It uncovered how supergranulations respond to solar cycles, aiding cycle prediction.

• Supergranulations are giant convection cells (or patterns) that form a vast network structure on the surface of the Sun.

About Solar Cycle 

• The solar cycle is a periodic rhythm of magnetic activity that Sun undergoes every ~11 years.
  • Mechanism: The Sun is composed of electrically charged gas (plasma) that generates a massive magnetic field. 
  • Every 11 years, this field undergoes a flip (north-south poles switch)
• This periodic cycle undergoes distinct phases:
  • Solar Minimum: Cycle begins at solar minimum (low activity and few sunspots)
    • Sunspots: Dark, cooler regions on the Sun caused by strong magnetic activity.  
    • Despite being cooler, more sunspots correlate with the Sun emitting more total energy.

• Solar Maximum: As activity builds toward solar maximum, Sun becomes "stormy," featuring the highest number of sunspots and frequent eruptions. 

• Impact on Space Weather: During the more active phases, the Sun also experiences an increase in giant eruptions, such as solar flares and coronal mass ejections (CMEs). 
  • Solar Flares: Sudden bursts of X-rays and radiation (travelling at speed of light) caused by release of magnetic energy in sunspot regions. 
  • CMEs: Massive bubbles of plasma and magnetic fields flung into space
  • Impact: They can disrupt power grids, navigation systems, radio communications, and satellite operations, affect astronauts, induce geomagnetic storms affecting magnetic fields and events like Auroras etc.