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    "results": [
        {
            "id": 3595,
            "url": "https://svs.gsfc.nasa.gov/3595/",
            "result_type": "Visualization",
            "release_date": "2009-07-27T00:00:00-04:00",
            "title": "Sentinels of the Heliosphere",
            "description": "Heliophysics is a term to describe the study of the Sun, its atmosphere or the heliosphere, and the planets within it as a system. As a result, it encompasses the study of planetary atmospheres and their magnetic environment, or magnetospheres. These environments are important in the study of space weather.As a society dependent on technology, both in everyday life, and as part of our economic growth, space weather becomes increasingly important. Changes in space weather, either by solar events or geomagnetic events, can disrupt and even damage power grids and satellite communications. Space weather events can also generate x-rays and gamma-rays, as well as particle radiations, that can jeopardize the lives of astronauts living and working in space.This visualization tours the regions of near-Earth orbit; the Earth's magnetosphere, sometimes called geospace; the region between the Earth and the Sun; and finally out beyond Pluto, where Voyager 1 and 2 are exploring the boundary between the Sun and the rest of our Milky Way galaxy. Along the way, we see these regions patrolled by a fleet of satellites that make up NASA's Heliophysics Observatory Telescopes. Many of these spacecraft do not take images in the conventional sense but record fields, particle energies and fluxes in situ. Many of these missions are operated in conjunction with international partners, such as the European Space Agency (ESA) and the Japanese Space Agency (JAXA).The Earth and distances are to scale. Larger objects are used to represent the satellites and other planets for clarity.Here are the spacecraft featured in this movie:Near-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTRACE: Observes the Sun in visible and ultraviolet wavelengths. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. AIM: Images and measures noctilucent clouds. SVS pageGeospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of five satellites to study how magnetospheric instabilities produce substorms. SVS pageL1 Fleet: The L1 point is a Lagrange Point, a point between the Earth and the Sun where the gravitational pull is approximately equal. Spacecraft can orbit this location for continuous coverage of the Sun.SOHO: Studies the Sun with cameras and a multitude of other instruments. SVS pageACE: Measures the composition and characteristics of the solar wind. Wind: Measures particle flows and fields in the solar wind. Heliospheric FleetSTEREO-A and B: These two satellites observe the Sun, with imagers and particle detectors, off the Earth-Sun line, providing a 3-D view of solar activity. SVS pageHeliopause FleetVoyager 1 and 2: These spacecraft conducted the original 'Planetary Grand Tour' of the solar system in the 1970s and 1980s. They have now travelled further than any human-built spacecraft and are still returning measurements of the interplanetary medium. SVS pageThis enhanced, narrated visualization was shown at the SIGGRAPH 2009 Computer Animation Festival in New Orleans, LA in August 2009; an eariler version created for AGU was called NASA's Heliophysics Observatories Study the Sun and Geospace. || ",
            "hits": 99
        },
        {
            "id": 10421,
            "url": "https://svs.gsfc.nasa.gov/10421/",
            "result_type": "Produced Video",
            "release_date": "2009-04-07T00:00:00-04:00",
            "title": "SOHO/TRACE Intro",
            "description": "On April 3, 2009, countries from around the world participated in the '100 Hours of Astronomy' webcast to celebrate the International Year of Astronomy. This movie was used to introduce the SOHO/TRACE segment. Alex Young and Dawn Meyers, NASA scientists, describe how both SOHO and TRACE view the sun in their own unique way. || ",
