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Context: Aditya-L1, has achieved a major scientific breakthrough by capturing the first-ever image of a solar flare ‘kernel’.
Key Highlights of the Observation
- The SUIT payload onboard Aditya-L1 has captured the first-ever image of a solar flare ‘kernel’ in the lower solar atmosphere (photosphere & chromosphere).
- This is the first time such a solar flare has been observed in this wavelength range with such high detail.
Link Between Solar Flare & Energy Deposition
- The observations confirm that the energy released from the flare spreads through different layers of the Sun’s atmosphere.
- A direct correlation was found between localized brightening in the lower atmosphere and the temperature increase in the solar corona (outermost layer of the Sun).
About the SUIT Payload
- SUIT (Solar Ultraviolet Imaging Telescope) is one of the seven scientific payloads onboard Aditya-L1.
- It is designed to observe the Sun’s photosphere and chromosphere in the ultraviolet (UV) wavelength
- Developed by: Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune.
Unique Features of SUIT
- It is the first instrument to observe the Sun in the Near Ultraviolet (NUV) range with such high precision.
- It can capture detailed images of solar eruptions, flares and magnetic field interactions.
- It helps in understanding the connection between the Sun’s lower atmosphere and its outer corona.
Other Scientific Payloads on Aditya-L1
- VELC (Visible Emission Line Coronagraph) – Studies the corona and its dynamics.
- ASPEX (Aditya Solar Wind Particle Experiment) – Analyzes solar wind particles.
- PAPA (Plasma Analyzer Package for Aditya) – Measures charged particles in solar wind.
- SoLEXS (Solar Low Energy X-ray Spectrometer) – Observes X-ray emissions.
- HEL1OS (High Energy L1 Orbiting X-ray Spectrometer) – Studies high-energy solar radiation.
- MAG (Magnetometer) – Measures interplanetary magnetic fields.