{
    "count": 9,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 4929,
            "url": "https://svs.gsfc.nasa.gov/4929/",
            "result_type": "Visualization",
            "release_date": "2021-08-30T14:00:00-04:00",
            "title": "Comparing Atomic Oxygen Emission Observed by GOLD with Ionospheric Total Electron Content (TEC)",
            "description": "At 23:00UTC on November 19, 2018, we see the maxima of TEC values (red dots) closely aligned with the maxima of OI 135.6nm emission (black dots) || GOLD_TEC_anomalies_inset.00034_print.jpg (1024x576) [121.4 KB] || ",
            "hits": 60
        },
        {
            "id": 4683,
            "url": "https://svs.gsfc.nasa.gov/4683/",
            "result_type": "Visualization",
            "release_date": "2018-10-10T00:00:00-04:00",
            "title": "NASA Scientists see Gravity Waves in Concentric Rings",
            "description": "NASA scientists have tracked gravity waves traveling thousands of miles across our atmosphere in concentric rings. Large storms can create these waves, which grow and spread upward hundreds of miles above Earth's surface. The AIRS instrument on NASA's Aqua satellite detected gravity waves in the troposphere and stratosphere 12 hours before a deadly EF5 tornado in Moore, Oklahoma, in 2013.  On the instrument's next pass 11 hours later, it detected even stronger waves.We pull up 250 miles to the ionosphere, where the waves can be observed by GPS satellites. Here gravity waves are shown in greens and yellows, like ripples in a pond.  The waves and tornado were both produced by a long-lived storm system.Understanding the spread of gravity waves improves global weather forecasting and space weather forecasting.Complete transcript available.This video is also available on our YouTube channel. || GravityWavesBeforeAfterMooreTornado_0740_print.jpg (1024x576) [131.1 KB] || GravityWavesBeforeAfterMooreTornado_0740_searchweb.png (320x180) [102.9 KB] || GravityWavesBeforeAfterMooreTornado_0740_thm.png (80x40) [8.3 KB] || GravityWavesBeforeAfterMooreTornado_0740.tif (1920x1080) [3.2 MB] || GravityWavesMooreOK-SameWordsDifferentOrder.webm (1920x1080) [7.4 MB] || GWfacebook-AIRS-TEC-GOES-4k-audio.mp4 (1920x1080) [76.1 MB] || GravityWavesMooreOK-SameWordsDifferentOrder.mp4 (1920x1080) [117.1 MB] || composite (3849x2160) [0 Item(s)] || GW4k-AIRS-TEC-GOES-4k-audio-youtube.en_US.srt [1.2 KB] || GW4k-AIRS-TEC-GOES-4k-audio-youtube.en_US.vtt [1.2 KB] || GW4k-AIRS-TEC-GOES-4k-audio-youtube.mp4 (3840x2160) [240.0 MB] || GWfacebook-AIRS-TEC-GOES-4k-audio.mp4.hwshow [199 bytes] || ",
            "hits": 155
        },
        {
            "id": 3310,
            "url": "https://svs.gsfc.nasa.gov/3310/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Ionosphere Total Electron Content - April 2001",
            "description": "A view of the ionospheric Total Electron Content (TEC) measured over North America during a storm in April 2001.  Red is high electron counts, blue is low, gray where there is no data.  From the pre-storm state, we see relatively low electron counts.  As the storm intensity increases, so do the number of electrons.  The increase will generate more interference for communications systems, GPS, etc. || ",
            "hits": 41
        },
        {
            "id": 3311,
            "url": "https://svs.gsfc.nasa.gov/3311/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to plasmapause-induced TEC enhancement - April 2001",
            "description": "Space weather events which disturb the plasmapause (displayed here as a green surface enclosing the Earth) can propagate down to the Earth's ionosphere.  There they enhance the ionosphere electron content which can disrupt radio signals from satellites.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 15
        },
        {
            "id": 3312,
            "url": "https://svs.gsfc.nasa.gov/3312/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "The 'Big Picture' View of the Plasmapause and Ionospheric Electron Content - April 2001",
            "description": "This visualization presents a wide-angle overview of the plasmapause-Earth system.  Electron content data is mapped to the sphere of the Earth.  As the space storm progresses, the structure of the plasmapause becomes distorted but is still constrained by the structure of the Earth's dipolar magnetic field. || ",
            "hits": 17
        },
        {
            "id": 3313,
            "url": "https://svs.gsfc.nasa.gov/3313/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Ionosphere Total Electron Content - November 2003",
            "description": "This movie displays plume formation for a space weather event in November 2003.  In this visualization, the observer is fixed between the Sun and the Earth (slightly off the center line for better perspective).  Blue represents low ionospheric electron counts, dark red is high electron counts. || ",
            "hits": 26
        },
        {
            "id": 3314,
            "url": "https://svs.gsfc.nasa.gov/3314/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Time-varying Plasmapause and Electron data - April 2001",
            "description": "This is another view of the plasmapause and electron content data for the April 11, 2001 time frame (similar to ID 3312).  This point of view is shifted slightly to the sunlit side of the Earth to present a better view of the plume formation. || ",
            "hits": 21
        },
        {
            "id": 3316,
            "url": "https://svs.gsfc.nasa.gov/3316/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to Plasmapause-Induced TEC Enhancement - April 2001 (Version 2)",
            "description": "Space weather events which disturb the plasmapause (displayed here as a green surface enclosing the Earth) can propagate down to the Earth's ionosphere. There they enhance the ionosphere electron content which can disrupt radio signals from satellites. This movie is a variation on animation ID 3311 with slightly different camera motions. NOTE: This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth. Technically, this is inaccurate. Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up. More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 22
        },
        {
            "id": 3317,
            "url": "https://svs.gsfc.nasa.gov/3317/",
            "result_type": "Visualization",
            "release_date": "2005-12-05T00:00:00-05:00",
            "title": "Zoom-in to plasmapause-induced TEC enhancement - April 2001",
            "description": "Space weather events which disturb the plasmapause can propagate down to the Earth's ionosphere.  There they enhance the ionosphere electron content which can disrupt radio signals from satellites.  This is a re-timed version of ID 3311.  This version is designed to play synchronously with ID 3310, ID 3312, and ID 3314.NOTE:  This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth.  Technically, this is inaccurate.  Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up.  More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?. || ",
            "hits": 13
        }
    ]
}