            "hits": 42
        },
        {
            "id": 3570,
            "url": "https://svs.gsfc.nasa.gov/3570/",
            "result_type": "Visualization",
            "release_date": "2008-12-15T00:00:00-05:00",
            "title": "NASA's Heliophysics Observatories Study the Sun and Geospace",
            "description": "Heliophysics is a term to describe the study of the Sun, its atmosphere or the heliosphere, and the planets within it as a system. As a result, it encompasses the study of planetary atmospheres and their magnetic environment, or magnetospheres. These environments are important in the study of space weather.As a society dependent on technology, both in everyday life, and as part of our economic growth, space weather becomes increasingly important. Changes in space weather, either by solar events or geomagnetic events, can disrupt and even damage power grids and satellite communications. Space weather events can also generate x-rays and gamma-rays, as well as particle radiations, that can jeopardize the lives of astronauts living and working in space.This visualization tours the regions of near-Earth orbit; the Earth's magnetosphere, sometimes called geospace; the region between the Earth and the Sun; and finally out beyond Pluto, where Voyager 1 and 2 are exploring the boundary between the Sun and the rest of our Milky Way galaxy. Along the way, we see these regions patrolled by a fleet of satellites that make up NASA's Heliophysics Observatory Telescopes. Many of these spacecraft do not take images in the conventional sense but record fields, particle energies and fluxes in situ. Many of these missions are operated in conjunction with international partners, such as the European Space Agency (ESA) and the Japanese Space Agency (JAXA).The Earth and distances are to scale. Larger objects are used to represent the satellites and other planets for clarity.Here are the spacecraft featured in this movie:Near-Earth Fleet:Hinode: Observes the Sun in multiple wavelengths up to x-rays. SVS pageRHESSI : Observes the Sun in x-rays and gamma-rays. SVS pageTRACE: Observes the Sun in visible and ultraviolet wavelengths. SVS pageTIMED: Studies the upper layers (40-110 miles up) of the Earth's atmosphere.FAST: Measures particles and fields in regions where aurora form.CINDI: Measures interactions of neutral and charged particles in the ionosphere. AIM: Images and measures noctilucent clouds. SVS pageGeospace Fleet:Geotail: Conducts measurements of electrons and ions in the Earth's magnetotail. Cluster: This is a group of four satellites which fly in formation to measure how particles and fields in the magnetosphere vary in space and time. SVS pageTHEMIS: This is a fleet of five satellites to study how magnetospheric instabilities produce substorms. SVS pageL1 Fleet: The L1 point is a Lagrange Point between the Sun and the Earth. Spacecraft can orbit this location for continuous coverage of the Sun.SOHO: Studies the Sun with cameras and a multitude of other instruments. SVS pageACE: Measures the composition and characteristics of the solar wind. Wind: Measures particle flows and fields in the solar wind. Heliospheric FleetSTEREO-A and B: These two satellites observe the Sun, with imagers and particle detectors, off the Earth-Sun line, providing a 3-D view of solar activity. SVS pageHeliopause FleetVoyager 1 and 2: These spacecraft conducted the original 'Planetary Grand Tour' of the solar system in the 1970s and 1980s. They have now travelled further than any human-built spacecraft and are still returning measurements of the interplanetary medium. SVS pageA refined and narrated version of this visualization, Sentinels of the Heliosphere, is now available. || ",
            "hits": 104
        },
        {
            "id": 3385,
            "url": "https://svs.gsfc.nasa.gov/3385/",
            "result_type": "Visualization",
            "release_date": "2006-11-08T00:00:00-05:00",
            "title": "Mercury Transit from TRACE (1600 Angstrom ultraviolet)",
