5 min read NASA, ESA Missions Help Scientists Uncover How Solar Wind Gets Energy Since the 1960s, astronomers have wondered how the Sun’s supersonic “solar wind,” a stream of energetic particles that flows out into the solar system, continues to receive energy once it leaves the Sun. Now, thanks to a lucky lineup of a NASA and an ESA (European Space Agency)/NASA spacecraft both currently studying the Sun, they may have discovered the answer — knowledge that is a crucial piece of the puzzle to help scientists better forecast solar…
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The sun might’ve just had a record-breaking number of visible sunspots
On Aug. 8, scientists may have caught hundreds of individual sunspots on images produced by NASA’s Solar Dynamics Observatory (SDO). To us, sunspots might seem really tiny — but don’t be fooled. They are actually dark areas typically the size of the entire Earth on the sun’s surface. Plus, they exhibit strong magnetic fields that can fire off solar flares, which spew pulses of electromagnetic radiation into space. These are the explosions that lead to coronal mass ejections (CMEs) that can create solar storms on Earth. “The process of the…
Read MoreThe sun fires off 2 powerful X flares in less than 2 hours (video, photo)
The sun showcased its immense power yet again this morning (August 5), firing off not one but two X-class flares. X flares are the strongest solar flare class. Today’s first X blast, which launched from a sunspot called AR3767, reached its peak around 9:40 a.m. EDT (1340 GMT), clocking in at X1.7 on solar scientists’ flare scale. Then, less than two hours later, the sunspot AR3780 fired off an X1.1 class solar flare, which peaked at 11:27 a.m. EDT (1527 GMT). Solar flares are often accompanied by huge eruptions of solar…
Read MoreMagnetic fields on the sun could solve longstanding solar heating mystery
Scientists have long wondered why the hot soup of charged particles in our sun’s atmosphere gets hotter moving away from the surface of the sun. New research may have the answer, finding the super-hot nature of the sun’s outer atmosphere or “corona” could be due to the intriguing behavior of small-scale waves in this nebulous plasma. These waves, known to scientists as “kinetic Alfvén waves” or “KAWs,” are wave-like vibrations of magnetic fields manifested by motions in the sun’s photosphere. The findings could provide an important clue to decoding the…
Read MoreSun blasts out most powerful flare of current solar cycle, sends massive coronal mass ejection into space (video)
On Tuesday (July 23), Europe’s Solar Orbiter (SolO) spacecraft witnessed an extremely powerful X14 class solar flare erupt from the far side of the sun. Although it was not the most powerful flare ever recorded, which was estimated at roughly a X45 back in 2003, solar flares of this magnitude can result in longer-lived radiation storms and even world-wide blackouts if they are directed at Earth. The X-class are the leaders on the classification scale, and blast out energy 10 times more powerful than M class flares, which is second…
Read MoreSun blasts out 2nd X-class flare this week, triggers more radio blackouts (video)
The sun continues firing off solar flares during what has been a period of intense activity. Sunspot AR3738 might be making its exit as it rotates out of our view on the sun’s western limb, but not before firing off a powerful X-class solar flare, the strongest of its kind. The solar flare from sunspot AR3738 occurred Tuesday morning (July 16) at 9:26 a.m. EDT (1326 GMT). A shortwave radio blackout in conjunction with the latest event was reported over mostly the Atlantic Ocean and also noted across much of Africa, Europe, and…
Read MoreScientists call the region of space influenced by the sun the heliosphere – but without an interstellar probe, they don’t know much about its shape
This article was originally published at The Conversation. The publication contributed the article to Space.com’s Expert Voices: Op-Ed & Insights. Sarah Spitzer is a research fellow in Climate and Space Sciences and Engineering at the University of Michigan. The sun warms the Earth, making it habitable for people and animals. But that’s not all it does, and it affects a much larger area of space. The heliosphere, the area of space influenced by the sun, is over a hundred times larger than the distance from the sun to the Earth. The sun is a…
Read MoreSolar maximum is in sight but when will it arrive (and when will we know)?
May and June 2024 saw the highest sunspot numbers on the sun since 2002, but is the peak of the solar cycle here yet? The sun follows an 11-year solar cycle of increasing and decreasing activity. Although not the first astronomer to discover the solar cycle, the solar cycle numbering and naming convention was first introduced in 1852 by Swiss astronomer Johann Rudolf Wolf. Within his new solar cycle numbering system, he set the historic 1755-1766 solar cycle ‘Solar Cycle 1’. By the time of his work, the sun was…
Read MoreCelebrate the Heliophysics Big Year with Free Heliophysics and Math Webinars from NASA HEAT
2 min read Celebrate the Heliophysics Big Year with Free Heliophysics and Math Webinars from NASA HEAT The Heliophysics Big Year (HBY) is a global celebration of the Sun’s influence on Earth and the entire solar system. It began with the Annular Solar Eclipse on Oct. 14, 2023, continued through the Total Solar Eclipse on Apr. 8, 2024, and will conclude with Parker Solar Probe’s closest approach to the Sun in December 2024. Challenged by the NASA Heliophysics Division to participate in as many Sun-related activities as possible, the NASA…
Read MoreSee the sun rage behind the ISS in epic time-lapse photo
Miguel Claro is a professional photographer, author and science communicator based in Lisbon, Portugal, who creates spectacular images of the night sky. As a European Southern Observatory Photo Ambassador and member of The World At Night and the official astrophotographer of the Dark Sky Alqueva Reserve, he specializes in astronomical “Skyscapes” that connect both Earth and the night sky. This image shows the silhouette of the International Space Station (ISS) as it crosses in front of the sun’s disk at a distance of 274 miles (441.5 km) from us and at a speed of about 4.5 miles…
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