This flare is classified as an M5.7-class flare. M-class flares are the weakest flares that can still cause some space weather effects near Earth. Increased numbers of flares are quite common at the moment, as the sun's normal 11-year activity cycle is ramping up toward solar maximum, which is expected in late 2013.", "items": [], "extra_data": {} }, { "id": 346004, "url": "https://svs.gsfc.nasa.gov/11262/#media_group_346004", "widget": "Single image", "title": "", "caption": "", "description": "A burst of solar material leaps off the left side of the sun in what's known as a prominence eruption. This image combines three images from NASA's Solar Dynamics Observatory captured on May 3, 2013, at 1:45 pm EDT, just as an M-class solar flare from the same region was subsiding. The images include light from the 131-, 171- and 304-angstrom wavelengths.
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Credit: NASA/SDO/AIA", "items": [ { "id": 309532, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465908, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/May_3_Flare_171-304-131_blend.jpg", "filename": "May_3_Flare_171-304-131_blend.jpg", "media_type": "Image", "alt_text": "A burst of solar material leaps off the left side of the sun in what's known as a prominence eruption. This image combines three images from NASA's Solar Dynamics Observatory captured on May 3, 2013, at 1:45 pm EDT, just as an M-class solar flare from the same region was subsiding. The images include light from the 131-, 171- and 304-angstrom wavelengths. Full resolution 4k image.Credit: NASA/SDO/AIA", "width": 4096, "height": 4096, "pixels": 16777216 } }, { "id": 309533, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465909, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/May_3_Flare_171-304-131_blend_web.jpg", "filename": "May_3_Flare_171-304-131_blend_web.jpg", "media_type": "Image", "alt_text": "A burst of solar material leaps off the left side of the sun in what's known as a prominence eruption. This image combines three images from NASA's Solar Dynamics Observatory captured on May 3, 2013, at 1:45 pm EDT, just as an M-class solar flare from the same region was subsiding. The images include light from the 131-, 171- and 304-angstrom wavelengths. Full resolution 4k image.Credit: NASA/SDO/AIA", "width": 320, "height": 320, "pixels": 102400 } }, { "id": 309531, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465907, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/May_3_Flare_171-304-131_blend.tif", "filename": "May_3_Flare_171-304-131_blend.tif", "media_type": "Image", "alt_text": "A burst of solar material leaps off the left side of the sun in what's known as a prominence eruption. This image combines three images from NASA's Solar Dynamics Observatory captured on May 3, 2013, at 1:45 pm EDT, just as an M-class solar flare from the same region was subsiding. The images include light from the 131-, 171- and 304-angstrom wavelengths. Full resolution 4k image.Credit: NASA/SDO/AIA", "width": 4096, "height": 4096, "pixels": 16777216 } } ], "extra_data": {} }, { "id": 346006, "url": "https://svs.gsfc.nasa.gov/11262/#media_group_346006", "widget": "Single image", "title": "", "caption": "", "description": "NASA's Solar Dynamics Observatory captured this image of an M5.7-class flare on May 3, 2013, at 1:30 p.m. EDT. This image shows light in the 131-angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal.
Credit: NASA/SDO/AIA", "items": [ { "id": 309534, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465910, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_173046_4096_0131_copy_2.jpg", "filename": "20130503_173046_4096_0131_copy_2.jpg", "media_type": "Image", "alt_text": "NASA's Solar Dynamics Observatory captured this image of an M5.7-class flare on May 3, 2013, at 1:30 p.m. EDT. This image shows light in the 131-angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal.Credit: NASA/SDO/AIA", "width": 1538, "height": 1500, "pixels": 2307000 } }, { "id": 309535, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465911, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_173046_4096_0131_copy_2_web.jpg", "filename": "20130503_173046_4096_0131_copy_2_web.jpg", "media_type": "Image", "alt_text": "NASA's Solar Dynamics Observatory captured this image of an M5.7-class flare on May 3, 2013, at 1:30 p.m. EDT. This image shows light in the 131-angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal.Credit: NASA/SDO/AIA", "width": 320, "height": 312, "pixels": 99840 } } ], "extra_data": {} }, { "id": 346007, "url": "https://svs.gsfc.nasa.gov/11262/#media_group_346007", "widget": "Single image", "title": "", "caption": "", "description": "NASA's Solar Dynamics Observatory captured this image of an M5.7-class flare on May 3, 2013, at 1:30 p.m. EDT. This image shows light in the 131-angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal. Full resolution 4k image.
