The NSSL, extending about 35,000 km beneath the Sun’s surface, is a region where rotational dynamics undergo dramatic ...

Scientists using South Africa’s MeerKAT telescope have peered into the interstellar medium like never before, uncovering ...

A burst of solar wind triggered a planet-wide heatwave in Jupiter’s upper atmosphere, say astronomers at the University in ...

The National Science Foundation’s Daniel K. Inouye telescope debuted a close-up of the sun captured by its new, ...

In a groundbreaking achievement for solar astronomy, the Daniel K. Inouye Solar Telescope (DKIST), the world’s largest solar ...

and the adjacent layer of the solar atmosphere, the chromosphere. The complex interaction of hot plasma flows and changing magnetic fields there holds the key to a better understanding of the ...

The interstellar plasma is turbulent and scatters pulsar radio waves slightly away from a direct, straight line path. The ...

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With the recently completed Visible Tunable Filter (VTF), the dynamics of solar plasma can now be fundamentally ... at different heights in the solar atmosphere. This is achieved by taking several ...

Image: ESA & NASA/Solar ... solar atmosphere—the corona—at wavelengths far beyond what our eyes can see. Closer to the solar surface are dark, filamentous prominences—solar plasma—arcing ...

This increase in radiation likely had major effects on Earth’s atmosphere, possibly altering its chemistry and circulation patterns ... interaction between solar plasma and planetary magnetic ...