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    "title": "Scientists Uncover Origins of Dynamic Jets on Sun's Surface",
    "description": "At any given moment, as many as 10 million wild jets of solar material burst from the sun’s surface. They erupt as fast as 60 miles per second, and can reach lengths of 6,000 miles before collapsing. These are spicules, and despite their grass-like abundance, scientists didn’t understand how they form. Now, for the first time, a computer simulation — so detailed it took a full year to run — shows how spicules form, helping scientists understand how spicules can break free of the sun’s surface and surge upward so quickly. This work relied upon high-cadence observations from NASA’s Interface Region Imaging Spectrograph, or IRIS, and the Swedish 1-meter Solar Telescope in La Palma. Together, the spacecraft and telescope peer into the lower layers of the sun’s atmosphere, known as the interface region, where spicules form. The results of this NASA-funded study were published in Science on June 22, 2017 — a special time of the year for the IRIS mission, which celebrates its fourth anniversary in space on June 26.Research: On the generation of solar spicules and Alfvénic waves.Journal: Science, June 22, 2017.Link to paper: http://science.sciencemag.org/content/356/6344/1269.full || ",
    "release_date": "2017-06-22T14:00:00-04:00",
    "update_date": "2023-05-03T13:47:35.273480-04:00",
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        "Scientific consulting by": [
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                "name": "Juan Martínez-Sykora",
                "employer": "Lockheed Martin/BAER Institute"
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                "name": "Bart De Pontieu",
                "employer": "Lockheed Martin Solar and Astrophysics Lab"
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            "description": "At any given moment, as many as 10 million wild jets of solar material burst from the sun’s surface. They erupt as fast as 60 miles per second, and can reach lengths of 6,000 miles before collapsing. These are spicules, and despite their grass-like abundance, scientists didn’t understand how they form. Now, for the first time, a computer simulation — so detailed it took a full year to run — shows how spicules form, helping scientists understand how spicules can break free of the sun’s surface and surge upward so quickly. <p>\rThis work relied upon high-cadence observations from NASA’s Interface Region Imaging Spectrograph, or IRIS, and the Swedish 1-meter Solar Telescope in La Palma. Together, the spacecraft and telescope peer into the lower layers of the sun’s atmosphere, known as the interface region, where spicules form. The results of this NASA-funded study were published in Science on June 22, 2017 — a special time of the year for the IRIS mission, which celebrates its fourth anniversary in space on June 26.<p>Research: On the generation of solar spicules and Alfvénic waves.<br>Journal: Science, June 22, 2017.<br>Link to paper: <a href=\"http://science.sciencemag.org/content/356/6344/1269.full\">http://science.sciencemag.org/content/356/6344/1269.full</a>",
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            "description": "See [https://www.nasa.gov/feature/goddard/2017/scientists-uncover-origins-of-the-sun-s-swirling-spicules](https://www.nasa.gov/feature/goddard/2017/scientists-uncover-origins-of-the-sun-s-swirling-spicules)",
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                "alt_text": "A coronal mass ejection burst off the side of the sun on May 9, 2014. The giant sheet of solar material erupting was the first CME seen by NASA's Interface Region Imaging Spectrograph, or IRIS. The field of view seen here is about five Earth's wide and about seven and a half Earth's tall.Watch this video on the NASAexplorer YouTube channel.For complete transcript, click here.",
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            "title": "Solar Close-ups with Hinode's Solar Optical Telescope",
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