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Space photo of the week: Pink 'raindrops' on the sun captured in greatest detail ever
Space photo of the week: Pink 'raindrops' on the sun captured in greatest detail ever

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time2 days ago

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Space photo of the week: Pink 'raindrops' on the sun captured in greatest detail ever

When you buy through links on our articles, Future and its syndication partners may earn a commission. Quick facts What it is: The sun's corona Where it is: The outermost layer of the sun's atmosphere. When it was shared: May 27, 2025 Solar "raindrops" — plasma streams and vast arches extending outward from the sun's surface and into the corona, the outermost part of the solar atmosphere — have been captured in spectacular new detail by a ground-based telescope in California. Among the images taken from time-lapse movies, which utilize new technology to eliminate blurring caused by Earth's atmosphere, is coronal rain, a phenomenon that occurs when cooling plasma condenses and falls back toward the sun's surface along magnetic field lines. Other features imaged include prominences — the term solar physicists use to describe the arches and loops — and finely structured plasma streams. The images are artificially colorized from the hydrogen-alpha light captured by the telescope, making them appear pink. The remarkable images, taken by researchers from the U.S. National Science Foundation's National Solar Observatory and New Jersey Institute of Technology, were published this week in a paper in the journal Nature. "These are by far the most detailed observations of this kind, showing features not previously observed, and it's not quite clear what they are," Vasyl Yurchyshyn, co-author of the study and a research professor at the New Jersey Institute of Technology, said in a statement. The researchers captured the new images using the 1.6-meter Goode Solar Telescope at the Big Bear Solar Observatory (BBSO) in California, equipped with a new technology called Cona, which employs a laser to correct for turbulence in Earth's upper atmosphere. Related: NASA spacecraft snaps eerie image of eclipsed sun with an extra moon overhead. What's going on? Cona is "like a pumped-up autofocus" for the sky, Nicolas Gorceix, chief observer at BBSO, said in the statement. It's a form of adaptive optics that works by measuring, and then adapting in real-time to, atmospheric distortions, reshaping a special mirror 2,200 times per second. Turbulence in Earth's upper atmosphere has always been a limiting factor when studying the sun, but Cona increases the resolution of what can be observed, from features over 620 miles (1,000 kilometers) wide to just 63 km (39 miles). SEE MORE SPACE PHOTOS —Violent galaxies seen 'jousting' near the dawn of time —Cotton candy clouds shine in one of Hubble's most beautiful images ever —Bizarre 1-armed spiral galaxy stuns Hubble scientists The sun's corona, which means crown, is one of the most mysterious places in the solar system. This outer layer of the sun's atmosphere is blocked from view by the brighter photosphere — the sun's surface — and is only visible briefly to the naked eye during a total solar eclipse. That also applies to prominences, which can be seen during totality as reddish-pink arches and loops. Despite its tenuous nature, the corona is millions of degrees hotter than the photosphere. It's of critical interest to solar scientists because it's in the corona that the solar wind originates. This constant stream of charged particles then radiates throughout the solar system, interacting with planetary atmospheres (including Earth's) to cause geomagnetic storms and auroras. Following the successful test of Cona, plans are underway to install it on the 4-meter Daniel K. Inouye Solar Telescope in Maui, Hawaii, the world's largest solar telescope.

New Imaging Technique Makes the Sun Look Like a Swirling Pink Liquid
New Imaging Technique Makes the Sun Look Like a Swirling Pink Liquid

Yahoo

time3 days ago

  • General
  • Yahoo

New Imaging Technique Makes the Sun Look Like a Swirling Pink Liquid

A swirling sea of pink, where fluffy tufts float majestically upward, while elsewhere violet plumes rain down from above. This is the Sun as seen in groundbreaking new images — and they're unlike anything you've ever laid eyes on. As detailed in a new study published in the journal Nature Astronomy, scientists have leveraged new coronal adaptive optics tech to bypass the blurriness caused by the turbulence of the Earth's atmosphere, a time-old obstacle that's frustrated astronomers' attempts to see features on our home star at a resolution better than 620 miles. Now, they've gotten it down to just under 40 miles — a light year sized leap. The result is some of the clearest images to date of the fine structures that make up the Sun's formidable corona, the outermost layer of its atmosphere known for its unbelievable temperatures and violent, unpredictable outbursts. The authors are optimistic that their blur-bypassing techniques will be a game-changer. "These are by far the most detailed observations of this kind, showing features not previously observed, and it's not quite clear what they are," coauthor Vasyl Yurchyshyn, a research professor at the New Jersey Institute of Technology's Center for Terrestrial Research (CSTR), said in a statement about the work. "It is super exciting to build an instrument that shows us the Sun like never before," echoed lead author Dirk Schmidt, an adaptive optics scientist at the US National Solar Observatory. Stretching for millions of miles into space, the corona is the staging ground for the Sun's violent outbursts, which range from solar storms, to solar flares, to coronal mass ejections. One reason scientists are interested in these phenomena is because they continue to batter our own planet's atmosphere, playing a significant role in the Earth's climate and wreaking havoc on our electronics. Then, at a reach totally beyond our very limited human purview, is the corona's mighty solar wind, which sweeps across the entire solar system, shielding it from cosmic rays. But astronomers are still trying to understand how these solar phenomena occur. One abiding mystery is why the corona can reach temperatures in the millions of degrees Fahrenheit, when the Sun's surface it sits thousands of miles above is no more than a relatively cool 10,000 degrees. The conundrum even has a name: the coronal heating problem. The level of detailed captured in the latest images, taken with an adaptive optics system installed on the Goode Solar Telescope at the CSTR, could be transformative in probing these mysteries. One type of feature the unprecedented resolution revealed were solar prominences, which are large, flashy structures that protrude from the sun's surface, found in twisty shapes like arches or loops. A spectacular video shows a solar prominence swirling like a tortured water spout as it's whipped around by the sun's magnetic field. Most awe-inspiring of all are the examples of what's known as coronal rain. Appearing like waterfalls suspended in midair, the phenomenon is caused as plasma cools and condenses into huge globs before crashing down to the sun's surface. These were imaged at a scale smaller than 100 kilometers, or about 62 miles. In solar terms, that's pinpoint accuracy. "With coronal adaptive optics now in operation, this marks the beginning of a new era in solar physics, promising many more discoveries in the years and decades to come," said coauthor Philip R. Goode at the CSTR in a statement. More on our solar system: Scientists Detect Mysterious Object in Deep Solar System

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