Revealed - Secret behind stealthy solar storms

New Delhi: The sun, which is by far the largest object in the solar system, continuously shoots solar material into space. And the grandest such events as per scientists are massive clouds that erupt from the sun, called coronal mass ejections, or CMEs.

While these solar storms often come first with some kind of warning - the bright flash of a flare, a burst of heat or a flurry of solar energetic particles - another kind of storm has left the scientists baffled for its lack of typical warning signs.

Dubbed 'stealth CMEs', these storms seem to come from nowhere, according to the scientists.

Now, an international team of scientists, led by the Space Sciences Laboratory at University of California, Berkeley, has developed a model that simulates the evolution of these stealthy solar storms.

For this work, the scientists relied upon NASA missions STEREO and SOHO, fine-tuning their model until the simulations matched the space-based observations.

Their work shows how a slow, quiet process can unexpectedly create a twisted mass of magnetic fields on the sun, which then pinches off and speeds out into space - all without any advance warning.

Compared to typical CMEs, which erupt from the sun as fast as 1800 miles per second, stealth CMEs move at a rambling gait - between 250 to 435 miles per second. That’s roughly the speed of the more common solar wind, the constant stream of charged particles that flows from the sun, says a NASA release.

At that speed, stealth CMEs aren’t typically powerful enough to drive major space weather events, but because of their internal magnetic structure they can still cause minor to moderate disturbances to Earth’s magnetic field.

The scientists developed a model of the sun’s magnetic fields, simulating their strength and movement in the sun’s atmosphere, to find out the origins of stealth CMEs.

Central to the model was the sun’s differential rotation, meaning different points on the sun rotate at different speeds. Unlike Earth, which rotates as a solid body, the sun rotates faster at the equator than it does at its poles.

The model showed differential rotation causes the sun’s magnetic fields to stretch and spread at different rates. The scientists demonstrated this constant process generates enough energy to form stealth CMEs over the course of roughly two weeks. The sun’s rotation increasingly stresses magnetic field lines over time, eventually warping them into a strained coil of energy.

When enough tension builds, the coil expands and pinches off into a massive bubble of twisted magnetic fields - and without warning - the stealth CME quietly leaves the sun.

Such computer models can help researchers better understand how the sun affects near-Earth space, and potentially improve our ability to predict space weather, as is done for the nation by the U.S. National Oceanic and Atmospheric Administration.

The study, which is funded in part by NASA, has been published in the Journal of Geophysical Research.

(With ANI inputs)