What is the Visible Emission Line Coronagraph (VELC)?

Visible Emission Line Coronagraph is the primary payload of the Aditya-L1 Mission.

What is the Visible Emission Line Coronagraph (VELC)?

About Visible Emission Line Coronagraph (VELC):

  • It is the primary payload of the Aditya-L1 MissionIndia’s first mission to observe the Sun from a vantage point 1.5 million kilometres from the earth.
  • It is an internally occulted solar coronagraph capable of simultaneous imaging, spectroscopy, and spectro-polarimetry close to the solar limb.
  • It is built by the Indian Institute of Astrophysics (IIA) at its CREST (Centre for Research and Education in Science and Technology) campus at Hosakote, Karnataka.
  • The VELC consists of a coronagraph, spectrograph, polarimetry module, and detectors, aside from auxiliary optics.
  • Purpose:
    • It will observe the solar corona, which is the tenuous, outermost layer of the solar atmosphere. 
    • VELC can image the solar corona down to 1.05 times the solar radius, which is the closest any such payload has imaged.
    • It will analyze the coronal temperature, plasma velocity, density, etc.
    • It will also study Coronal Mass Ejections (CMEs) and the solar wind. 

What is a Coronagraph?

  • It is a specialized instrument designed to block out the light of the sun so that researchers can glimpse the burning star’s hot, thin, outermost layer, called the corona
  • The French astronomer Bernard Lyot invented the coronagraph in the 1930s.
  • The sun’s corona is normally visible only during solar eclipses, when the moon’s shadow covers the bright central layers of our parent star and allows its dimmer corona to appear.
  • A coronagraph mimics this natural phenomenon with a circular mask that sits inside a telescope and selectively blocks the bulk of the sun’s light.
  • The specialized coronagraphs act as filters on the central star, allowing the tiny fragments of planetary light to shine through.

Q1: What are Coronal Mass Ejections (CMEs)?

CMEs are large expulsions of plasma and magnetic field from the sun’s atmosphere—the corona, that propagate outward into interplanetary space. During a CME, the sun releases a colossal amount of material, including electrons, protons, and heavier ions, as well as magnetic fields.

News: ‘First significant’ results from payload onboard maiden solar mission Aditya-L1

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