Mixer Waves of the Solar Wind: How the Corona Heats Up express

Original: "Free Energy Sources of Ion-scale Waves Observed by Parker Solar Probe"
arXiv:2512.11182 · 2025-12-12 · CC BY 4.0 · 1 min
The Parker probe caught two types of spiral waves that, like mixers, redistribute heat in the solar wind and explain the corona's anomalous heating.

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The solar wind isn't a calm stream but a bubbling soup of charged particles. Diving close to the Sun, the Parker probe picked up two types of stirring waves. Left-handed ones, like a whisk in a chef's hand, whip up the material when the temperature differs along and across the flow. They rage nearly a third of the time near the star, boosting the share of the fastest particles — much like a mixer pushing foam to the surface.

Right-handed waves

emerge less often and weaker near the Sun, but intensify farther out, driven by streams of hot protons (hydrogen nuclei) — like tiny steam bubbles rising in soup.

Fine analysis of light (spectroscopy) and machine learning captured the moment when thermal jets give birth to right-handed waves. Paradoxically, it's this invisible ripple, not grand eruptions, that heats the giant corona — its temperature is hundreds of times that of the solar surface. The rhythm of these waves determines space weather near Earth.

The solar wind carries away about the mass of Mount Everest every minute.

Scientists
Ludwig BoltzmannEnrico FermiCecilia Payne-GaposchkinJoseph von FraunhoferFred Lawrence WhippleGalileo Galilei
Concepts
plasma wave solar wind waves alfven wave marine heatwave ionosphere parker solar probe ionized gas radio source microwave photon plasma lhaaso particle shower direct waves radiosonde pulsar companion microwave signal Southern Oscillation index Solar wind standing wave pulsar phenomena