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            "description": "The 2.2MeV emission fades and the other footpoint appears.",
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            "caption": "",
            "description": "High energy emission drops with some low energy still visible.",
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                        "alt_text": "Still low-energy emission.  Loops more visible in Hydrogen-Alpha.",
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            "caption": "",
            "description": "The coronal loops glow brightly in TRACE 195 angstrom band.",
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            "description": "The loops continue to fade in TRACE.",
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                        "alt_text": "The loops continue to fade in TRACE.",
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            "caption": "",
            "description": "Video slate image says, \"RHESS Observes 2.2 MeV Line Emission from a Solar Flare<p>The solar flare at Active Region AR 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 keV electron-positron (antimatter) annihilation line. In the animation, the RHESSI low-energy channels (12-25 keV) are represented in red and appears predominantly in coronal loops. The high-energy flux appears as blue at the footpoints of the coronal loops. Violet is used to indicate the location and relative intensity of the 2.2MeV emission.\"",
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                        "alt_text": "Video slate image says, \"RHESS Observes 2.2 MeV Line Emission from a Solar FlareThe solar flare at Active Region AR 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 keV electron-positron (antimatter) annihilation line. In the animation, the RHESSI low-energy channels (12-25 keV) are represented in red and appears predominantly in coronal loops. The high-energy flux appears as blue at the footpoints of the coronal loops. Violet is used to indicate the location and relative intensity of the 2.2MeV emission.\"",
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                        "alt_text": "Video slate image says, \"RHESS Observes 2.2 MeV Line Emission from a Solar FlareThe solar flare at Active Region AR 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 keV electron-positron (antimatter) annihilation line. In the animation, the RHESSI low-energy channels (12-25 keV) are represented in red and appears predominantly in coronal loops. The high-energy flux appears as blue at the footpoints of the coronal loops. Violet is used to indicate the location and relative intensity of the 2.2MeV emission.\"",
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    "credits": [
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            "people": [
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                    "name": "Tom Bridgman",
                    "employer": "Global Science and Technology, Inc."
                },
                {
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                    "employer": "Global Science and Technology, Inc."
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                    "name": "Robert Lin",
                    "employer": "University of California at Berkeley"
                },
                {
                    "name": "Sam Krucker",
                    "employer": "University of California at Berkeley"
                },
                {
                    "name": "Gordon J. Hurford",
                    "employer": "University of California at Berkeley"
                },
                {
                    "name": "Ronald J. Murphy",
                    "employer": "NRL"
                },
                {
                    "name": "G. H. Share",
                    "employer": "NRL"
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                {
                    "name": "X.-M. Hua",
                    "employer": "L-3 Communications Analytics Corporation"
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                {
                    "name": "David M. Smith",
                    "employer": "University of California at Berkeley"
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                {
                    "name": "Richard A. Schwartz",
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                },
                {
                    "name": "Benzion Kozlovsky",
                    "employer": "Tel Aviv University"
                }
            ]
        },
        {
            "role": "Writer",
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            "credit": "",
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            "url": "http://hesperia.gsfc.nasa.gov/hessi/",
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            "common_name": "",
            "platform": "TRACE",
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            "organizations": [],
            "description": "The TRACE satellite views the Sun at ultraviolet wavelengths with high temporal (approximately 1-12 seconds) and spatial (1 arcsecond per pixel) resolution.  Launched on April 2, 1998, it orbits the Earth in a Sun-synchronous orbit.",
            "credit": "",
            "url": "http://sunland.gsfc.nasa.gov/smex/trace/",
            "date_range": "2002/07/23T00:00:59-2002/07/23T03:32:45"
        },
        {
            "name": "H-alpha",
            "common_name": "",
            "platform": "Big Bear Solar Observatory",
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            "type": "Observed Data",
            "organizations": [
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            "description": "Solar imagery in Hydrogen-alpha spectral line",
            "credit": "",
            "url": "http://www.bbso.njit.edu",
            "date_range": "2002/07/22T16:22:36-2002/07/23T01:21:45"
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    "keywords": [
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        "Antimatter",
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        "Earth Science",
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    "recommended_pages": [],
    "related": [],
    "sources": [],
    "products": [],
    "newer_versions": [],
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    "alternate_versions": []
}