            "description": "This is a view of the planet Mercury (a black dot) as seen by TRACE through the 1600 angstrom ultraviolet filter. Because the TRACE field-of-view is much smaller than the solar disk, the spacecraft is repointed three times during the transit (creating the position jumps of the movie).  This movie was generated from telemetry which has undergone a minimum of processing (to deliver quickly for the media) so data dropouts and other quick-processing artifacts may be visible. Special thanks to Dawn Myers of the TRACE project for this effort. || ",
            "hits": 28
        },
        {
            "id": 2921,
            "url": "https://svs.gsfc.nasa.gov/2921/",
            "result_type": "Visualization",
            "release_date": "2005-03-08T12:00:00-05:00",
            "title": "Solar Tsunamis",
            "description": "Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event.  The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. || ",
            "hits": 33
        },
        {
            "id": 2922,
            "url": "https://svs.gsfc.nasa.gov/2922/",
            "result_type": "Visualization",
            "release_date": "2005-03-08T12:00:00-05:00",
            "title": "Solar Tsunamis - View with a Spin",
            "description": "Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event.  The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below.  This view rotates on the push-in to keep the region of the flare event visible (to the left in the final frame). || ",
            "hits": 10
        },
        {
            "id": 2750,
            "url": "https://svs.gsfc.nasa.gov/2750/",
            "result_type": "Visualization",
            "release_date": "2003-09-02T12:00:00-04:00",
            "title": "RHESSI Observes 2.2 MeV Line Emission from a Solar Flare",
            "description": "The solar flare at Active Region 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. || ",
            "hits": 32
        },
        {
            "id": 2764,
            "url": "https://svs.gsfc.nasa.gov/2764/",
            "result_type": "Visualization",
            "release_date": "2003-07-09T12:00:00-04:00",
            "title": "High Resolution Solar Views From VAULT",
            "description": "This movie illustrates the VAULT camera pointings in relation to the rest of the Sun and views from other instruments. || ",
            "hits": 24
        },
        {
            "id": 2765,
            "url": "https://svs.gsfc.nasa.gov/2765/",
            "result_type": "Visualization",
            "release_date": "2003-07-09T12:00:00-04:00",
            "title": "Hi-resolution Solar Views from VAULT: Active Region",
            "description": "This movie presents the VAULT imagery in the context of simultaneous multi-mission observations.  We zoom-in to a subset of the image which focuses on an active solar region which shows plumes of hot gases rising above the solar surface. || ",
            "hits": 20
        },
        {
            "id": 2735,
            "url": "https://svs.gsfc.nasa.gov/2735/",
            "result_type": "Visualization",
            "release_date": "2003-05-07T12:00:00-04:00",
            "title": "Mercury Transit of the Sun",
            "description": "The planet Mercury is visible passing between the Sun and the TRACE spacecraft.  Data collected on May 7, 2003, from 04:32:04 to 08:08:57. || a002735.00005_print.png (720x480) [358.5 KB] || a002735.00240_print.png (720x480) [528.2 KB] || MercuryTransit_640x480_pre.jpg (320x240) [5.5 KB] || MercuryTransit_320x240_pre.jpg (320x240) [5.3 KB] || a002735.webmhd.webm (960x540) [4.3 MB] || MercuryTransit_640x480.mpg (640x480) [7.7 MB] || a002735.m2v (720x480) [10.4 MB] || 720x480_4x3_30p (720x486) [16.0 KB] || a002735.dv (720x480) [54.9 MB] || a002735.mp4 (640x480) [2.5 MB] || MercuryTransit_320x240.mpg (320x240) [2.0 MB] || ",
            "hits": 32
        },
        {
            "id": 2717,
            "url": "https://svs.gsfc.nasa.gov/2717/",
            "result_type": "Visualization",
            "release_date": "2003-04-11T12:00:00-04:00",
