default | grid-3 | grid-2

Post per Page

60,000-mile-tall 'plasma waterfall' seen showering the sun with impossibly fast fire

A massive wall of falling plasma, known as a polar crown prominence, was recently captured in a stunningly-detailed new photo of the sun.

An astrophotographer has snapped a stunning shot of an enormous wall of plasma falling down toward the solar surface at impossibly fast speeds after being spat out near the sun's south pole. 

Eduardo Schaberger Poupeau, who is based near Rafaela in Argentina, captured the striking image(opens in new tab) on March 9 using specialized camera equipment. The plasma wall "rose some 100,000 km [kilometers, or 62,000 miles] above the solar surface," Poupeau told For context, that is as tall as around eight Earths stacked on top of one another. "On my computer screen, it looked like hundreds of threads of plasma were dripping down a wall," Poupeau added.

The dazzling phenomenon is known as a polar crown prominence (PCP), according to PCPs are similar to normal solar prominences, which are loops of plasma, or ionized gas, that are ejected from the solar surface by magnetic fields. However, PCPs occur near the sun's magnetic poles at latitudes between 60 and 70 degrees North and South, which often causes them to collapse back towards the sun because the magnetic fields near the poles are much stronger, according to NASA. This collapse back to the sun has earned them the nickname "plasma waterfalls."

The plasma within PCPs is not actually in freefall because it is still contained within the magnetic field that initially spat them out. However, the plasma travels downwards at speeds of up to 22,370 mph (36,000 km/h), which is much faster than the magnetic fields should allow based on experts' calculations, according to NASA. Researchers are still trying to figure out how this is possible.

An image of the sun captured March 10 by NASA's Solar Dynamics Observatory. The "plasma waterfall" is circled in the image. (Image credit: NASA/SDO)

A study published in 2021 in the journal Frontiers in Physics(opens in new tab) revealed that PCPs undergo two phases during their eruptions: A slow phase, where plasma slowly shoots upward, and a fast phase, where plasma accelerates towards its altitude peak. It is possible that this may affect how the plasma falls back to the surface, but more research is needed to tell for sure.

Sped-up video footage of a PCP rising and falling above the sun on Nov. 30 2006. (Image credit: NASA)

Solar physicists often study solar prominences because they can be accompanied by coronal mass ejections, or massive magnetized plasma plumes that can fully break away from the sun and slam into Earth. But PCPs are also of interest to nuclear physicists because the sun's magnetic field seems to be particularly adept at containing the plasma loops in the polar regions, which could provide insights that help researchers improve experimental nuclear fusion reactors. 

PCP's are very common and could happen almost every day, although images of the phenomenon like the one Poupeau captured are rare, according to NASA. However, like many other plasma-related solar phenomena, PCPs could become even more frequent and intense as the sun ramps up to a peak in its 11-year solar cycle known as the solar maximum. 

On Feb. 2, a massive solar prominence, just below the latitude needed to be deemed a PCP, broke off from the sun and became trapped in an enormous and fast-moving polar vortex(opens in new tab) around the sun's north pole for about 8 hours. On Sept. 5, 2022, an enormous, undulating stream of plasma shot across the solar surface like a snake(opens in new tab), and on Sept. 24, 2022, a colossal 1-million-mile long plume of plasma(opens in new tab) erupted from the sun's surface after another prominence snapped in half.

Originally published on

No comments

Error Page Image

Error Page Image

Oooops.... Could not find it!!!

The page you were looking for, could not be found. You may have typed the address incorrectly or you may have used an outdated link.

Go to Homepage