. So far, the mission has collected more than 250 hours of high-resolution videos of the sun's atmosphere, ...
Astronomy
Apr 13, 2026
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