Credit: NASA/SDO/AIA", "items": [ { "id": 309536, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465912, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_173046_4096_0131_copy.jpg", "filename": "20130503_173046_4096_0131_copy.jpg", "media_type": "Image", "alt_text": "NASA's Solar Dynamics Observatory captured this image of an M5.7-class flare on May 3, 2013, at 1:30 p.m. EDT. This image shows light in the 131-angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal. Full resolution 4k image.Credit: NASA/SDO/AIA", "width": 4096, "height": 4096, "pixels": 16777216 } }, { "id": 309537, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465913, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_173046_4096_0131_copy_web.jpg", "filename": "20130503_173046_4096_0131_copy_web.jpg", "media_type": "Image", "alt_text": "NASA's Solar Dynamics Observatory captured this image of an M5.7-class flare on May 3, 2013, at 1:30 p.m. EDT. This image shows light in the 131-angstrom wavelength, a wavelength of light that can show material at the very hot temperatures of a solar flare and that is typically colorized in teal. Full resolution 4k image.Credit: NASA/SDO/AIA", "width": 320, "height": 320, "pixels": 102400 } } ], "extra_data": {} }, { "id": 346008, "url": "https://svs.gsfc.nasa.gov/11262/#media_group_346008", "widget": "Single image", "title": "", "caption": "", "description": "SOHO LASCO coronograph image from 18:47 UT on May 3. The white circle represents the sun.
Credit: SOHO/ESA&NASA", "items": [ { "id": 309538, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465914, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_1847_c2_1024.jpg", "filename": "20130503_1847_c2_1024.jpg", "media_type": "Image", "alt_text": "SOHO LASCO coronograph image from 18:47 UT on May 3. The white circle represents the sun.Credit: SOHO/ESA&NASA", "width": 1024, "height": 1024, "pixels": 1048576 } }, { "id": 309539, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465915, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_1847_c2_1024_web.jpg", "filename": "20130503_1847_c2_1024_web.jpg", "media_type": "Image", "alt_text": "SOHO LASCO coronograph image from 18:47 UT on May 3. The white circle represents the sun.Credit: SOHO/ESA&NASA", "width": 320, "height": 320, "pixels": 102400 } } ], "extra_data": {} }, { "id": 346009, "url": "https://svs.gsfc.nasa.gov/11262/#media_group_346009", "widget": "Single image", "title": "", "caption": "", "description": "SOHO LASCO coronograph image from 21:18 UT on May 3. The white circle represents the sun.
Credit: SOHO/ESA&NASA", "items": [ { "id": 309540, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465916, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_2118_c3_1024.jpg", "filename": "20130503_2118_c3_1024.jpg", "media_type": "Image", "alt_text": "SOHO LASCO coronograph image from 21:18 UT on May 3. The white circle represents the sun.Credit: SOHO/ESA&NASA", "width": 1024, "height": 1024, "pixels": 1048576 } }, { "id": 309541, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 465917, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011200/a011262/20130503_2118_c3_1024_web.jpg", "filename": "20130503_2118_c3_1024_web.jpg", "media_type": "Image", "alt_text": "SOHO LASCO coronograph image from 21:18 UT on May 3. The white circle represents the sun.Credit: SOHO/ESA&NASA", "width": 320, "height": 320, "pixels": 102400 } } ], "extra_data": {} }, { "id": 346010, "url": "https://svs.gsfc.nasa.gov/11262/#media_group_346010", "widget": "Basic text", "title": "For More Information", "caption": "", "description": "See [http://www.nasa.gov/mission_pages/sunearth/news/News050313-flare.html](http://www.nasa.gov/mission_pages/sunearth/news/News050313-flare.html)", "items": [], "extra_data": {} } ], "studio": "gms", "funding_sources": [ "NASA Heliophysics" ], "credits": [ { "role": "Producer", "people": [ { "name": "Scott Wiessinger", "employer": "USRA" }, { "name": "Genna Duberstein", "employer": "USRA" } ] }, { "role": "Writer", "people": [ { "name": "Karen Fox", "employer": "ADNET Systems, Inc." } ] } ], "missions": [ "SDO", "SOHO" ], "series": [ "Heliophysics Breaking News" ], "tapes": [ "2013 Heliophysics Breaking News (Produced by: Robert Crippen)" ], "papers": [], "datasets": [ { "name": "", "common_name": "", "platform": "SOHO", "sensor": null, "type": "Other", "organizations": [ "NASA and ESA" ], "description": "SOHO monitors the Sun with a variety of instruments.