            "title": "Closeup of Solar 'Tadpoles' with time tags",
            "description": "Here is a close-up view of dark 'tentacles' or 'tadpoles' moving towards the solar surface in this solar flare of April 21, 2002 seen by TRACE.  One theory proposed in this press release is that they are due to voids created by magnetic reconnection in the flare.  This version of the visualization displays the instrument clock time tags. || ",
            "hits": 13
        },
        {
            "id": 2718,
            "url": "https://svs.gsfc.nasa.gov/2718/",
            "result_type": "Visualization",
            "release_date": "2003-04-11T12:00:00-04:00",
            "title": "Closeup of Solar 'Tadpoles' without time tags",
            "description": "Here is a close-up view of dark 'tentacles' or 'tadpoles' moving towards the solar surface in this solar flare of April 21, 2002 seen by TRACE.  One theory proposed in this press release is that they are due to voids created by magnetic reconnection in the flare.  This version of the visualization does not display the instrument clock time tags. || ",
            "hits": 5
        },
        {
            "id": 2464,
            "url": "https://svs.gsfc.nasa.gov/2464/",
            "result_type": "Visualization",
            "release_date": "2002-06-10T12:00:00-04:00",
            "title": "Another View of AR9906 from TRACE",
            "description": "Another view of the flare over AR9906 on April 21, 2002.  This version represents the full resolution of the TRACE data.  This visualization represents eight hours of observing time. || ",
            "hits": 7
        },
        {
            "id": 2458,
            "url": "https://svs.gsfc.nasa.gov/2458/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - Time Tagged",
            "description": "Close-up view of the solar active region AR9906 on April 21, 2002 with TRACE and RHESSI data. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 13
        },
        {
            "id": 2459,
            "url": "https://svs.gsfc.nasa.gov/2459/",
            "result_type": "Visualization",
            "release_date": "2002-06-05T12:00:00-04:00",
            "title": "RHESSI Observes the Flare over AR9906 - No time tags",
            "description": "Close-up view of the solar active region AR9906 on April 21, 2002 with TRACE data and RHESSI. RHESSI observes x-rays from this flare. The red contours represent the 12-25 keV photon energy range and the blue contours represent 50-100 keV. || ",
            "hits": 10
        },
        {
            "id": 2446,
            "url": "https://svs.gsfc.nasa.gov/2446/",
            "result_type": "Visualization",
            "release_date": "2002-05-29T12:00:00-04:00",
            "title": "TRACE Observes the X-ray Flare Over AR9906",
            "description": "The TRACE spacecraft observes an X-ray flare over solar active region AR9906, April 21, 2002. || Movie of the flaring of active region AR9906 || a002446.00070_print.png (720x480) [447.5 KB] || xflare-ar9906_pre.jpg (320x240) [5.3 KB] || a002446.webmhd.webm (960x540) [2.1 MB] || a002446.dv (720x480) [44.6 MB] || xflare-ar9906.mpg (320x240) [1.7 MB] || ",
            "hits": 15
        },
        {
            "id": 2425,
            "url": "https://svs.gsfc.nasa.gov/2425/",
            "result_type": "Visualization",
            "release_date": "2002-05-15T12:00:00-04:00",
            "title": "TRACE Observes Flows over Active Regions (Slow Play)",
            "description": "Zoom in on the Sun to show the outflow region. || a002425.00100_print.png (720x480) [478.8 KB] || a002425_pre.jpg (320x240) [9.0 KB] || a002425.webmhd.webm (960x540) [4.3 MB] || a002425.dv (720x480) [150.9 MB] || a002425.mpg (320x240) [2.6 MB] || Full-disk view of the Sun with SOHO-EIT around the time of the TRACE observations. || trace0001.jpg (2560x1920) [386.8 KB] || trace0001_web.jpg (320x240) [9.3 KB] || trace0001.tif (2560x1920) [2.7 MB] || ",
            "hits": 11
        },
        {
            "id": 2426,
