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    "results": [
        {
            "id": 11204,
            "url": "https://svs.gsfc.nasa.gov/11204/",
            "result_type": "Produced Video",
            "release_date": "2013-03-14T14:30:00-04:00",
            "title": "Jupiter's Hot Spots",
            "description": "Jupiter's bright Equatorial Zone swirls with dark patches, dubbed \"hot spots\" for their infrared glow. These holes in the ammonia clouds at the top of the atmosphere allow a glimpse into Jupiter's darker, hotter layers below. In 1995 NASA's Galileo spacecraft dropped a probe directly into a hot spot, taking the first and only in situ measurements of Jupiter's atmosphere. Now, movies recorded by NASA's Cassini spacecraft reveal that hot spots are not just local weather phenomena, but are in fact linked to much larger-scale atmospheric structures called Rossby waves. || ",
            "hits": 71
        },
        {
            "id": 10927,
            "url": "https://svs.gsfc.nasa.gov/10927/",
            "result_type": "Produced Video",
            "release_date": "2012-03-13T13:00:00-04:00",
            "title": "RATTLING JET STREAM ON JUPITER",
            "description": "New movies of Jupiter are the first to catch an invisible wave shaking up one of the giant planet's jet streams, an interaction that also takes place in Earth's atmosphere and influences the weather.For complete transcript, click here. || G2012-013_Jupiter_Weather_portal.00752_print.jpg (1024x576) [69.0 KB] || G2012-013_Jupiter_Weather_portal_web.png (320x180) [190.6 KB] || G2012-013_Jupiter_Weather_portal_thm.png (80x40) [16.5 KB] || G2012-013_Jupiter_Weather.wmv (1280x720) [62.8 MB] || G2012-013_Jupiter_Weather_youtube_hq.mov (1280x720) [70.4 MB] || G2012-013_Jupiter_Weather_appletv.m4v (960x540) [56.5 MB] || G2012-013_Jupiter_Weather_appletv.webmhd.webm (960x540) [27.4 MB] || G2012-013_Jupiter_Weather_portal.mov (640x360) [53.2 MB] || G2012-013_Jupiter_Weather_ipod_lg.m4v (640x360) [22.3 MB] || GSFC_20120313_Jupiter_m10927_Weather.en_US.vtt [2.7 KB] || G2012-013_Jupiter_Weather_prores.mov (1280x720) [1.9 GB] || G2012-013_Jupiter_Weather_ipod_sm.mp4 (320x240) [11.7 MB] || ",
            "hits": 76
        },
        {
            "id": 3604,
            "url": "https://svs.gsfc.nasa.gov/3604/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Pull out from Jupiter Showing Moon Orbits",
            "description": "NOTE: The orbital plane of the moons in these visualizations is incorrect.  The Galilean moons should be aligned to Jupiter's equator.This visualization shows jupiter and 63 of its moons. We start close in to Jupiter showing relativly fast moving inner moons that are generally in the same orbital plane including the so called 'Galilean moons': Europa, Io, Ganymede, and Callisto. Other inner moons are: Amalthea, Thebe, Adrastea, and Metis. These inner moons orbit Jupiter as fast as about every 7 hours to about every 17 days. These moons are also relativly close to Jupiter: from around 100 thousand to a couple of million kilometers away.We pull back revealing many smaller moons much farther away (tens of millions of kilometers) in much longer orbits (up to several years). Time speeds up to show the motion of these moons in irregular orbits. The following outer moons are displayed: Himalia, Elara, Pasiphae, Sinope, Lysithea, Carme, Ananke, Leda, Callirrhoe, Themisto, Megaclite, Taygete, Chaldene, Harpalyke, Kalyke, Iocaste, Erinome, Isonoe, Praxidike, Autonoe, Thyone, Hermippe, Aitne, Eurydome, Euanthe, Euporie, Orthosie, Sponde, Kale, Pasithee, Hegemone, Mneme, Aoede, Thelxinoe, Arche, Kallichore, Helike, Carpo, Eukelade, Cyllene, Kore, S/2000 J11, S/2003 J2, S/2003 J3, S/2003 J4, S/2003 J5, S/2003 J9 ,S/2003 J10, S/2003 J12, S/2003 J15, S/2003 J16, S/2003 J17, S/2003 J18, S/2003 J19, and S/2003 J23.This visualization was created in support of the Science On a Sphere film called \"Largest\" which is about Jupiter. The visualziation was choreographed to fit into \"Largest\" as a layer that is Intended to be composited with other layers including a background starfield. Three copies of this shot are arranged with orbits that fade on as we pull back in order to facilitate a seamless inset (without orbits falling off the boarder) on the Science On a Sphere composited frames. || ",
            "hits": 187
        },
        {
            "id": 3607,
            "url": "https://svs.gsfc.nasa.gov/3607/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Shoemaker-Levy 9 Hitting Jupiter with Orbit Trails",
