Page 4: 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.

NASA analysis shows sun's activity ramping up

The sun has become increasingly active since 2008, a new NASA study shows. Solar activity is known to fluctuate in cycles of 11 years, but there are longer-term variations that can last decades. Case in point: Since the 1980s, ...

Influence of the planets may subdue solar activity

Our sun is about five times less magnetically active than other sunlike stars—effectively a special case. The reason for this could reside in the planets in our solar system, say researchers at the Helmholtz-Zentrum Dresden-Rossendorf ...

Solar cycles and climate: Expert shares what you need to know

Solar Maximum 2025 is the expected peak of solar activity in Solar Cycle 25, characterized by heightened sunspots, solar flares, and coronal mass ejections. This peak is anticipated around mid to late 2025, coinciding with ...

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