{
    "id": 11285,
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    "title": "First X-Class Solar Flares of 2013",
    "description": "On May 13, 2013, the sun emitted an X2.8-class flare, peaking at 12:05 p.m. EDT. This is the the strongest X-class flare of 2013 so far, surpassing in strength the X1.7-class flare that occurred 14 hours earlier. It is the 16th X-class flare of the current solar cycle and the third-largest flare of that cycle. The second-strongest was an X5.4 event on March 7, 2012. The strongest was an X6.9 on Aug. 9, 2011.On May 12, 2013, the sun emitted a significant solar flare, peaking at 10 p.m. EDT. This flare is classified as an X1.7, making it the first X-class flare of 2013. The flare was also associated with another solar phenomenon, called a coronal mass ejection (CME) that can send solar material out into space. This CME was not Earth-directed. The May 12 flare was also associated with a coronal mass ejection, another solar phenomenon that can send billions of tons of solar particles into space, which can affect electronic systems in satellites and on the ground. Experimental NASA research models show that the CME left the sun at 745 miles per second and is not Earth-directed, however its flank may pass by the STEREO-B and Spitzer spacecraft, and their mission operators have been notified. If warranted, operators can put spacecraft into safe mode to protect the instruments from solar material. There is some particle radiation associated with this event, which is what can concern operators of interplanetary spacecraft since the particles can trip computer electronics on board. || ",
    "release_date": "2013-05-13T10:30:00-04:00",
    "update_date": "2023-05-03T13:52:10.120221-04:00",
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        "alt_text": "The sun erupted with an X1.7-class solar flare on May 12, 2013.  This is a blend of two images of the flare from NASA's Solar Dynamics Observatory (SDO) — one image shows light in the 171 angstrom wavelength, the other in 131 angstroms.Credit: NASA/SDO/AIA",
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        "alt_text": "On May 12-13 the sun erupted with an X1.7-class and an X2.8-class flare as well as two coronal mass ejections, or CMEs, off the upper left side of the sun.  Solar material also danced and blew off the sun in what's called a prominence eruption, both in that spot and on the lower right side of the sun.  This movie compiles imagery of this activity from NASA's Solar Dynamics Observatory and from the ESA/NASA Solar Heliospheric Observatory.Credit: NASA/SDO/ESA/SOHOMusic: \"Long Range Cruise\" by Lars Leonhard, courtesy of the artist and BineMusic.For complete transcript, click here.",
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    "main_credits": {
        "Visualizations by": [
            {
                "name": "Tom Bridgman",
                "employer": "Global Science and Technology, Inc."
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            "description": "On May 13, 2013, the sun emitted an X2.8-class flare, peaking at 12:05 p.m. EDT. This is the the strongest X-class flare of 2013 so far, surpassing in strength the X1.7-class flare that occurred 14 hours earlier. It is the 16th X-class flare of the current solar cycle and the third-largest flare of that cycle. The second-strongest was an X5.4 event on March 7, 2012. The strongest was an X6.9 on Aug. 9, 2011.<p><p>On May 12, 2013, the sun emitted a significant solar flare, peaking at 10 p.m. EDT. This flare is classified as an X1.7, making it the first X-class flare of 2013. The flare was also associated with another solar phenomenon, called a coronal mass ejection (CME) that can send solar material out into space. This CME was not Earth-directed. <p><p>The May 12 flare was also associated with a coronal mass ejection, another solar phenomenon that can send billions of tons of solar particles into space, which can affect electronic systems in satellites and on the ground. Experimental NASA research models show that the CME left the sun at 745 miles per second and is not Earth-directed, however its flank may pass by the STEREO-B and Spitzer spacecraft, and their mission operators have been notified. If warranted, operators can put spacecraft into safe mode to protect the instruments from solar material. There is some particle radiation associated with this event, which is what can concern operators of interplanetary spacecraft since the particles can trip computer electronics on board.",
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            "description": "On May 12-13 the sun erupted with an X1.7-class and an X2.8-class flare as well as two coronal mass ejections, or CMEs, off the upper left side of the sun.  Solar material also danced and blew off the sun in what's called a prominence eruption, both in that spot and on the lower right side of the sun.  This movie compiles imagery of this activity from NASA's Solar Dynamics Observatory and from the ESA/NASA Solar Heliospheric Observatory.<p>Credit: NASA/SDO/ESA/SOHO<p><p>Music: \"Long Range Cruise\" by<a href=\"http://www.lars-leonhard.de/\"> Lars Leonhard</a>, courtesy of the artist and BineMusic.<p><p><p>For complete transcript, click <a href=\"/vis/a010000/a011200/a011285/May_13_2_X_Flares_HTML_Transcript.html\">here</a>.",
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                        "alt_text": "On May 12-13 the sun erupted with an X1.7-class and an X2.8-class flare as well as two coronal mass ejections, or CMEs, off the upper left side of the sun.  Solar material also danced and blew off the sun in what's called a prominence eruption, both in that spot and on the lower right side of the sun.  This movie compiles imagery of this activity from NASA's Solar Dynamics Observatory and from the ESA/NASA Solar Heliospheric Observatory.Credit: NASA/SDO/ESA/SOHOMusic: \"Long Range Cruise\" by Lars Leonhard, courtesy of the artist and BineMusic.For complete transcript, click here.",
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            "description": "The sun erupted with an X1.7-class solar flare on May 12, 2013.  This is a blend of two images of the flare from NASA's Solar Dynamics Observatory (SDO) — one image shows light in the 171 angstrom wavelength, the other in 131 angstroms.<p><p>Credit: NASA/SDO/AIA",
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        {
            "id": 10959,
            "url": "https://svs.gsfc.nasa.gov/10959/",
            "page_type": "Produced Video",
            "title": "NASA Scientists Answer Top Space Weather Questions",
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            "release_date": "2012-04-24T10:00:00-04:00",
            "update_date": "2023-05-03T13:53:06.910171-04:00",
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                "alt_text": "Part 1For complete transcript, click here.",
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            "page_type": "Produced Video",
            "title": "X-Class: A Guide to Solar Flares",
            "description": "Flares happen when the powerful magnetic fields in and around the sun reconnect. They're usually associated with active regions, often seen as sun spots, where the magnetic fields are strongest. Flares are classified according to their strength. The smallest ones are B-class, followed by C, M and X, the largest. Similar to the Richter scale for earthquakes, each letter represents a ten-fold increase in energy output. So an X is 10 times an M and 100 times a C. Within each letter class, there is a finer scale from 1 to 9. C-class flares are too weak to noticeably affect Earth. M-class flares can cause brief radio blackouts at the poles and minor radiation storms that might endanger astronauts. Although X is the last letter, there are flares more than 10 times the power of an X1, so X-class flares can go higher than 9. The most powerful flare on record was in 2003, during the last solar maximum. It was so powerful that it overloaded the sensors measuring it. They cut-out at X17, and the flare was later estimated to be about X45. A powerful X-class flare like that can create long lasting radiation storms, which can harm satellites and even give airline passengers, flying near the poles, small radiation doses. X flares also have the potential to create global transmission problems and world-wide blackouts. || ",
            "release_date": "2011-08-09T10:00:00-04:00",
            "update_date": "2023-05-03T13:53:41.957045-04:00",
            "main_image": {
                "id": 487409,
                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010100/a010109/Solar_Flares_1280x720_Still_1_print.jpg",
                "filename": "Solar_Flares_1280x720_Still_1_print.jpg",
                "media_type": "Image",
                "alt_text": "Short narrated video about flares, how they are classified, and their effect on Earth.For complete transcript, click here.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        }
    ],
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}