{
    "id": 4066,
    "url": "https://svs.gsfc.nasa.gov/4066/",
    "page_type": "Visualization",
    "title": "SDO's Multi-wavelength View of a May 2013 Solar Flare",
    "description": "An active region on the left limb of the Sun launches a large flare and coronal material in this sequence from early May 2013. || ",
    "release_date": "2014-02-11T10:00:00-05:00",
    "update_date": "2025-02-02T22:10:52.532650-05:00",
    "main_image": {
        "id": 459251,
        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_stand.HD1080i.00200.jpg",
        "filename": "May2013Flare_304A_stand.HD1080i.00200.jpg",
        "media_type": "Image",
        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
        "width": 1920,
        "height": 1080,
        "pixels": 2073600
    },
    "main_video": null,
    "main_credits": {
        "Visualizations by": [
            {
                "name": "Tom Bridgman",
                "employer": "Global Science and Technology, Inc."
            }
        ]
    },
    "progress": "Complete",
    "media_groups": [
        {
            "id": 341785,
            "url": "https://svs.gsfc.nasa.gov/4066/#media_group_341785",
            "widget": "Basic text with HTML",
            "title": "",
            "caption": "",
            "description": "An active region on the left limb of the Sun launches a large flare and coronal material in this sequence from early May 2013.",
            "items": [],
            "extra_data": {}
        },
        {
            "id": 341786,
            "url": "https://svs.gsfc.nasa.gov/4066/#media_group_341786",
            "widget": "Video player",
            "title": "",
            "caption": "",
            "description": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
            "items": [
                {
                    "id": 294863,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459236,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_stand.HD1080i.00200.jpg",
                        "filename": "May2013Flare_131A_stand.HD1080i.00200.jpg",
                        "media_type": "Image",
                        "alt_text": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294862,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459233,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_stand.HD1080i.00200_web.png",
                        "filename": "May2013Flare_131A_stand.HD1080i.00200_web.png",
                        "media_type": "Image",
                        "alt_text": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 320,
                        "height": 180,
                        "pixels": 57600
                    }
                },
                {
                    "id": 294858,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459235,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_HD720.mov",
                        "filename": "May2013Flare_131A_HD720.mov",
                        "media_type": "Movie",
                        "alt_text": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 1280,
                        "height": 720,
                        "pixels": 921600
                    }
                },
                {
                    "id": 294860,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459237,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_HD1080.webmhd.webm",
                        "filename": "May2013Flare_131A_HD1080.webmhd.webm",
                        "media_type": "Movie",
                        "alt_text": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 960,
                        "height": 540,
                        "pixels": 518400
                    }
                },
                {
                    "id": 294861,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459232,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/1920x1080_16x9_30p/AIA131A/",
                        "filename": "AIA131A",
                        "media_type": "Frames",
                        "alt_text": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294857,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459231,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_HD1080.mov",
                        "filename": "May2013Flare_131A_HD1080.mov",
                        "media_type": "Movie",
                        "alt_text": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294859,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459234,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_iPod.m4v",
                        "filename": "May2013Flare_131A_iPod.m4v",
                        "media_type": "Movie",
                        "alt_text": "A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 640,
                        "height": 360,
                        "pixels": 230400
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 341787,
            "url": "https://svs.gsfc.nasa.gov/4066/#media_group_341787",
            "widget": "Video player",
            "title": "",
            "caption": "",
            "description": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
            "items": [
                {
                    "id": 294870,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459243,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_stand.HD1080i.00200.jpg",
                        "filename": "May2013Flare_171A_stand.HD1080i.00200.jpg",
                        "media_type": "Image",
                        "alt_text": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294869,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459240,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_stand.HD1080i.00200_web.png",
                        "filename": "May2013Flare_171A_stand.HD1080i.00200_web.png",
                        "media_type": "Image",
                        "alt_text": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 320,
                        "height": 180,
                        "pixels": 57600
                    }
                },
                {
                    "id": 294864,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459238,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_HD1080.mov",
                        "filename": "May2013Flare_171A_HD1080.mov",
                        "media_type": "Movie",
                        "alt_text": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294865,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459241,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_HD720.mov",
