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Aditya-L1 Records Coronal Mass Ejection, Reveals New Details on Solar Plasma Movement and Magnetic Activity

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Indian researchers have analysed a big photo voltaic occasion utilizing information from the Visible Emission Line Coronagraph (VELC) onboard the Aditya-L1 mission, as per experiences. As India’s first photo voltaic statement mission, Aditya-L1 noticed a Coronal Mass Ejection (CME) on July 16, 2024, offering invaluable insights into the Sun’s dynamic outer ambiance. This occasion, characterised by a large ejection of photo voltaic plasma and magnetic fields, was studied intimately utilizing emission at a particular wavelength of 5303 Å, recognized for its inexperienced hue brought on by superheated iron atoms.

Launched on September 2, 2023 and efficiently positioned in a halo orbit across the Sun-Earth Lagrange Point L1 in January 2024, Aditya-L1 is positioned 1.5 million kilometres from Earth. According to experiences, the mission goals to watch photo voltaic exercise and its impression on area climate. The findings associated to the CME have been printed in The Astrophysical Journal Letter by researchers from the Indian Institute of Astrophysics.

Observations of Coronal Mass Ejection

Reportedly, the researchers recognized a phenomenon often called coronal dimming, the place the brightness of the Sun’s corona decreased by almost 50 % within the affected area because of the ejection of photo voltaic materials. This dimming persevered for roughly six hours. The examine additionally recorded a 30% enhance in temperature and heightened turbulence within the area, marked by non-thermal plasma movement at a velocity of 24.87 km/s.

Plasma Movement and Magnetic Influence

Doppler velocity measurements indicated that the plasma was redshifted, transferring away from the observer at a velocity of about 10 km/s, as per sources. The CME’s trajectory was influenced by the Sun’s magnetic subject, which prompted a deflection within the motion of the ejected materials. This discovery underscores the significance of understanding magnetic forces in predicting the conduct of CMEs as they traverse interplanetary area.

These findings spotlight the important function of Aditya-L1 in unraveling the complexities of photo voltaic phenomena, paving the way in which for improved area climate predictions and advancing photo voltaic science.

 



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