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    "title": "RHESSI and TRACE View of January 20, 2005 Solar Flare",
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            "description": "As the TRACE imager saturates, we see multiple hot-spots at the loop footpoints in RHESSI.",
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            "description": "Closeup of AR 10720.  Blue high-energy emission marks the footpoints of the coronal loops.  The lower-energy red emission is from the\nloop structure.  See note below under ImageMods.",
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            "widget": "Basic text",
            "title": "For More Information",
            "caption": "",
            "description": "See [http://www.nasa.gov/vision/universe/solarsystem/solar_fireworks.html](http://www.nasa.gov/vision/universe/solarsystem/solar_fireworks.html)",
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    "credits": [
        {
            "role": "Animator",
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                {
                    "name": "Tom Bridgman",
                    "employer": "Global Science and Technology, Inc."
                }
            ]
        },
        {
            "role": "Scientist",
            "people": [
                {
                    "name": "Robert Lin",
                    "employer": "University of California at Berkeley"
                },
                {
                    "name": "Richard Mewaldt",
                    "employer": "CalTech"
                },
                {
                    "name": "Richard Nightingale",
                    "employer": "LMSAL"
                }
            ]
        }
    ],
    "missions": [
        "RHESSI",
        "TRACE"
    ],
    "series": [
        "Astrophysics Stills",
        "New Space Weather Mystery"
    ],
    "tapes": [],
    "papers": [],
    "datasets": [
        {
            "name": "",
            "common_name": "",
            "platform": "RHESSI",
            "sensor": "X-ray Imaging Spectrometer",
            "type": "Other",
            "organizations": [],
            "description": "The RHESSI instrument is an imaging spectrometer observing the Sun at X-ray to gamma-rays (photon energies of 3 keV to 17 MeV) at time resolutions of a few seconds.  (<a href=\"http://imagine.gsfc.nasa.gov/docs/features/topics/snr_group/eV.html\">eV</a> stands for &quot;electron volt&quot; and is a unit of energy.  Note that photons of visible light have energies of 2-3 eV.  1 keV is a thousand electron volts and 1 MeV is a million electron volts.",
            "credit": "",
            "url": "http://hesperia.gsfc.nasa.gov/hessi/",
            "date_range": "2005/01/20T06:20:13 - 2005/01/20T07:26:00"
        },
        {
            "name": "1600 Angstroms",
            "common_name": "",
            "platform": "TRACE",
            "sensor": "Optical Telescope",
            "type": "Other",
            "organizations": [],
            "description": "",
            "credit": "",
            "url": "",
            "date_range": "2005/01/20T06:20:00 - 2005/01/20T08:43:57"
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    ],
    "nasa_science_categories": [
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    ],
    "keywords": [
        "Active Region 10720",
        "Earth Science",
        "RHESSI",
        "Solar Active Regions",
        "Solar Activity",
        "Solar Flares",
        "Space science",
        "Space Weather",
        "Sun-earth Interactions",
        "TRACE",
        "X-ray",
        "X-ray Imaging"
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    "recommended_pages": [],
    "related": [],
    "sources": [],
    "products": [],
    "newer_versions": [],
    "older_versions": [],
    "alternate_versions": []
}