Page 2: Research news on Solar cycle

The solar cycle as a research area focuses on the quasi-periodic (~11-year) modulation of solar magnetic activity and its physical drivers, modeling, and impacts. It encompasses the study of dynamo processes in the solar interior, emergence and evolution of magnetic flux, sunspot number variability, and associated phenomena such as flares and coronal mass ejections. Researchers investigate cycle prediction methods, long-term modulation (e.g., grand minima and maxima), and coupling between solar radiative, particulate, and magnetic outputs and the heliosphere, planetary space weather, and climate-relevant upper-atmospheric processes, using observations, theory, and magnetohydrodynamic simulations.

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 ...

Young sunlike star reveals rapid two-year magnetic cycle

Scientists at the Leibniz Institute for Astrophysics Potsdam (AIP) have uncovered the intricate magnetic heartbeat of a distant star remarkably similar to our own sun—but much younger and more active. This study, part of ...

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, ...

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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