{
    "count": 9,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 3346,
            "url": "https://svs.gsfc.nasa.gov/3346/",
            "result_type": "Visualization",
            "release_date": "2006-03-30T00:00:00-05:00",
            "title": "Grand Tour of the Coronal Loops Model",
            "description": "This is a longer coronal loops tour combining components of the two previous versions (Animation IDs 3286 and 3287). The solar model is constructed from magnetogram data collected by SOHO/MDI. Because we do not see the full solar surface at any one time, the magnetograms collected over the course of a solar rotation are processed through a time-evolving solar surface model which provides a snapshot of the surface at a fixed time. The resulting magnetogram is then processed through the Potential Field Source Surface (PFSS) model which constructs the magnetic field above the solar surface. The magnetic field around the Sun is then analyzed for field lines, which creates the loop structures we see in the model. Hot plasma tends to flow along the magnetic field lines, creating the coronal loops. These loops are only visible at the higher temperatures corresponding to ultraviolet light, in this case, 195 angstroms, one of the filter wavelengths of SOHO/EIT. For this version, we color the coronal loops green for ready comparison to the EIT 195 angstrom imagery using the EIT standard color table. || ",
            "hits": 95
        },
        {
            "id": 3286,
            "url": "https://svs.gsfc.nasa.gov/3286/",
            "result_type": "Visualization",
            "release_date": "2005-10-27T00:00:00-04:00",
            "title": "Flight through the Coronal Loops",
            "description": "Here we illustrate the potential benefits of the 3-D views of the Sun which STEREO will provide. Starting with a simple 2-D EIT ultraviolet image from SOHO, we transition to a 3-D model and move through the coronal loops which are constructed along solar magnetic fields. The solar model is constructed from magnetogram data collected by SOHO/MDI. Because we do not see the full solar surface at any one time, the magnetograms collected over the course of a solar rotation are processed through a time-evolving solar surface model to provide a snapshot of the surface at a fixed time. The resulting magnetogram is then processed through the Potential Field Source Surface (PFSS) model. Coronal loops are visible at the higher temperatures of ultraviolet light, in this case, 195 angstroms, the filter wavelength of SOHO/EIT. For this version, we color the coronal loops green for ready comparison to the EIT 195 angstrom imagery using the EIT 'standard color table'. || ",
            "hits": 58
        },
        {
            "id": 3287,
            "url": "https://svs.gsfc.nasa.gov/3287/",
            "result_type": "Visualization",
            "release_date": "2005-10-27T00:00:00-04:00",
            "title": "Rotating Tour of Solar Coronal Loops",
            "description": "A slow rotating tour of a data-based coronal loop model. This version is designed for continuous loop play. The solar model is constructed from magnetogram data collected by SOHO/MDI. Because we do not see the full solar surface at any one time, the magnetograms collected over the course of a solar rotation are processed through a time-evolving solar surface model to provide a snapshot of the surface at a fixed time. The resulting magnetogram is then processed through the Potential Field Source Surface (PFSS) model. Coronal loops are visible at the higher temperatures of ultraviolet light, in this case, 195 angstroms, the filter wavelength of SOHO/EIT. || ",
            "hits": 89
        },
        {
            "id": 20064,
            "url": "https://svs.gsfc.nasa.gov/20064/",
            "result_type": "Animation",
            "release_date": "2005-04-27T12:00:00-04:00",
            "title": "Model for Coronal Mass Ejections",
            "description": "A coronal mass ejection (CME) is a massive burst of solar wind, other light isotope plasma, and magnetic fields rising above the solar corona or being released into space. || CME_640x480_pre.00002_print.jpg (1024x768) [45.1 KB] || CME_640x480_thm.png (80x40) [4.5 KB] || CME_640x480_pre.jpg (320x240) [3.1 KB] || CME_320x240_pre.jpg (320x240) [2.9 KB] || CME_320x240_pre_searchweb.jpg (320x180) [11.8 KB] || CME_NTSC.webmhd.webm (960x540) [1.1 MB] || 720x486_4x3_30 (720x486) [32.0 KB] || CME_640x480.mpg (640x480) [10.7 MB] || CME_NTSC.m2v (720x480) [17.2 MB] || a010066_seq.mpg (720x480) [8.2 MB] || a010066_H264_640x480.mp4 (640x480) [7.1 MB] || CME_320x240.mpg (320x240) [2.8 MB] || ",
            "hits": 62
        },
        {
            "id": 20062,
            "url": "https://svs.gsfc.nasa.gov/20062/",
            "result_type": "Animation",
            "release_date": "2005-04-26T12:00:00-04:00",
            "title": "STEREO Watches the Active Sun",
            "description": "The Sun belches out gas at thousands of kilometers per second as the STEREO A spacecraft looks on. || stereo_640x480_pre.00002_print.jpg (1024x768) [47.0 KB] || stereo_640x480_pre.jpg (320x240) [4.4 KB] || stereo_320x240_pre.jpg (320x240) [4.2 KB] || STEREO_flyby_720p.m2v (1280x720) [12.0 MB] || 1280x720_16x9_30 (1280x720) [32.0 KB] || 1920x1080_16x9_30 (1920x1080) [64.0 KB] || a010064_H264_1280x720.mp4 (1280x720) [7.9 MB] || stereo_NTSC.webmhd.webm (960x540) [4.5 MB] || 720x486_4x3_30 (720x486) [32.0 KB] || stereo_640x480.mpg (640x480) [12.0 MB] || stereo_NTSC.m2v (720x480) [19.2 MB] || a010064_1280x720_seq.mpg (720x480) [14.5 MB] || a010064_720x486_seq.mpg (720x480) [16.3 MB] || a010064_H264_640x480.mp4 (640x480) [7.7 MB] || stereo_320x240.mpg (320x240) [3.1 MB] || STEREO_flyby_512x288.mpg (512x288) [3.1 MB] || ",
            "hits": 44
        },
        {
            "id": 20058,
            "url": "https://svs.gsfc.nasa.gov/20058/",
            "result_type": "Animation",
            "release_date": "2005-04-12T12:00:00-04:00",
            "title": "STEREO On-Station",
            "description": "The STEREO spacecraft will observed the Sun and the region between the Sun and the Earth from the Lagrange Points of the Sun-Earth system. || ",
            "hits": 51
        },
        {
            "id": 20059,
            "url": "https://svs.gsfc.nasa.gov/20059/",
            "result_type": "Animation",
            "release_date": "2005-04-12T12:00:00-04:00",
            "title": "STEREO Enroute: The Lunar Flyby",
            "description": "STEREO A and B get a gravity-assist for their trajectory in a fly-by of the Moon. || ",
            "hits": 50
        },
        {
            "id": 20060,
            "url": "https://svs.gsfc.nasa.gov/20060/",
            "result_type": "Animation",
            "release_date": "2005-04-12T12:00:00-04:00",
            "title": "STEREO Spacecraft Beauty-Pass",
            "description": "A close-up view of a STEREO satellite. || ",
            "hits": 42
        },
        {
            "id": 20061,
            "url": "https://svs.gsfc.nasa.gov/20061/",
            "result_type": "Animation",
            "release_date": "2005-04-12T12:00:00-04:00",
            "title": "STEREO Enroute: Earth Flyby",
            "description": "STEREO A gets a final boost in velocity with a gravity-assist by the Earth. || ",
            "hits": 47
        }
    ]
}