            "description": "This visualziation shows the major fragments of comet Showmaker-Levy 9 colliding with Jupiter. The orbits are driven using ephemeris data. The impacts occurred over a series of about six Earth days which is why Jupiter (which rotates about once every Earth 10 hours) appears to be rotating so fast in this visualization; time is is depicted at about 7 hours per second of animation.The comet fragments shown are: \"a\", \"b\", \"c\", \"d\", \"e\", \"f\", \"g\", \"h\", \"k\", \"l\", \"n\", \"p\", \"p\", \"q\", \"q\", \"r\", \"s\", \"t\", \"u\", \"v\", and \"w\". Several letters were skipped (due to lack of ephemeris) and 2 letters \"p\" and \"q\" appear twice; these are also known as \"p1\", \"p2\", \"q1\", and \"q2\".This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. The visualziation was choreographed to fit into \"LARGEST\" as a layer that is intended to be composited with other layers including a match-rendered background star field. Three copies of this shot are arranged in order to facilitate a seamless inset on the Science On a Sphere composited frames. || ",
            "hits": 88
        },
        {
            "id": 3609,
            "url": "https://svs.gsfc.nasa.gov/3609/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Rotation Period Comparison Between Earth and Jupiter",
            "description": "This animation illustrates the difference in the rotational period between the Earth and Jupiter. Earth rotates once in 24 hours; whereas, Jupiter rotates more quickly, taking only about 10 hours. This means that Jupiter rotates about 2 1/2 times faster than the Earth. However, Jupiter is about 11 times bigger than the Earth, so matter near the outer 'surface' of Jupiter is travelling much faster (about 30 times faster) than matter at the outer 'surface' of Earth.This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. The visualziation was choreographed to fit into \"LARGEST\" as a layers intended to be composited. The 2 animations of Earth and Jupiter are match rendered so that if played back at the same frame rate (say 30 frames per second), the relative rotational speed differences will be accurate. An example composite is provided for reference; in this composite, only a portion of Jupiter is shown so that the relative sizes of the planets are also represented. The composited shot is designed to be repeated around the scienice on a sphere display several times. || ",
            "hits": 906
        },
        {
            "id": 3610,
            "url": "https://svs.gsfc.nasa.gov/3610/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Jupiter Cloud Sequence from Cassini",
            "description": "When the Cassini mission flew by the planet Jupiter in late 2000, a sequence of full disk images were taken of the planet. Assembled with proper spatial and temporal registration, the sequence could produce fourteen distinct images suitable for wrapping around a sphere.But the time steps between images were large and exhibited significant jumping. The solution was to create additional images between the existing set by interpolation. But simple interpolation would not work due to significant changes between the images.To solve this, we interpolated between the images using the velocity vector field of the cloud images. The velocity vector field was computed by performing a 2-dimensional cross-correlation (Wikipedia: Cross-correlation) between the images. This velocity field was checked against Jupiter velocity profiles from the scientific literature and agreement was excellent. With the addition of a simple vortex flow at the location of the Great Red Spot, the interpolation process was used to generate intermediate images, increasing the total number of images from 14 to 220 and resulting in a smoother animation.  The elapsed time between each interpolated frame corresponds to about 1 hour.  More info on the image sequence is available at Jupiter Mosaics and Movies - Rings, Satellites, AtmosphereIMPORTANT NOTE: These images are for visualization purposes only. They are not suitable for scientific analysis. || ",
            "hits": 104
        },
        {
            "id": 3616,
            "url": "https://svs.gsfc.nasa.gov/3616/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Galilean moon orbits from Callisto into Jupiter",
