{
    "count": 6,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 10755,
            "url": "https://svs.gsfc.nasa.gov/10755/",
            "result_type": "Produced Video",
            "release_date": "2011-04-08T00:00:00-04:00",
            "title": "LAMP: Peering Into the Lunar Dark",
            "description": "The Lyman-Alpha Mapping Project (LAMP) is an instrument on NASA's Lunar Reconnaissance Orbiter mission to map and study the Moon. LAMP is a spectrograph that images the ultraviolet region of the spectrum. Utilizing the faint glow of stars and other light reflected off the lunar surface, LAMP can see inside the darkest areas of the Moon to search for water ice and other valuable resources. || ",
            "hits": 67
        },
        {
            "id": 3785,
            "url": "https://svs.gsfc.nasa.gov/3785/",
            "result_type": "Visualization",
            "release_date": "2010-10-21T13:55:00-04:00",
            "title": "LAMP Observes the LCROSS Impact",
            "description": "A two-ton Atlas Centaur rocket body, part of the Lunar Crater Observation and Sensing Satellite (LCROSS), struck the floor of Cabeus crater, near the south pole of the moon, at 11:31 UT on October 9, 2009. The purpose of the crash was to create a plume of debris that could be examined for the presence of water and other chemicals in the lunar regolith.The Lyman-Alpha Mapping Project (LAMP) instrument aboard Lunar Reconnaissance Orbiter (LRO) observed the tenuous vapor cloud created by the LCROSS impact. LAMP is LRO's \"night vision.\" Most of the time, it uses the ultraviolet light in starlight to peer into deep shadows on the moon's surface. For the LCROSS impact, LAMP was pointed just above the lunar horizon to watch for the arrival of a rapidly expanding cloud of vaporized debris from the crash.In this animation, the viewer looks down the LAMP boresight and through its narrow window. The LAMP sensor lights up as the leading edge of the expanding vapor cloud passes through its field of view. What's shown here is actually the difference between the data recorded after the LCROSS impact and that recorded on LRO's previous orbit. See this entry for more about the process of subtracting the background to enhance the LAMP signal. || ",
            "hits": 44
        },
        {
            "id": 10683,
            "url": "https://svs.gsfc.nasa.gov/10683/",
            "result_type": "Produced Video",
            "release_date": "2010-10-21T13:55:00-04:00",
            "title": "LAMP Observes the LCROSS Impact - WIth Overlays",
            "description": "This video shows LAMP's view of the LCROSS plume. The line in the center of the screen is the LAMP viewport scanning across the horizon, passing through the plume, and moving on. || lamp_lcross_youtube_hq.14_print.jpg (1280x720) [89.6 KB] || lamp_lcross_ipod_lg_web.png (320x180) [163.3 KB] || lamp_lcross_ipod_lg_thm.png (80x40) [11.9 KB] || lamp_lcross_appletv.m4v (960x540) [13.1 MB] || lamp_lcross_prores.mov (1280x720) [194.7 MB] || lamp_lcross_wmv.wmv (1280x720) [11.5 MB] || lamp_lcross_youtube_hq.mov (1280x720) [16.7 MB] || lamp_lcross_appletv.webmhd.webm (960x540) [3.9 MB] || lamp_lcross_ipod_lg.m4v (640x360) [5.7 MB] || lamp_lcross_nasaportal.mov (640x360) [8.6 MB] || lamp_lcross_nasacast.mp4 (320x240) [2.4 MB] || lamp_lcross_svs.mpg (512x288) [4.3 MB] || ",
            "hits": 20
        },
        {
            "id": 10685,
            "url": "https://svs.gsfc.nasa.gov/10685/",
            "result_type": "Produced Video",
            "release_date": "2010-10-21T13:55:00-04:00",
            "title": "LCROSS Plume Model with LAMP viewport",
            "description": "The movie shows the simulated evolution of the vapor cloud of molecular hydrogen from the impact of LCROSS into the southern polar region of the Moon.  The movie is displayed in the frame of reference of the LAMP instrument, with its field of view shown by the vertical red line at [0,0].  The LCROSS impact site moves to the left as time goes on in this reference frame.  It shows how the timing of the signal LAMP detects is a combination of the expansion of the cloud and the motion of LRO past the impact site.  It also shows how the signal observed by LAMP is from only a small portion of the entire cloud, emphasizing the need to use modeling to relate the observations to the overall release. || ",
            "hits": 34
        },
        {
            "id": 3165,
            "url": "https://svs.gsfc.nasa.gov/3165/",
            "result_type": "Visualization",
            "release_date": "2005-09-30T12:00:00-04:00",
            "title": "X-ray Images of the North Polar Region from the Chandra HRC-I Instrument",
            "description": "Here are X-rays images (shown on the same brightness scale) of the north polar region obtained by Chandra HRC-I on different days, showing large variability in soft (0.1-10.0 keV) X-ray emissions from Earth s aurora. Note that the images are not snap shots, but are ~20-min scans of the northern auroral region in the HRC-I field-of-view. The brightness scale in Rayleighs (R) assumes an average effective area of 40 cm2. The day-night terminator at an altitude of 0 km is displayed with lighting. The day-night terminator at an altitude of 100 km is shown by the blue line. || ",
            "hits": 29
        },
        {
            "id": 3170,
            "url": "https://svs.gsfc.nasa.gov/3170/",
            "result_type": "Visualization",
            "release_date": "2005-06-01T12:00:00-04:00",
            "title": "X-Ray Images of the North Polar Region (WMS)",
            "description": "Here are X-rays images (shown on the same brightness scale) of the north polar region obtained by Chandra HRC-I on different days, showing large variability in soft (0.1-10.0 keV) X-ray emissions from Earth s aurora. Note that the images are not snap shots, but are approximately 20-min scans of the northern auroral region in the HRC-I field-of-view. The brightness scale in Rayleighs (R) assumes an average effective area of 40 cm2. The day-night terminator at an altitude of 0 km is displayed with lighting. The day-night terminator at an altitude of 100 km is shown by the blue line. || ",
            "hits": 14
        }
    ]
}