The Reason the Year 2026 Will Be an Unprecedented Year for India's Solar Observation Mission
For India's first solar observatory, the year 2026 is expected to be like no other.
It's the first time the observatory – that entered into space recently – can observe the Sun when it reaches its maximum activity cycle.
According to scientific data, this occurs approximately every 11 years as the Sun's polarity reverses – a similar Earth scenario could be the planet's poles changing places.
It's a time marked by intense activity. It involves our star transition from calm to stormy and is marked by a huge increase in the number of solar eruptions and coronal mass ejections (CMEs) – massive bubbles of fire that blow out of the Sun's outermost layer.
Made up of ionized particles, a CME can weigh of billions of tons and reach velocities exceeding 2,000 miles per second. It can travel toward various directions, including towards the Earth. At maximum velocity, the journey takes an ejection 15 hours to cover the vast distance Earth-Sun distance.
"During typical or quiet periods, the Sun emits a few solar eruptions a day," explains a leading scientist. "Next year, we expect them to be over ten daily."
Researching CMEs is one of the most important research goals of India's first solar observatory. One, because the ejections provide an opportunity to study the star at the centre of our solar system, and two, because activities occurring on the Sun threaten infrastructure on Earth and in orbit.
Impacts on Earth and Space Infrastructure
CMEs seldom present immediate danger to human life, yet they impact our planet by causing magnetic disturbances affecting the weather in near space, where about 11,000 satellites, including Indian satellites, are stationed.
"The most spectacular manifestations from solar eruptions include northern lights, being direct evidence that charged particles from Sun are travelling to Earth," the scientist explains.
"But they can also cause electronic systems on a satellite fail, disable electrical networks and affect meteorological and telecom spacecraft."
Historical Solar Events
- The most powerful solar storm ever recorded was the 1859 solar superstorm which knocked out communication systems worldwide
- In 1989, sections of Canadian electrical network failed, leaving six million people in darkness for nine hours
- During late 2015, solar activity disrupted air traffic control, causing chaos in Sweden and various European air hubs
- Recently in 2022, a CME caused 38 commercial satellites being lost
If we are able to observe what happens on the Sun's corona and spot a solar storm or a coronal mass ejection in real time, record its temperature at the source and watch its path, it can work as a forewarning to switch off electrical systems and spacecraft redirecting them out of harm's way.
The Mission's Unique Advantage
There are other space observatories watching the Sun, Aditya-L1 holds an edge over others when it comes to watching the corona.
"Aditya-L1's coronagraph has perfect dimensions that lets it nearly mimic the Moon, completely blocking the solar disk and allowing it an uninterrupted view of almost all of the corona around the clock, throughout the year, including during solar events," says the researcher.
In other words, the coronagraph acts like a synthetic eclipse, blocking the Sun's bright surface allowing scientists continuously observe the dim solar atmosphere – something natural eclipses provide only during eclipses.
Additionally, it's unique capable of examining solar events using optical wavelengths, letting it measure a CME's temperature and thermal output – crucial data indicating how strong a CME would be when traveling our direction.
Preparation for Maximum Activity
In preparation for next year's peak solar activity period, researchers worked together to study the data obtained from a major CMEs that Aditya-L1 has recorded until now.
This event began on 13 September 2024 during early hours. The eruption's weight was 270 million tonnes – for comparison that sank Titanic was 1.5 million tonnes.
At origin, the heat was 1.8 million degrees Celsius and the energy content was equivalent to millions of tons of TNT – relative to the atomic bombs on Hiroshima and Nagasaki were 15 kilotons and 21 kilotons each.
Even though these figures make it sound massive, the scientist describes it as a "medium-sized" one.
The asteroid that eliminated the dinosaurs on Earth was 100 million megatons and when solar peak occurs, there may be CMEs carrying power matching greater levels.
"I consider this eruption we evaluated happened during periods was in the normal activity phase. Now this sets the standard for future comparison to evaluate what to expect when the maximum activity cycle occurs," he says.
"The insights from this will assist in work out protective measures to be adopted to protect satellites in orbit. They will also help us gain deeper knowledge of our space environment," he concludes.