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Aditya-L1: research into solar eruptions

This dossier follows scientific results from India’s Aditya-L1 solar observatory, methods and limitations.

Last updated : 1 key moments

Where things stand

On 3 November 2026, Indian science authorities present a study reconstructing the asymmetric expansion of a coronal ejection observed in 2024. Generalisation requires further testing.

Aditya-L1 sheds light on asymmetric solar-eruption expansion

India’s science ministry and ISRO presented a study on 3 November 2026 using Aditya-L1 to reconstruct the asymmetric expansion of a coronal mass ejection. The announcement concerns analysis of observations from 5 August 2024, rather than a new eruption.

2012 archive solar image, NASA/SDO, public domain; does not depict the 2024 ejection studied.
2012 archive solar image, NASA/SDO, public domain; does not depict the 2024 ejection studied. — NASA/SDO — domaine public — image solaire d’archives de 2012, sans modification.

The Indian Institute of Astrophysics team combined VELC spectroscopy, images from NASA’s SDO observatory and a three-dimensional model. Uniform expansion did not reproduce the measured signatures, whereas uneven lateral expansion with a tilted axis did.

The study appears in The Astrophysical Journal Letters. Researchers intend to apply the method to other ejections. It could assist space-weather research, but an operational forecasting improvement has not been established.

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