{
    "count": 5,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 5165,
            "url": "https://svs.gsfc.nasa.gov/5165/",
            "result_type": "Visualization",
            "release_date": "2024-01-05T00:00:00-05:00",
            "title": "STEREO - The Second Time Around...",
            "description": "In mid-August 2023, the still-operational STEREO-A (STEREO-B went offline in October 2014) passed Earth for the first time since its launch 17 years ago. See also STEREO-A Returns by Earth.While STEREO-B is no longer available, it is possible to construct stereo imagery of the Sun using STEREO-A with Solar Dynamics Observatory (SDO).  Here we present a series of images for corresponding filters between the two missions which can be used for stereo viewing.Color (SDO color table) Left/Right Image PairsIn this section, we present frame-synchronized left eye (STEREO-A) and right eye (SDO) for the specified ultraviolet filter.  They are provided as separate movie and frame-sets to maximize flexibility for the target viewing technology.  Time stamps are provided as separate image files for compositing if desired.   If you match frame numbers for the image sets for a specific filter, you will have images closest in time for apropriate left/right eye pairing.171 Angstrom filter || ",
            "hits": 30
        },
        {
            "id": 4500,
            "url": "https://svs.gsfc.nasa.gov/4500/",
            "result_type": "Visualization",
            "release_date": "2016-10-25T10:00:00-04:00",
            "title": "STEREO in stereo: Spring 2007 at 195 Ångstroms",
            "description": "Red/Cyan stereo glasses are required to view it properly. || 2007stereo_STEREO_RedCyan_010_EUVI195A_UHD3840.02000_print.jpg (1024x576) [51.7 KB] || 2007stereo_RedCyan_010_EUVI195A_2160p30.mp4 (3840x2160) [287.8 MB] || RedCyan (3840x2160) [512.0 KB] || 2007stereo_RedCyan_010_EUVI195A_2160p30.webm (3840x2160) [12.6 MB] || ",
            "hits": 24
        },
        {
            "id": 4177,
            "url": "https://svs.gsfc.nasa.gov/4177/",
            "result_type": "Visualization",
            "release_date": "2014-07-23T00:00:00-04:00",
            "title": "As Seen by STEREO-A: The Carrington-Class CME of 2012",
            "description": "STEREO-A, at a position along Earth's orbit where it has an unobstructed view of the far side of the Sun, could clearly observe possibly the most powerful coronal mass ejection (CME) of solar cyle 24 on July 23, 2012.  The visualizations on this page cover the entire day.We see the flare erupt in the lower right quadrant of the solar disk from a large active region.  The material is launched into space in a direction towards STEREO-A.  This creates the ring-like 'halo' CME visible in the STEREO-A coronagraph, COR-2 (blue circular image).As the CME expands beyond the field of view of the COR-2 imager, the high energy particles reach STEREO-A, creating the snow-like noise in the image.  The particles also strike the HI-2 imager (blue square) brightening the image.The HI-1 imager has had 'bloom removal' enabled and filled with contents of the immediately previous HI-1 image, which creates a linear artifact above and below bright stars and planets. || ",
            "hits": 244
        },
        {
            "id": 3694,
            "url": "https://svs.gsfc.nasa.gov/3694/",
            "result_type": "Visualization",
            "release_date": "2010-03-24T00:00:00-04:00",
            "title": "A Comparative View of the Sun: SDO/AIA 193 and STEREO-B/EUVI 195",
            "description": "This movie compares the spatial and temporal resolutions of the SDO/AIA (Atmospheric Imaging Assembly) imager to the STEREO/EUVI (Extreme UltraViolet Imager) imager. STEREO-B/EUVI's highest resolution is 2048x2048 pixels with images taken about every 5 minutes for the 195 Ångstrom band. The SDO/AIA 193 band takes images at 4096x4096 pixels every twelve seconds!While STEREO's vantage point at this time is very different from SDO, we can still identify some features of the Active Region 1087 in these two views. EUVI shows the launch of the filament, while AIA reveals many finer details.This visualization is a companion piece to A Comparative View of the Sun: SDO/AIA 193 and SOHO/EIT 195. || ",
            "hits": 20
        },
        {
            "id": 3428,
            "url": "https://svs.gsfc.nasa.gov/3428/",
            "result_type": "Visualization",
            "release_date": "2007-04-25T12:00:00-04:00",
            "title": "First 3-D Stereo from STEREO: EUVI 195 Angstroms (Full Disk View)",
            "description": "This movie shows the Sun from the two STEREO spacecraft using the 195 || ",
            "hits": 37
        }
    ]
}