Indian astronomers decode how solar storms 'cool down' on their way to Earth
IIA scientists have traced how giant solar eruptions evolve thermally across the Sun-Earth journey — insight that sharpens space-weather forecasting for the satellites, GPS, aviation and power grids these storms can disrupt.
What happened
- Astrophysicists at the Indian Institute of Astrophysics (IIA), Bengaluru — an autonomous institute under the Department of Science and Technology — uncovered how Interplanetary Coronal Mass Ejections (ICMEs) evolve thermally as they travel from the Sun to the Earth.
- ICMEs are massive blasts of magnetised plasma from the Sun's outer atmosphere; when directed at Earth, they can trigger geomagnetic storms.
- Such storms can disrupt satellite operations, GPS and radio communications, aviation routes and power grids — and produce auroras.
- Solar activity follows an ~11-year cycle; the peak of the current Cycle 25 was in 2025, increasing ICME frequency.
- Analysing three decades of solar-storm data, the team found patterns in ICMEs' thermal signatures that can improve forecasting of their geo-effectiveness and space-weather preparedness.
For Prelims
- CME / ICME: A Coronal Mass Ejection is a large expulsion of magnetised plasma from the Sun's corona; in interplanetary space it is an ICME. Earth-directed ICMEs drive geomagnetic storms.
- Space weather: Sun-driven conditions (solar flares, CMEs, solar wind) that affect satellites, GPS, HF radio, aviation (polar routes) and power grids — a growing strategic concern.
- Solar cycle: The Sun's activity waxes and wanes over an ~11-year cycle; Solar Cycle 25 peaked around 2025, raising flare/CME frequency.
- Aditya-L1: India's first solar mission (at the Sun-Earth L1 Lagrange point) studies the corona, solar wind and space weather — complementing such research.
- IIA & DST: The Indian Institute of Astrophysics (Bengaluru) is an autonomous body under the Department of Science and Technology; it operates observatories (e.g. Kodaikanal, Hanle).
- Geomagnetic storm impacts: Can cause satellite drag/anomalies, GPS errors, radio blackouts, grid-current surges (transformer damage) — hence forecasting matters.
- Don't confuse: A solar flare (electromagnetic burst) is distinct from a CME (plasma ejection); not every CME is Earth-directed, and the ICME's thermal/magnetic state determines its 'geo-effectiveness'.
For UPSC: IIA scientists mapped how ICME solar storms evolve thermally Sun-to-Earth, improving space-weather forecasting for satellites, GPS, aviation and grids. Anchor CMEs/ICMEs and geomagnetic storms, space weather and its infrastructure impacts, the ~11-year solar cycle (Cycle 25 peak 2025), Aditya-L1, and IIA/DST.
What it is NOT: A solar flare (an electromagnetic burst) is distinct from a CME (a plasma ejection); only Earth-directed ICMEs cause geomagnetic storms, and their 'geo-effectiveness' depends on their thermal and magnetic state — not all CMEs are hazardous to Earth.
For Mains
Syllabus: GS3.13 · GS1.12 · Linkage L2
Anchor
Space science with real-world stakes — forecasting solar storms to protect critical space and ground infrastructure.
Substantiation (data)
IIA (DST) study on ICME thermal evolution Sun-to-Earth using three decades of data; relevance to satellites, GPS, aviation and grids; Solar Cycle 25 peak 2025.
Exemplification
Cite ICME forecasting, Aditya-L1 and IIA observatories as India's space-weather research and preparedness capability.
Problematisation
Predicting geo-effectiveness is hard; growing satellite/grid dependence raises vulnerability; forecasting lead-time and modelling remain challenges.
Way-forward
Strengthen space-weather monitoring (Aditya-L1/ground networks), improve forecasting models, and harden satellites and grids against storms.
Position
Government/science stance: indigenous astrophysics research builds India's space-weather forecasting and resilience of critical infrastructure.
Deploys into: Space science & space weather (CME/ICME/Aditya-L1) · resilience of satellites/GPS/grids · solar cycle & geomagnetic storms · indigenous research (IIA/DST) (GS3.13 space & S&T, GS1.12 geophysical phenomena).
Ministry of Science & Technology · 2026-06-30 · PRID 2279357 · PIB source ↗