Categories: Science & Space

Solar storms and LEO satellites: ISRO monitors decay

Solar storms and LEO satellites: ISRO monitors decay

Solar storms push satellites in Low Earth Orbit toward decay

In the realm of space weather, solar storms are a powerful reminder that the Sun’s activity can directly influence objects far from Earth. When charged particles erupt from the Sun and strike Earth’s upper atmosphere, they heat and expand the outer layer of our planet’s atmosphere. In Low Earth Orbit (LEO), this causes increased atmospheric drag on satellites, effectively pulling them down toward lower altitudes. Recent observations and monitoring confirm that solar storms accelerate the natural decay of satellites already operating in orbit.

What happens to satellites during solar storms

A solar storm injects a surge of energy into Earth’s space environment. The result is a thicker, more dynamic upper atmosphere. For satellites circling roughly 600 to 1,000 kilometers above the planet’s surface, this extra drag can alter their trajectories and shorten mission lifespans. Operators must repeatedly adjust orbits to compensate, and in stronger events some satellites may require reboosts to maintain the desired height. The net effect is a tighter orbital corridor and an uptick in collision avoidance maneuvers as missions navigate the shifting space weather landscape.

Monitoring and management at ISRO

India’s space agency, ISRO, relies on its Master Control Facility (MCF) to closely monitor the health and orbits of operational satellites during periods of elevated solar activity. The MCF serves as a hub for real-time telemetry, orbit determination, and maneuver planning. When solar storms intensify, ground teams analyze orbital data, forecast atmospheric density changes, and determine whether reboosts or trajectory tweaks are necessary to preserve mission objectives.

Active region 4274 and recent sunspot activity

Solar activity is often tracked through sunspots, with groups catalogued by solar observers. A cluster designated Active Region 4274, also referred to as Sunspot Group 6, has drawn attention for its potential to drive geomagnetic disturbances. While not every sunspot leads to a major storm, certain configurations can unleash coronal mass ejections (CMEs) that interact with Earth’s magnetosphere and atmosphere. The presence of notable sunspot regions keeps space weather teams vigilant, even as satellite operators work to minimize disruption to critical services.

Implications for satellite operators and space missions

While a stronger atmosphere drag is a natural consequence of solar activity, it places real constraints on mission planning. Satellite designers and operators now factor space weather into lifetime estimates, collision avoidance budgeting, and end-of-life strategies. For stakeholders relying on Earth observation, communications, or navigation services, the goal is resilient operation through adaptive scheduling, power management, and, when necessary, orbital maintenance maneuvers.

Looking ahead

As solar cycles continue, the role of space weather forecasting becomes increasingly central to satellite operations. Agencies like ISRO, along with international partners, are advancing models that translate solar wind conditions and sunspot activity into actionable orbit guidance. The ongoing collaboration aims to minimize disruption, extend mission lifetimes, and ensure continuity of services that rely on satellites in Low Earth Orbit.