Solar Sub-Surface Activity

PWOnlyIAS

April 30, 2025

Solar Sub-Surface Activity

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

Key Observations on Solar Sub-Surface Activity

  • Discovery
    • Plasma flows beneath the Sun’s surface converge at sunspot zones but reverse direction midway through the NSSL.
    • Despite influencing local motion, these flows don’t power the Sun’s larger-scale torsional oscillations, indicating deeper unknown drivers.Active regions generate rotational shear and meridional flow patterns influenced by the Coriolis effect, like Earth’s storm systems.

PW OnlyIAS Extra Edge

Helioseismology 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.

About the Solar Cycle

  • The solar cycle is an 11-year cycle during which the Sun’s magnetic field flips and returns to its original polarity.
  • Solar activity, including sunspots and flares, increases toward the solar maximum and declines at the solar minimum.
  • Sunspot count is a key indicator of solar cycle progression.
  • Magnetic changes during the cycle drive increased surface activity and energy releases.

Solar Surface Features and Their Characteristics

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

Impact of Solar Activities on Earth and Infrastructure

  • Space Weather Hazards: Increased solar activity can disrupt satellite operations, GPS signals, and radio communications.
  • Power Grid Vulnerability: Strong geomagnetic storms caused by CMEs can induce currents that damage transformers and electric grids.
  • Auroras: Solar storms trigger spectacular auroras near polar regions, a visual effect of solar particles interacting with Earth’s atmosphere.
  • Radiation Exposure: Astronauts and high-altitude flights face higher radiation risks during intense solar flares.
  • Navigation and Communication: HF radio blackouts and signal degradation can affect aviation and maritime operations during solar flares.
  • Climate Influence (Minor/Indirect): Long-term variations in solar output can influence Earth’s upper atmosphere temperature and circulation patterns.
  • Technological Systems: Satellites may experience drag changes or orbit perturbations due to atmospheric heating from solar energy bursts.

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UDAAN PRELIMS WALLAH
Comprehensive coverage with a concise format
Integration of PYQ within the booklet
Designed as per recent trends of Prelims questions
हिंदी में भी उपलब्ध
Quick Revise Now !
UDAAN PRELIMS WALLAH
Comprehensive coverage with a concise format
Integration of PYQ within the booklet
Designed as per recent trends of Prelims questions
हिंदी में भी उपलब्ध

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