Important Geophysical phenomena

GS-1

SOLAR ROTATION

Kodaikanal Solar Observatory Digitized Data probes Sun’s rotation over the century.

Who conducted the study?

  • Researchers led by a Ph.D. student from the Aryabhatta Research Institute of Observational Sciences (ARIES), an autonomous institute under Department of Science and Technology (DST), Govt. of India
  • Collaborators from Max Planck Institute for Solar System Research, Goettingen, Germany.
  • Collaborators from Southwest Research Institute, Boulder, USA. The researchers studied the solar rotation by tracing sun spots from century-old digitalized films and photographs.
  • The old films and photographs were taken at the Kodaikanal Solar Observatory (KoSO) of the Indian Institute of Astrophysics (Bengaluru).
  • This estimation would help study magnetic field generated in the interior of the Sun, which causes sunspots and results in extreme situations like the historical mini-ice age on Earth (absence of sunspots).
  • It could also help predict solar cycles and their variations in the future.

Solar rotation:

  • The Sun rotates more quickly at its equator than at its poles.
  • Over time, the Sun’s differential rotation rates cause its magnetic field to become twisted and tangled.
  • The tangles in the magnetic field lines can produce strong localized magnetic fields.
  • When the Sun’s magnetic field gets twisted, there are lots of sunspots.
  • The sunspots which form at the surface with an 11-year periodicity are the only route to probe the solar dynamo or solar magnetism inside the Sun and hence measure the variation in solar rotation.
  • The solar rotation period is 24.47 days at the equator and almost 38 days at the poles. The average rotation is 28 days.

 

SOURCE: DTE

 

 

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