                        "filename": "May2013Flare_171A_HD720.mov",
                        "media_type": "Movie",
                        "alt_text": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 1280,
                        "height": 720,
                        "pixels": 921600
                    }
                },
                {
                    "id": 294867,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459244,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_HD1080.webmhd.webm",
                        "filename": "May2013Flare_171A_HD1080.webmhd.webm",
                        "media_type": "Movie",
                        "alt_text": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 960,
                        "height": 540,
                        "pixels": 518400
                    }
                },
                {
                    "id": 294868,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459239,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/1920x1080_16x9_30p/AIA171A/",
                        "filename": "AIA171A",
                        "media_type": "Frames",
                        "alt_text": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294866,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459242,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_iPod.m4v",
                        "filename": "May2013Flare_171A_iPod.m4v",
                        "media_type": "Movie",
                        "alt_text": "In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 640,
                        "height": 360,
                        "pixels": 230400
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 341788,
            "url": "https://svs.gsfc.nasa.gov/4066/#media_group_341788",
            "widget": "Video player",
            "title": "",
            "caption": "",
            "description": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
            "items": [
                {
                    "id": 294878,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459251,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_stand.HD1080i.00200.jpg",
                        "filename": "May2013Flare_304A_stand.HD1080i.00200.jpg",
                        "media_type": "Image",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294875,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459247,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_stand.HD1080i.00200_web.png",
                        "filename": "May2013Flare_304A_stand.HD1080i.00200_web.png",
                        "media_type": "Image",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 320,
                        "height": 180,
                        "pixels": 57600
                    }
                },
                {
                    "id": 294877,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459248,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_stand.HD1080i.00200_thm.png",
                        "filename": "May2013Flare_304A_stand.HD1080i.00200_thm.png",
                        "media_type": "Image",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 80,
                        "height": 40,
                        "pixels": 3200
                    }
                },
                {
                    "id": 294871,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459246,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_HD1080.mov",
                        "filename": "May2013Flare_304A_HD1080.mov",
                        "media_type": "Movie",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294872,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459249,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_HD720.mov",
                        "filename": "May2013Flare_304A_HD720.mov",
                        "media_type": "Movie",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 1280,
                        "height": 720,
                        "pixels": 921600
                    }
                },
                {
                    "id": 294874,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459245,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/1920x1080_16x9_30p/AIA304A/",
                        "filename": "AIA304A",
                        "media_type": "Frames",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 1920,
                        "height": 1080,
                        "pixels": 2073600
                    }
                },
                {
                    "id": 294876,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459252,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_HD1080.webmhd.webm",
                        "filename": "May2013Flare_304A_HD1080.webmhd.webm",
                        "media_type": "Movie",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 960,
                        "height": 540,
                        "pixels": 518400
                    }
                },
                {
                    "id": 294873,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459250,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_iPod.m4v",
                        "filename": "May2013Flare_304A_iPod.m4v",
                        "media_type": "Movie",
                        "alt_text": "In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 640,
                        "height": 360,
                        "pixels": 230400
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 341789,
            "url": "https://svs.gsfc.nasa.gov/4066/#media_group_341789",
            "widget": "Video player",
            "title": "",
            "caption": "",
            "description": "4Kx4K full resolution images.  A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
            "items": [
                {
                    "id": 294882,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459257,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A.00150.jpg",
                        "filename": "May2013Flare_131A.00150.jpg",
                        "media_type": "Image",
                        "alt_text": "4Kx4K full resolution images.  A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                },
                {
                    "id": 294884,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459255,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A.00150_web.png",
