Summary
Scientists found the eruption’s cloud did not expand evenly.
Understanding this helps predict how solar storms may affect satellites and communications.
Aditya‑L1 works together with the United States Space Agency’s Solar Dynamics Observatory and the Indian Institute of Astrophysics.
The Visible Emission Line Coronagraph measured how hot gas moved toward and away from Earth.
A new three‑dimensional model showed the eruption’s shape was tilted and grew unevenly.
These findings improve forecasts of space weather that can affect satellites.
Scientists found the eruption’s cloud did not expand evenly.
Understanding this helps predict how solar storms may affect satellites and communications.
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