Waves Spinning in Opposite Directions Found Inside a Solar Eruption express

Original: "Evidence of energy conversion in weakly collisional plasma during an interplanetary coronal mass ejection"
arXiv:2601.12476 · 2026-01-18 · CC BY 4.0 · 1 min
In a clump of solar gas, particles rotate left and right at the same time.

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The Sun constantly emits a stream of charged particles, mostly hydrogen — the solar wind. Sometimes the Sun ejects dense blobs of magnetized gas, inside which calm usually reigns. But in 2000, scientists noticed two regions inside one such cloud where the gas was churning. Using rainbow splitting of light (a method that breaks down glow into colors), they found that waves simultaneously exist there, making particles swirl left and right.

It was previously thought that such different rotations couldn’t coexist in a magnetic cloud.

It’s like a ballroom where some couples waltz clockwise and others counterclockwise, yet they never collide. This dual motion helps transfer energy and heat the cosmos. When electrons gain more heat, the right-handed vortices strengthen, and the magnetic field sways in sync with density — like a well-coordinated step. The system moves toward equilibrium, ramping up disorder.

Surprisingly, similar paired vortices are sometimes seen in terrestrial hurricanes, where adjacent spiral arms can spin in opposite directions — nature loves recycling winning designs.

Whistlers — those very 'right-handed' waves — on Earth sound like mysterious whistles on a radio after a thunderstorm, sliding along magnetic field lines.

Scientists
Albert EinsteinBarry BarishKip ThorneRichard FeynmanRussell HulseShuji Nakamura
Concepts
coronal mass ejection solar eruption plasma wave solar magnetic phenomena magnetic fluctuation confinement alfven wave intracluster medium intermittency plasma helicity ionized gas pulsar wind radio pulse international space station molecular vibration ion channel noise acoustic oscillations plasma heating interstellar medium