                        "filename": "May2013Flare_131A.00150_web.png",
                        "media_type": "Image",
                        "alt_text": "4Kx4K full resolution images.  A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 320,
                        "height": 320,
                        "pixels": 102400
                    }
                },
                {
                    "id": 294883,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459258,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_1Kx1K.webmhd.webm",
                        "filename": "May2013Flare_131A_1Kx1K.webmhd.webm",
                        "media_type": "Movie",
                        "alt_text": "4Kx4K full resolution images.  A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 960,
                        "height": 540,
                        "pixels": 518400
                    }
                },
                {
                    "id": 294879,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459256,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_131A_1Kx1K.mov",
                        "filename": "May2013Flare_131A_1Kx1K.mov",
                        "media_type": "Movie",
                        "alt_text": "4Kx4K full resolution images.  A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 1024,
                        "height": 1024,
                        "pixels": 1048576
                    }
                },
                {
                    "id": 294880,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459253,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/4096x4096_1x1_30p/131A-Frames/",
                        "filename": "131A-Frames",
                        "media_type": "Frames",
                        "alt_text": "4Kx4K full resolution images.  A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                },
                {
                    "id": 294881,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459254,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/4096x4096_1x1_30p/131A-Time/",
                        "filename": "131A-Time",
                        "media_type": "Frames",
                        "alt_text": "4Kx4K full resolution images.  A view of the flare in the 13.1nm filter.  The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise.  The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD.  The 'waffle' pattern is also an artifact of the imaging system with bright events.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 341790,
            "url": "https://svs.gsfc.nasa.gov/4066/#media_group_341790",
            "widget": "Video player",
            "title": "",
            "caption": "",
            "description": "4Kx4K full resolution images.  In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
            "items": [
                {
                    "id": 294888,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459263,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A.00150.jpg",
                        "filename": "May2013Flare_171A.00150.jpg",
                        "media_type": "Image",
                        "alt_text": "4Kx4K full resolution images.  In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                },
                {
                    "id": 294890,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459261,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A.00150_web.png",
                        "filename": "May2013Flare_171A.00150_web.png",
                        "media_type": "Image",
                        "alt_text": "4Kx4K full resolution images.  In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 320,
                        "height": 320,
                        "pixels": 102400
                    }
                },
                {
                    "id": 294885,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459262,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_1Kx1K.mov",
                        "filename": "May2013Flare_171A_1Kx1K.mov",
                        "media_type": "Movie",
                        "alt_text": "4Kx4K full resolution images.  In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 1024,
                        "height": 1024,
                        "pixels": 1048576
                    }
                },
                {
                    "id": 294889,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459264,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_171A_1Kx1K.webmhd.webm",
                        "filename": "May2013Flare_171A_1Kx1K.webmhd.webm",
                        "media_type": "Movie",
                        "alt_text": "4Kx4K full resolution images.  In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 960,
                        "height": 540,
                        "pixels": 518400
                    }
                },
                {
                    "id": 294886,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459259,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/4096x4096_1x1_30p/171A-Frames/",
                        "filename": "171A-Frames",
                        "media_type": "Frames",
                        "alt_text": "4Kx4K full resolution images.  In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                },
                {
                    "id": 294887,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459260,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/4096x4096_1x1_30p/171A-Time/",
                        "filename": "171A-Time",
                        "media_type": "Frames",
                        "alt_text": "4Kx4K full resolution images.  In the filter for 17.1nm light, the flare is not as bright, but exhibits twisting hot plasma that erupts from the Sun.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 341791,
            "url": "https://svs.gsfc.nasa.gov/4066/#media_group_341791",
            "widget": "Video player",
            "title": "",
            "caption": "",
            "description": "4Kx4K full resolution images.  In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
            "items": [
                {
                    "id": 294894,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459269,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A.00150.jpg",
                        "filename": "May2013Flare_304A.00150.jpg",
                        "media_type": "Image",
