{
    "count": 7,
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    "results": [
        {
            "id": 13494,
            "url": "http://svs.gsfc.nasa.gov/13494/",
            "result_type": "Produced Video",
            "release_date": "2019-12-11T13:00:00-05:00",
            "title": "AGU 2019 - New Science from NASA's Parker Solar Probe Mission",
            "description": "Little more than a year into its mission, Parker Solar Probe has returned gigabytes of data on the Sun and its atmosphere. The very first science from the Parker mission is just beginning to be shared, and five researchers presented new findings from the mission at the fall meeting of the American Geophysical Union on Dec. 11, 2019. Their research hints at the processes behind both the Sun's continual outflow of material — the solar wind — and more infrequent solar storms that can disrupt technology and endanger astronauts, along with new insight into space dust that creates the Geminids meteor shower.Speakers:Nicholeen Viall - Research Astrophysicist, NASA's Goddard Space Flight CenterTim Horbury - Professor of Physics, Imperial College LondonKelly Korreck - Astrophysicist, Head of Science Operations for SWEAP Suite, Harvard and Smithsonian Center for AstrophysicsNathan Schwadron - Presidential Chair, Norman S. and Anna Marie Waite Professor, University of New HampshireKarl Battams - Computational Scientist, U.S. Naval Research Laboratory || ",
            "hits": 66
        },
        {
            "id": 4087,
            "url": "http://svs.gsfc.nasa.gov/4087/",
            "result_type": "Visualization",
            "release_date": "2013-07-10T13:00:00-04:00",
            "title": "IBEX Heliotail Observations",
            "description": "The IBEX (Interstellar Boundary EXplorer) continues to collect data on the flux of neutral atoms from the boundary of the solar wind with the interstellar medium.Starting with the IBEX satellite in orbit around the Earth, we zoom out to beyond the orbit of Neptune, illustrating the direction of the Sun relative to the local stars (red arrow) and relative to the local interstellar medium (violet arrow). These directions are different because the local interstellar medium (mostly gas and dust) move relative to the local stars.The boundaries of the termination shock (red ellipsoidal surface) and heliopause (green) created by the interaction of the solar wind with the interstellar medium is displayed. The camera rotates to a view 'nose on' with the heliopause, and a sphere is faded in representing the region where the neutral atoms detected by IBEX originate. The sphere around the Sun is 'unwrapped' to reproject the IBEX data into an approximately Aitoff projection. || ",
            "hits": 59
        },
        {
            "id": 11301,
            "url": "http://svs.gsfc.nasa.gov/11301/",
            "result_type": "Produced Video",
            "release_date": "2013-07-10T12:30:00-04:00",
            "title": "IBEX Provides First View Of the Solar System’s Tail",
            "description": "This page contains resources from the July 10, 2013 media briefing.To watch the media briefing on YouTube, click here.To view the web short on YouTube about this story, click here.NASA’s Interstellar Boundary Explorer, or IBEX, recently mapped the boundaries of the solar system’s tail, called the heliotail. By combining observations from the first three years of IBEX imagery, scientists have mapped out a tail that shows a combination of fast and slow moving particles. The entire structure twisted, because it experiences the pushing and pulling of magnetic fields outside the solar system. || ",
            "hits": 67
        },
        {
            "id": 3900,
            "url": "http://svs.gsfc.nasa.gov/3900/",
            "result_type": "Visualization",
            "release_date": "2012-01-31T13:00:00-05:00",
            "title": "The Local Interstellar Wind as Seen by IBEX",
            "description": "This visual presents a color-coded full-sky neutral atom map in a Hammer projection. This map is different from earlier IBEX maps in that it shows atoms only at energies where the interstellar wind is the brightest feature in the maps. In Earth's orbit, where IBEX makes its observations, the maximum flow (in red) is seen to arrive from Libra instead of Scorpio because the interstellar wind is forced to curve around the Sun by gravity. || ",
            "hits": 45
        },
        {
            "id": 10669,
            "url": "http://svs.gsfc.nasa.gov/10669/",
            "result_type": "Produced Video",
            "release_date": "2010-09-30T13:00:00-04:00",
            "title": "NASA Mission Shows Evolution of Conditions at Edge of Solar System",
            "description": "New data from NASA's Interstellar Boundary Explorer, or IBEX, spacecraft, reveal that conditions at the edge of our solar system may be much more dynamic than previously thought. Future exploration missions will benefit in design and mission objectives from a better understanding of the changing conditions in this outer region of our solar system.The IBEX has produced a new set of \"all-sky\" maps of our solar system's interaction with the galaxy, allowing researchers to continue viewing and studying the interaction between our galaxy and sun. The new maps reveal changing conditions in the region that separates the nearest reaches of our galaxy, called the local interstellar medium, from our heliosphere — a protective bubble that shields and protects our solar system.In October 2009, scientists announced that the first map data produced by IBEX revealed an unpredicted bright ribbon of energetic neutral atoms emanating toward the sun from the edge of the solar system. This discovery was unexpected to scientists, because the ribbon of bright emissions did not resemble any previous theoretical models of the region.The IBEX spacecraft creates sky maps by measuring and counting particles referred to as energetic neutral atoms that are created in an area of our solar system known as the interstellar boundary region. This imaging technique is required since this region emits no light that can be collected by conventional telescopes. This interstellar boundary is where charged particles from the sun, called the solar wind, flow outward far beyond the orbits of the planets and collide with material between stars. These collisions cause energetic neutral atoms to travel inward toward the sun from interstellar space at velocities ranging from 100,000 mph to more than 2.4 million mph.This second set of all-sky maps, created using data collected during six months of observations, show the evolution of the interstellar boundary region. The maps help delineate the interstellar boundary region, the area at the edge of our solar system that shields it from most of the dangerous galactic cosmic radiation that would otherwise enter from interstellar space. The new findings were published this week in the Journal of Geophysical Research - Space Physics, a publication of the American Geophysical Union. || ",
            "hits": 44
        },
        {
            "id": 3769,
            "url": "http://svs.gsfc.nasa.gov/3769/",
            "result_type": "Visualization",
            "release_date": "2010-09-30T12:00:00-04:00",
            "title": "IBEX Skymaps and the Bright Stars",
            "description": "In this image set, the brighter stars from the Tycho skymap have been reprojected into positions corresponding to the coordinate system used by the IBEX mission.The colors represent the number of neutral atoms (in the specified band of energies) detected by IBEX in each block of sky. Each block in the map is roughly a square about 6 degrees by 6 degrees (or the width of 12 full Moons, on a side). For the energy band displayed of 2.73 keV, violet corresponds to undetectable emission, while red corresponds to the detection of about 50 atoms per second per square centimeter in the angular segment of the sky. There is a 'hole' in the data (black) created when the IBEX scan cuts through the Earth's magnetotail.The images in this set have been co-registered for easy compositing. || ",
            "hits": 32
        },
        {
            "id": 3770,
            "url": "http://svs.gsfc.nasa.gov/3770/",
            "result_type": "Visualization",
            "release_date": "2010-09-30T12:00:00-04:00",
            "title": "IBEX Observes Changes in Heliopause Emission",
            "description": "The camera view moves from the heliosphere 'nose', the apparent direction of the heliopause relative to the interstellar wind, towards the 'knot'. The 'knot' represents a direction of high emission of neutral atoms which has changed significantly in the six months since the first IBEX map.We fade-in an artistic conception of the 'knot', which untangles during the six months as we fade to the second IBEX map. || ",
            "hits": 32
        }
    ]
}