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An international team of solar physicists have traced giant tides of plasma beneath the Sun’s surface at a region called near-surface shear layer (NSSL).
Using over a decade of data and a technique called helioseismology, the team has tracked how these plasma currents change over time in sync with the Sun’s 11-year sunspot cycle
PW OnlyIAS Extra EdgeHelioseismology is the study of sound waves traveling through the Sun’s interior, used to map its internal structure, dynamics, and activity by analyzing surface oscillations and vibrations. The Near-surface shear layer (NSSL): The Near-surface shear layer (NSSL) , which is present about 35,000 km deep, shows varying rotational behavior with depth and time, influenced by sunspot-related magnetic fields. |
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Feature | Description | Impact/Behavior |
Sunspots | Dark, cooler regions with intense magnetic activity | Increase during solar maximum, affect magnetic dynamics |
Solar Flares | Sudden, intense explosions of energy | Emit radiation across spectrum; disrupt satellites and comms |
Coronal Mass Ejections (CMEs) | Massive bursts of solar plasma and magnetic field | Can cause geomagnetic storms on Earth |
Plasma Tides | Flows of ionized gas influenced by solar dynamics | Converge and diverge beneath surface, shaped by Coriolis effect |
Torsional Oscillations | Global-scale solar interior flow patterns | Not powered by shallow flows; hint at deeper unknown forces |
Meridional Flows | Pole-to-equator currents beneath the surface | Affected by sunspots and Coriolis forces |
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