ADITYA-L1: UNVEILING THE MECHANICS OF SOLAR SUPER-STORMS

India’s Aditya-L1, in collaboration with six U.S. satellites (including NASA’s Parker and Wind), has decoded the unusual behavior of the May 2024 Solar Storm (Gannon’s Storm).
The Phenomenon: The mission observed a rare event where two Coronal Mass Ejections (CMEs) collided, triggering a process known as Magnetic Reconnection.

Magnetic Reconnection: Typically, CMEs carry twisted “magnetic ropes.” During this event, two CMEs collided, compressing the magnetic field lines until they snapped and rejoined.
Scale of Event: The reconnection region was approximately 1.3 million km wide (nearly 100 times the size of Earth).
Impact: This process caused a sudden reversal of magnetic fields, significantly intensifying the storm’s impact on Earth’s magnetic shield.
Significance: This is the first recorded instance of such a massive magnetic breakup and rejoining observed inside a CME.

Objective: To study the Sun’s outermost layers: the Photosphere, Chromosphere, and Corona.
Placement: Positioned in a Halo Orbit around the Lagrange Point 1 (L1), approx. 1.5 million km from Earth.
Strategic Advantage: The L1 point allows for a continuous, uninterrupted view of the Sun without any occultation or eclipse.
Payloads: It carries seven payloads to observe the Sun across various wavelengths (Visible, UV, X-ray) and measure particle flux/magnetic fields in situ.

Parker Solar Probe (NASA): Closest mission to the Sun; studies the outer corona and solar wind.
Solar Orbiter (ESA/NASA): Focuses on the Sun’s poles and the 11-year solar cycle.
SOHO (NASA/ESA): Provides real-time data on space weather.
ASO-S / Kuafu-1 (China): Studies solar flares and magnetic fields to understand Earth’s environmental impact.