KNOWLEDGE BASE

ADITYA-L1 MISSION: SOLAR ERUPTIONS

ISRO’s Aditya-L1 used its VELC instrument to generate Doppler velocity images of the solar corona, helping study plasma motion and assess Earth-directed Coronal Mass Ejections (CMEs).

News: ISRO’s Aditya-L1 used its VELC instrument to generate Doppler velocity images of the solar corona → Helps determine solar plasma motion and improve assessment of Earth-directed CMEs.

Aditya-L1 Mission

  • Launched by: ISRO → India’s first dedicated space-based solar observatory.
  • Location: Sun–Earth L1 point, about 1.5 million km from Earth.
  • Objective: Study the Sun’s atmosphere + solar activity + space weather.

VELC Instrument

  • Full form: Visible Emission Line Coronagraph.
  • Function: Observes the Sun’s faint corona by blocking its bright disc.
  • Significance: Uses spectroscopic observations to generate Doppler velocity images.

Coronal Mass Ejections (CMEs)

  • Large eruptions of plasma + magnetic fields from the Sun’s corona.
  • Earth-directed CMEs → Can cause geomagnetic storms and affect satellites, communication, navigation + power grids.

Doppler Effect

  • Blueshift → Source moves towards the observer.
  • Redshift → Source moves away from the observer.
  • Wavelength shifts help estimate plasma velocity along the line of sight.
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