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Aditya-L1 VELC Spots a Flareless Coronal Mass Ejection

15 March 20251 min read
SCIENCE & TECHNOLOGYAditya-L1 VELCSpots a FlarelessCoronal MassEjection15 March 2025safalsetu.com

Why in the news

Indian researchers recorded an eruption from the Sun that occurred without any flare, hinting at other routes for such events.

Key facts

  • Seen by the Indian Institute of Astrophysics through the Visible Emission Line Coronagraph (VELC); date 5 July 2024.
  • VELC watches the corona closer and faster than earlier coronagraphs, tracking CME origins near the solar limb.
  • Results are due in the Astrophysical Journal.

Flare vs CME

FeatureFlareCME
CauseMagnetic reconnectionPlasma eruption of about a trillion kg
OutputElectromagnetic radiationSpeeds up to 3,000 km/s

Significance

  • Helps separate magnetic instabilities behind flares and CMEs; their link is still unclear.
  • CME activity should rise as the Sun nears the Solar Cycle 25 peak.

Exam angle

  • Instrument: VELC; mission: Aditya-L1.

Test yourself

1. Which Aditya-L1 instrument detected the flareless CME on 5 July 2024?

The Visible Emission Line Coronagraph (VELC) observed the event.

2. Solar flares are caused by which process, according to the Aditya-L1 notes?

Flares arise from magnetic reconnection and release electromagnetic radiation.

3. Aditya-L1 is described as India's first mission of which type?

It is India's first dedicated solar research mission.