            "url": "https://svs.gsfc.nasa.gov/2426/",
            "result_type": "Visualization",
            "release_date": "2002-05-15T12:00:00-04:00",
            "title": "TRACE Observes Flows over Active Regions (Fast Play)",
            "description": "Zoom in on the Sun to show the outflow region. || a002426.00100_print.png (720x480) [465.6 KB] || a002426_pre.jpg (320x240) [9.0 KB] || a002426.webmhd.webm (960x540) [3.1 MB] || a002426.dv (720x480) [89.3 MB] || a002426.mpg (320x240) [1.8 MB] || Full-disk view of the Sun with SOHO-EIT around the time of the TRACE observations. || tracefast0001.jpg (2560x1920) [386.8 KB] || tracefast0001_web.jpg (320x240) [9.3 KB] || tracefast0001.tif (2560x1920) [2.7 MB] || ",
            "hits": 14
        },
        {
            "id": 1168,
            "url": "https://svs.gsfc.nasa.gov/1168/",
            "result_type": "Visualization",
            "release_date": "2000-06-13T12:00:00-04:00",
            "title": "'Bastille Day' Flare Animation",
            "description": "Fly-in of TRACE full sun image to the flare location.  Fade to a model of the field lines with a magnetogram of the solar surface.  Pull back out to display a movie of  flare images.  This version uses lens flares to illustrate matter motion along the field lines. || ",
            "hits": 13
        },
        {
            "id": 1169,
            "url": "https://svs.gsfc.nasa.gov/1169/",
            "result_type": "Visualization",
            "release_date": "2000-06-13T12:00:00-04:00",
            "title": "Bastille Day Flare Without Matter Motion",
            "description": "Fly-in of TRACE full sun image to the flare location. Fade to a model of the field lines with a magnetogram of the solar surface. Pull back out to display a movie of flare images. This version does not show the matter motion along the field lines. || ",
            "hits": 13
        },
        {
            "id": 689,
            "url": "https://svs.gsfc.nasa.gov/689/",
            "result_type": "Visualization",
            "release_date": "1999-07-14T12:00:00-04:00",
            "title": "TRACE: Viewing a Coronal Loop with a Diagram of the Earth for Scale.",
            "description": "Zooming into the sun to show an animation of the Bastille Day solar flare from TRACE imagery || a000689.00010_print.png (720x480) [443.9 KB] || TRACE_pre.jpg (320x240) [6.2 KB] || a000689_pre.jpg (320x242) [6.3 KB] || a000689.webmhd.webm (960x540) [3.6 MB] || a000689.dv (720x480) [54.9 MB] || a000689.mp4 (640x480) [4.6 MB] || TRACE.mov (320x240) [934.9 KB] || a000689.mpg (352x240) [3.0 MB] || ",
            "hits": 50
        },
        {
            "id": 690,
            "url": "https://svs.gsfc.nasa.gov/690/",
            "result_type": "Visualization",
            "release_date": "1999-07-14T12:00:00-04:00",
            "title": "TRACE: Viewing a Coronal Loop",
            "description": "Zooming into the sun to show an animation of the Bastille Day solar flare from TRACE imagery || a000690.00010_print.png (720x480) [439.2 KB] || a000690_pre.jpg (320x242) [6.3 KB] || a000690.webmhd.webm (960x540) [3.6 MB] || a000690.dv (720x480) [51.5 MB] || a000690.mp4 (640x480) [4.5 MB] || a000690.mpg (352x240) [3.1 MB] || ",
            "hits": 48
        },
        {
            "id": 691,
            "url": "https://svs.gsfc.nasa.gov/691/",
            "result_type": "Visualization",
            "release_date": "1999-07-14T12:00:00-04:00",
            "title": "TRACE: A Coronal Loop with a Co-temporal Yohkoh Soft X-ray Image Overlaid",
            "description": "An image of a coronal loop from TRACE, with a co-temporal soft x-ray image from YOKOH overlaid || a000691.00010_print.png (720x480) [457.8 KB] || a000691_thm.png (80x40) [6.3 KB] || a000691_pre.jpg (320x238) [7.7 KB] || a000691_pre_searchweb.jpg (320x180) [56.6 KB] || a000691.webmhd.webm (960x540) [434.6 KB] || a000691.dv (720x480) [24.0 MB] || a000691.mp4 (640x480) [2.0 MB] || a000691.mpg (352x240) [1.5 MB] || ",
            "hits": 36
        },
        {
            "id": 692,