                        "alt_text": "4Kx4K full resolution images.  In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                },
                {
                    "id": 294896,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459267,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A.00150_web.png",
                        "filename": "May2013Flare_304A.00150_web.png",
                        "media_type": "Image",
                        "alt_text": "4Kx4K full resolution images.  In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 320,
                        "height": 320,
                        "pixels": 102400
                    }
                },
                {
                    "id": 294895,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459270,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_1Kx1K.webmhd.webm",
                        "filename": "May2013Flare_304A_1Kx1K.webmhd.webm",
                        "media_type": "Movie",
                        "alt_text": "4Kx4K full resolution images.  In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 960,
                        "height": 540,
                        "pixels": 518400
                    }
                },
                {
                    "id": 294891,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459268,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/May2013Flare_304A_1Kx1K.mov",
                        "filename": "May2013Flare_304A_1Kx1K.mov",
                        "media_type": "Movie",
                        "alt_text": "4Kx4K full resolution images.  In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 1024,
                        "height": 1024,
                        "pixels": 1048576
                    }
                },
                {
                    "id": 294892,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459266,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/4096x4096_1x1_30p/304A-Time/",
                        "filename": "304A-Time",
                        "media_type": "Frames",
                        "alt_text": "4Kx4K full resolution images.  In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                },
                {
                    "id": 294893,
                    "type": "media",
                    "extra_data": null,
                    "title": null,
                    "caption": null,
                    "instance": {
                        "id": 459265,
                        "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004000/a004066/frames/4096x4096_1x1_30p/304A-Frames/",
                        "filename": "304A-Frames",
                        "media_type": "Frames",
                        "alt_text": "4Kx4K full resolution images.  In the 30.4nm wavelength of the helium ion, we can see both the flare, as well as some of the ejected solar material.",
                        "width": 4096,
                        "height": 4096,
                        "pixels": 16777216
                    }
                }
            ],
            "extra_data": {}
        }
    ],
    "studio": "svs",
    "funding_sources": [
        "NASA Heliophysics"
    ],
    "credits": [
        {
            "role": "Animator",
            "people": [
                {
                    "name": "Tom Bridgman",
                    "employer": "Global Science and Technology, Inc."
                }
            ]
        },
        {
            "role": "Producer",
            "people": [
                {
                    "name": "Scott Wiessinger",
                    "employer": "USRA"
                }
            ]
        },
        {
            "role": "Scientist",
            "people": [
                {
                    "name": "None None",
                    "employer": "SDO Science Team and the Virtual Solar Observatory"
                }
            ]
        },
        {
            "role": "Project support",
            "people": [
                {
                    "name": "Laurence Schuler",
                    "employer": "ADNET Systems, Inc."
                },
                {
                    "name": "Ian Jones",
                    "employer": "ADNET Systems, Inc."
                }
            ]
        }
    ],
    "missions": [
        "SDO"
    ],
    "series": [
        "Solar Dynamics Observatory: Year 4"
    ],
    "tapes": [],
    "papers": [],
    "datasets": [
        {
            "name": "304 Filter",
            "common_name": "AIA 304",
            "platform": "SDO",
            "sensor": "AIA",
            "type": "Other",
            "organizations": [
                "JOINT SCIENCE OPERATIONS CENTER "
            ],
            "description": "",
            "credit": "",
            "url": "http://jsoc.stanford.edu/",
            "date_range": "2013-05-03T17:00:00 - 2013-05-03T19:30:00"
        },
        {
            "name": "171 Filter",
            "common_name": "AIA 171",
            "platform": "SDO",
            "sensor": "AIA",
            "type": "Other",
            "organizations": [
                "JOINT SCIENCE OPERATIONS CENTER "
            ],
            "description": "",
            "credit": "",
            "url": "http://jsoc.stanford.edu/",
            "date_range": "2013-05-03T17:00:00 - 2013-05-03T19:30:00"
        },
        {
            "name": "131 Filter",
            "common_name": "AIA 131",
            "platform": "SDO",
            "sensor": "AIA",
            "type": "Other",
            "organizations": [
                "JOINT SCIENCE OPERATIONS CENTER "
            ],
            "description": "",
            "credit": "",
            "url": "http://jsoc.stanford.edu/",
            "date_range": "2013-05-03T17:00:00 - 2013-05-03T19:30:00"
        }
    ],
    "nasa_science_categories": [
        "Sun"
    ],
    "keywords": [
        "Corona",
        "Coronal Mass Ejections",
        "Earth Science",
        "EUV Imaging",
        "Extreme Ultraviolet Imaging",
        "HDTV",
        "Heliophysics",
        "Hyperwall",
        "SDO",
        "Solar Activity",
        "Solar Dynamics Observatory",
        "Solar Flares",
        "Solar Ultraviolet",
        "Solar Wind",
        "Space Weather",
        "Sun-earth Interactions"
    ],
    "recommended_pages": [],
    "related": [],
    "sources": [],
    "products": [],
    "newer_versions": [],
    "older_versions": [],
    "alternate_versions": []
}