Among the SOHO instruments is the Michelson Doppler Interferometer (MDI) and the Extreme ultraviolet Imaging Telescope (EIT).", "credit": "", "url": "http://sohowww.nascom.nasa.gov", "date_range": null }, { "name": "", "common_name": "", "platform": "SDO", "sensor": null, "type": "Other", "organizations": [], "description": "", "credit": "", "url": "http://sdo.gsfc.nasa.gov/", "date_range": null } ], "nasa_science_categories": [ "Sun" ], "keywords": [ "Corona", "Earth Science", "Heliophysics", "SDO", "Solar Activity", "Solar Dynamics Observatory", "Solar Flares", "Solar Ultraviolet", "Space Weather", "Sun-earth Interactions" ], "recommended_pages": [], "related": [ { "id": 11179, "url": "https://svs.gsfc.nasa.gov/11179/", "page_type": "Produced Video", "title": "Space Weather Vocabulary", "description": "We are all familiar with weather on Earth, but how much do you know about weather in space? Suitable for all ages, this introduction to space weather covers vocabulary like coronal mass ejection (CME), solar wind, and solar flare. It also outlines potential effects of solar storms on our planet.This video is available in English and Spanish, both with English subtitles.Todo el mundo está familiarizado con el clima de la Tierra pero, ¿cuánto sabes sobre meteorología espacial? Este video introductorio al clima espacial, apropiado para todas las edades y niveles, explica términos científicos como eyección de masa coronal, viento solar o erupción solar.También provee una descripción general sobre los efectos potenciales que tienen las tormentas solares en nuestro planeta.El vídeo está disponible en español e inglés, ambas versiones con subtítulos en inglés. || ", "release_date": "2013-02-26T00:00:00-05:00", "update_date": "2023-05-03T13:52:22.850331-04:00", "main_image": { "id": 468113, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a011100/a011179/vocab320.jpg", "filename": "vocab320.jpg", "media_type": "Image", "alt_text": "Video in English.For complete transcript, click here.", "width": 320, "height": 180, "pixels": 57600 } }, { "id": 10959, "url": "https://svs.gsfc.nasa.gov/10959/", "page_type": "Produced Video", "title": "NASA Scientists Answer Top Space Weather Questions", "description": "NASA scientists answer some common questions about the sun, space weather, and how they affect the Earth. This is a two-part series.Part One addresses:1. What is space weather?2. What are coronal mass ejections?3. What are solar flares?4. What are solar energetic particles?5. What causes flares and CMEs?Part Two addresses:1. Do all flares and CMEs affect the Earth?2. What happens when a flare or CME hits the Earth?3. How quickly can we feel the effects of space weather?4. Why are there more flares and CMEs happening now?For more information about all these questions and more, visit NASA's Space Weather FAQ.For individual interview responses to frequently asked space weather questions, go here. || ", "release_date": "2012-04-24T10:00:00-04:00", "update_date": "2023-05-03T13:53:06.910171-04:00", "main_image": { "id": 476895, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a010900/a010959/SW_Part1_Still.png", "filename": "SW_Part1_Still.png", "media_type": "Image", "alt_text": "Part 1For complete transcript, click here.", "width": 1280, "height": 720, "pixels": 921600 } }, { "id": 10109, "url": "https://svs.gsfc.nasa.gov/10109/", "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 } } ], "sources": [], "products": [], "newer_versions": [], "older_versions": [], "alternate_versions": [] }