            "url": "https://svs.gsfc.nasa.gov/692/",
            "result_type": "Visualization",
            "release_date": "1999-07-14T12:00:00-04:00",
            "title": "TRACE Still",
            "description": "Yellow Box around a MOSS patch shown magnified by a factor of about 1.6 in the lower right corner. || A TRACE image showing a MOSS patch outlined in yellow and magnified. || a000692_still.jpg (720x528) [78.7 KB] || a000692_pre.jpg (320x238) [7.7 KB] || a000692_thm.png (80x40) [6.0 KB] || a000692_pre_searchweb.jpg (320x180) [54.8 KB] || ",
            "hits": 43
        },
        {
            "id": 693,
            "url": "https://svs.gsfc.nasa.gov/693/",
            "result_type": "Visualization",
            "release_date": "1999-07-14T12:00:00-04:00",
            "title": "TRACE: Shot of MOSS at the Limb",
            "description": "Shot of MOSS at the limb showing the thin layer effect as well as many small and one large dark chromospheric jets projecting in front || a000693_still.jpg (720x528) [53.1 KB] || a000693_pre.jpg (320x238) [4.2 KB] || a000693_thm.png (80x40) [3.0 KB] || a000693_pre_searchweb.jpg (320x180) [22.0 KB] || For More Information || See [http://pao.gsfc.nasa.gov/gsfc/spacesci/sunearth/sunearth.htm#moss](http://pao.gsfc.nasa.gov/gsfc/spacesci/sunearth/sunearth.htm#moss) || ",
            "hits": 29
        },
        {
            "id": 694,
            "url": "https://svs.gsfc.nasa.gov/694/",
            "result_type": "Visualization",
            "release_date": "1999-07-14T12:00:00-04:00",
            "title": "TRACE: 171 Ångstrom Wavelength Image Showing MOSS Disc Center.",
            "description": "An animation of TRACE imagery in the 171 Ångstrom wavelength, showing a MOSS disc center || a000694.00010_print.png (720x480) [479.1 KB] || a000694_thm.png (80x40) [6.2 KB] || a000694_pre.jpg (320x238) [9.8 KB] || a000694_pre_searchweb.jpg (320x180) [58.7 KB] || a000694.webmhd.webm (960x540) [2.1 MB] || a000694.dv (720x480) [29.8 MB] || a000694.mp4 (640x480) [1.5 MB] || a000694.mpg (352x240) [1.3 MB] || ",
            "hits": 33
        },
        {
            "id": 695,
            "url": "https://svs.gsfc.nasa.gov/695/",
            "result_type": "Visualization",
            "release_date": "1999-07-14T12:00:00-04:00",
            "title": "TRACE: 195 Ångstrom Wavelength Image Showing MOSS Shockwave.",
            "description": "An animation of TRACE imagery in the 195 Ångstrom wavelength, showing a MOSS shockwave || a000695.00010_print.png (720x480) [485.4 KB] || a000695_thm.png (80x40) [5.3 KB] || a000695_pre.jpg (320x238) [10.0 KB] || a000695_pre_searchweb.jpg (320x180) [54.2 KB] || a000695.webmhd.webm (960x540) [3.1 MB] || a000695.dv (720x480) [39.6 MB] || a000695.mp4 (640x480) [1.9 MB] || a000695.mpg (352x240) [1.9 MB] || ",
            "hits": 35
        },
        {
            "id": 289,
            "url": "https://svs.gsfc.nasa.gov/289/",
            "result_type": "Visualization",
            "release_date": "1998-12-22T12:00:00-05:00",
            "title": "Zoom in on the Sun with TRACE Imagery: Zoom 1",
            "description": "Zoom into TRACE solar mosaic || a000289.00095_print.png (720x480) [299.7 KB] || a000289_thm.png (80x40) [5.4 KB] || a000289_pre.jpg (320x238) [9.1 KB] || a000289_pre_searchweb.jpg (320x180) [61.8 KB] || a000289.webmhd.webm (960x540) [4.1 MB] || a000289.dv (720x480) [110.0 MB] || a000289.mp4 (640x480) [6.3 MB] || a000289.mpg (352x240) [3.7 MB] || Video slate image reads \"TRACE Zoom One\". || a000289_slate.jpg (720x528) [55.3 KB] || a000289_slate_web.png (320x234) [49.8 KB] || ",
            "hits": 81
        },
        {
            "id": 290,
            "url": "https://svs.gsfc.nasa.gov/290/",
            "result_type": "Visualization",
            "release_date": "1998-12-22T12:00:00-05:00",
            "title": "Zoom in on the Sun with TRACE Imagery: Zoom 2",
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            "title": "Zoom into the Bottom Right of the Sun using TRACE Imagery",
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}