Why 2026 Is Set to Be an Unprecedented Year for India's Solar Observation Mission

Solar activity visualization
A coronal mass ejection is much bigger than our planet

For Aditya-L1, 2026 is expected to be like no other.

This marks the initial occasion the observatory – that entered in orbit recently – can watch our star when it reaches the peak of its solar cycle.

As per research, it comes approximately once every 11 years as the Sun's polarity reverses – a similar Earth scenario would be the planet's poles changing places.

This period of great turbulence. It sees our star transition from calm to stormy and features a significant rise in the frequency of solar eruptions and coronal mass ejections (CMEs) – enormous clouds of plasma that erupt from the solar corona.

Composed of charged particles, a CME can weigh up to a trillion kilograms and reach a speed exceeding 2,000 miles per second. It can travel toward various directions, including towards the Earth. At maximum velocity, the journey takes an ejection about half a day to cover the vast distance Earth-Sun distance.

"In the normal or quiet periods, the Sun launches two to three CMEs a day," says a leading scientist. "In 2026, it's anticipated them to be over ten daily."

Researching CMEs is one of the most important scientific objectives for the Indian first solar observatory. Firstly, because the ejections provide an opportunity to learn about the star at the centre of our solar system, and two, because activities occurring on the Sun endanger infrastructure on our planet and in space.

Aurora display
The aurora borealis illuminated the night sky over the US last autumn

Effects on Our Planet and Space Infrastructure

Coronal mass ejections rarely pose immediate danger to people, yet they impact life on Earth by causing magnetic disturbances that impact conditions in Earth's vicinity, where about thousands of spacecraft, comprising Indian satellites, are stationed.

"The most spectacular displays of a CME are auroras, being a clear example that solar particles from Sun journey toward our planet," the expert clarifies.

"However, they may make all the electronics aboard spacecraft fail, disable electrical networks and affect meteorological and telecom spacecraft."

Past Solar Incidents

  • The strongest solar event ever recorded occurred during the Carrington Event that disabled telegraph lines across the globe
  • In 1989, sections of Quebec's power grid failed, leaving six million people in darkness for hours
  • In November 2015, solar activity disturbed flight operations, leading to disruption in Sweden and various European air hubs
  • In February 2022, an ejection had led to dozens of spacecraft failing

If we are able to see events in the solar atmosphere and spot solar activity or solar eruption as it happens, measure its heat at the source and track its path, this serves as a forewarning to switch off power grids and spacecraft and move them to safety.

Solar corona during eclipse
The Sun's corona can be seen when the Moon blocks the Sun from Earth

Aditya-L1's Unique Advantage

There are other solar missions watching the Sun, Aditya-L1 has an advantage over others regarding studying the solar atmosphere.

"The instrument is the exact size that lets it effectively simulate lunar coverage, completely blocking the solar disk and allowing it continuous observation of almost all solar atmosphere 24 hours a day, throughout the year, including during eclipses and occultations," says the researcher.

Essentially, the coronagraph acts like a synthetic eclipse, blocking the solar glare allowing researchers continuously observe the dim solar atmosphere – a feat the real Moon does only during eclipses.

Moreover, it's unique that can study eruptions using optical wavelengths, letting it determine eruption heat and heat energy – key clues that show how strong a CME would be if it headed toward Earth.

Preparation for Maximum Activity

In preparation for next year's peak solar activity period, scientists collaborated to study the data obtained from a major solar eruption that Aditya-L1 has observed recently.

It originated on 13 September 2024 during early hours. The eruption's weight totaled billions of tons – for comparison that struck the ship was 1.5 million tonnes.

At origin, the heat was 1.8 million degrees Celsius with energy equivalent comparable to 2.2 million megatons of TNT – relative to the atomic bombs used in Japan were 15 kilotons in scale respectively.

Although these figures seem massive, the scientist classifies it as a "medium-sized" one.

The asteroid which wiped out prehistoric life on Earth carried enormous energy and when solar peak occurs, we could see CMEs carrying power matching greater levels.

"I consider the CME we analyzed to have occurred during periods was in the normal activity phase. Now this sets the standard that we'll be using to evaluate what is in store during solar maximum occurs," he says.

"The learnings gained will help us work out the countermeasures to implement safeguarding spacecraft in near space. Additionally, they'll aid us gain a better understanding of near-Earth space," he concludes.

Alyssa Smith
Alyssa Smith

A seasoned business strategist with over 15 years of experience in digital transformation and corporate innovation.