Page 3: Research news on Solar activity

Solar activity as a research area focuses on the study of time-varying phenomena originating from the Sun’s magnetic field, including sunspots, flares, coronal mass ejections, solar wind variability, and associated irradiance changes. It integrates solar physics, plasma astrophysics, and space weather science to understand magnetic field generation via the solar dynamo, energy storage and release in the corona, and particle acceleration processes. This field employs multi-wavelength observations, in situ spacecraft measurements, and magnetohydrodynamic modeling to quantify solar variability and its coupling to the heliosphere, planetary magnetospheres, and upper atmospheres, with implications for technological systems and long-term space climate.

New model predicts solar storm particle acceleration and escape

The sun, a searing hot sphere of gas primarily composed of hydrogen and helium, boasts surface and outer atmospheric temperatures ranging from 10,000 to 3.6 million degrees Fahrenheit on its surface and its atmosphere's outermost ...

Video: Our sun is the star in a new simulation

NASA supercomputers are shedding light on what causes some of the sun's most complex behaviors. Using data from the suite of active sun-watching spacecraft currently observing the star at the heart of our solar system, researchers ...

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