{
    "id": 3742,
    "url": "https://svs.gsfc.nasa.gov/3742/",
    "page_type": "Visualization",
    "title": "Space Weather Event: A View from the Orbit Plane",
    "description": "We start with a view of the space between the Sun (left) and the Earth (within the small rectangular box on the right), slightly above the ecliptic plane. In the plane of the Earth's orbit, we show a 'slice' of the particle density profile of the solar wind (white to yellow for decreasing particle density). Perpendicular to this, we have another 'slice' of particle density from the Enlil model. The Enlil model extends to 60 degrees above and below the solar equator, and beyond 20 solar radii from the Sun. This gap creates the 'hourglass' empty region around the Sun.The CME (orange surface) erupts in the direction of the Earth. The orange surface represents a boundary of common pressure differences, which better identifies sharp transitions in pressure common in shocks fronts. The CME clears out particles in the region behind it, called a rarefaction (Wikipedia), visible in the particle density.This visualization is part of a series of visualizations on space weather modeling. || ",
    "release_date": "2010-07-08T00:00:00-04:00",
    "update_date": "2023-05-03T13:54:09.159055-04:00",
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        "filename": "SWsideViewXZ.slate_tour.HD720p.0086.jpg",
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        "width": 1280,
        "height": 720,
        "pixels": 921600
    },
    "main_video": null,
    "main_credits": {
        "Visualizations by": [
            {
                "name": "Tom Bridgman",
                "employer": "Global Science and Technology, Inc."
            }
        ]
    },
    "progress": "Complete",
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            "title": "",
            "caption": "",
            "description": "We start with a view of the space between the Sun (left) and the Earth (within the small rectangular box on the right), slightly above the ecliptic plane. In the plane of the Earth's orbit, we show a 'slice' of the particle density profile of the solar wind (white to yellow for decreasing particle density). Perpendicular to this, we have another 'slice' of particle density from the Enlil model. The Enlil model extends to 60 degrees above and below the solar equator, and beyond 20 solar radii from the Sun. This gap creates the 'hourglass' empty region around the Sun.<p><p>The CME (orange surface) erupts in the direction of the Earth. The orange surface represents a boundary of common pressure differences, which better identifies sharp transitions in pressure common in shocks fronts. The CME clears out particles in the region behind it, called a rarefaction (<a href=\"http://en.wikipedia.org/wiki/Rarefaction\">Wikipedia</a>), visible in the particle density.<p><p>This visualization is part of a series of visualizations on <a href=\"/Gallery/SpaceWeatherModeling.html\">space weather modeling</a>.</p>",
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            "title": "",
            "caption": "",
            "description": "This is the full movie of the CME striking the Earth. ",
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            "description": "The CME has not yet been ejected.",
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            "url": "https://svs.gsfc.nasa.gov/3742/#media_group_353042",
            "widget": "Single image",
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            "description": "The CME has passed the Earth.",
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    "studio": "svs",
    "funding_sources": [
        "NASA Heliophysics"
    ],
    "credits": [
        {
            "role": "Animator",
            "people": [
                {
                    "name": "Tom Bridgman",
                    "employer": "Global Science and Technology, Inc."
                },
                {
                    "name": "Greg Shirah",
                    "employer": "NASA/GSFC"
                }
            ]
        },
        {
            "role": "Producer",
            "people": [
                {
                    "name": "Scott Wiessinger",
                    "employer": "UMBC"
                }
            ]
        },
        {
            "role": "Scientist",
            "people": [
                {
                    "name": "Michael Hesse",
                    "employer": "NASA/GSFC"
                }
            ]
        }
    ],
    "missions": [],
    "series": [
        "Space Weather Modeling"
    ],
    "tapes": [],
    "papers": [],
    "datasets": [
        {
            "name": "Enlil Heliospheric Model",
            "common_name": "Enlil Heliospheric Model",
            "platform": null,
            "sensor": null,
            "type": "Model",
            "organizations": [
                "Community Coordinated Modeling Center (CCMC)"
            ],
            "description": "MHD solar wind simulation",
            "credit": "",
            "url": "",
            "date_range": "2006/1211T02:24:42 -2006/12/15T23:55:02"
        }
    ],
    "nasa_science_categories": [
        "Earth",
        "Sun"
    ],
    "keywords": [
        "Computer Model",
        "Coronal Mass Ejections",
        "Earth Science",
        "HDTV",
        "Solar Activity",
        "Space Weather",
        "Sun-earth Interactions"
    ],
    "recommended_pages": [],
    "related": [
        {
            "id": 4188,
            "url": "https://svs.gsfc.nasa.gov/4188/",
            "page_type": "Visualization",
            "title": "Comparative Magnetospheres: A Noteworthy Coronal Mass Ejection",
            "description": "In an effort to understand and predict the impact of space weather events on Earth, the Community-Coordinated Modeling Center (CCMC) at NASA Goddard Space Flight Center, routinely runs computer models of the many historical events.  These model runs are then compared to actual data to determine ways to improve the model, and therefore forecasts of the impacts of future space weather events.In mid-December of 2006, the Sun erupted with a bright flare and coronal mass ejection (CME) that launched particles Earthward.  While not the brightest or largest event observed, its impact on Earth was substantial, requiring some effort to protect satellites (ESA: Reacting to a solar flare).The visualization presented here is a CCMC run of a BATS-R-US model simulating the impact of this event on Earth.  Here, lines are used to represent the 'flow direction' of magnetic field of the solar wind impacting Earth, as well as the effects on Earth's geomagnetic field. A 'cut-plane' through the data illustrates the changes in the particle density in the solar wind and magnetosphere.  The color of the data represents a logarithmic scaling of density, with red as the highest (1000 particles per cubic centimeter) down to blue (0.01 particles per cubic centimeter).  In this simulation, each frame of the movie corresponds to two minutes of real time.In the movie, we see vertical field lines of magnetic field carried by the solar wind, coming in from the left.  As this field, and the plasma carrying it, strike Earth's magnetic field, they bend and reconnect, around the Earth.  Some field lines actually reconnect to the polar regions of the Earth, providing a ready flow-path for particles to reach the ionosphere and generate aurora.   This interaction between the solar wind and the plasma trapped in Earth's magnetosphere also creates a density enhancement between Earth and the solar wind helping to shield Earth from some of the effects.   A lower density wake forms behind Earth (the blue region).  There is a circular 'hole' around the Earth which is a gap in the model. || ",
            "release_date": "2014-09-25T10:00:00-04:00",
            "update_date": "2025-01-05T22:31:29.713646-05:00",
            "main_image": {
                "id": 452471,
                "url": "https://svs.gsfc.nasa.gov/vis/a000000/a004100/a004188/Earth_December2006_Pullout.noslate_GSEmove.HD1080i.0300_print.jpg",
                "filename": "Earth_December2006_Pullout.noslate_GSEmove.HD1080i.0300_print.jpg",
                "media_type": "Image",
                "alt_text": "This movie opens with a close-up view of Earth with geo-magnetic field lines.  The camera pulls out and fades in a profile slice of the plasma density data.This video is also available on our YouTube channel.",
                "width": 1024,
                "height": 576,
                "pixels": 589824
            }
        }
    ],
    "sources": [],
    "products": [],
    "newer_versions": [],
    "older_versions": [],
    "alternate_versions": []
}