            "description": "NOTE: The orbital plane of the moons in these visualizations is incorrect.  The Galilean moons should be aligned to Jupiter's equator.This visualization starts close in on Jupiter's moon Callisto. We pull back and start moving in towards Jupiter, passing Ganymede on the way. Io and Europa are off in the distance behind Jupiter as we push in and Jupiter fills the screen.This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. The visualziation was choreographed to fit into \"LARGEST\" as a layers to be composited in post-production. There are five separate layers that were designed to give the editors flexibility in reagrds to when particular objects faded in/out. There are three layers that are identical except that Callisto and Jupiter are offset 0, 120, and 240 degrees; this is for a zoom out/in effect that transitions quickly to fully wrapped images of Callisto/Jupiter. A background layer contains only Io and Europa. Finally a layer with Jupiter as a gray ball in included for use in masking. All of the layers are intended to be composited over a starfield. Since there is very little camera motion other than a push in, a moving starfield is not provided for this shot.A composite movie is included to illustrate how the layers were intended to be used. || ",
            "hits": 101
        },
        {
            "id": 3617,
            "url": "https://svs.gsfc.nasa.gov/3617/",
            "result_type": "Visualization",
            "release_date": "2009-09-21T00:00:00-04:00",
            "title": "Inner moons of Jupiter Push In to Europa",
            "description": "This visualization starts showing the orbits of Jupiter's inner moons (Europa, Io, Ganymede, Callisto, Amalthea, Thebe, Adrastea, and Metis). As the orbits procede we begin to zero in on Europa. Other moons and orbits fade away as we push in to Europa filling the screen.This visualization was created in support of the Science On a Sphere film called \"LARGEST\" which is about Jupiter. Mulitple layer offset 120 degrees from each other are intended to overlay the orbits. A Europa label is provided so that it can be faded out in post production. A separate layer for Jupiter is also provided so that the other moons and orbit trails can also be faded out, leaving only Jupiter. || ",
            "hits": 124
        },
        {
            "id": 10477,
            "url": "https://svs.gsfc.nasa.gov/10477/",
            "result_type": "Produced Video",
            "release_date": "2009-09-04T00:00:00-04:00",
            "title": "LARGEST: A Spherical Movie About Jupiter",
            "description": "NASA's home for spherical films on Magic Planet. Download the Magic Planet-ready movie file here.Three hundred and eighty million miles from Earth, the solar system's largest planet spins like a sizzling top in the night, massive and powerful beyond all comparison short of the sun itself. It's therefore only fitting—and certainly about time—that the fifth planet receive its proper cinematic due, set naturally on the most appropriate cinematic platform. With the movie LARGEST, Jupiter comes to Science On a Sphere.LARGEST examines the gas giant like a work of art, like a destination of celestial wonder. Starting with the basics, the movie examines the gross anatomy of the immense planet. From swirling winds to astounding rotational velocity to unimaginable size, Jupiter demands nothing less than a list of superlatives. But where general description sets the stage, LARGEST parts the curtains on humanity's experience with the fifth planet. The movie takes us on a journey to this immense sphere via dramatic fly-bys with some of the most astounding robotic probes ever designed. Then, with NASA instruments trained on the striped behemoth, the drama really begins.NASA released LARGEST on September 15, 2009. It is one in a series of spherical movies created entirely by staff at the NASA Goddard Space Flight Center. But while the process to create a fully spherical movie is something of an in-house Goddard creation, the Science On a Sphere projection system itself is an invention of the space agency's sibling NOAA.This film has been prepared exclusively for playback on spherical projections systems. It will not play properly on a traditional computer or television screen. If you are interested in downloading the complete final movie file for spherical playback, please visit ftp://public.sos.noaa.gov/extras/.For more information about the movie itself, visit the main website at www.nasa.gov/largest. || ",
            "hits": 39
        }
    ]
}