{
    "count": 9,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 4026,
            "url": "https://svs.gsfc.nasa.gov/4026/",
            "result_type": "Visualization",
            "release_date": "2013-02-20T10:00:00-05:00",
            "title": "July 2012: Coronal Rain",
            "description": "A moderate solar flare was emitted by the sun on July 19, 2012. At 5:58 UTC it peaked at M7.7 on the flare scale, which makes it fairly powerful, but still much weaker than X-class flares, which are the largest. What made this particular event so noteworthy was the associated activity in the sun's corona. For the next day, hot plasma in corona cooled and condensed along the strong magnetic fields of the region that produced the flare. Magnetic fields are invisible, but the plasma is very obvious in the extreme ultraviolet wavelength of 304 angstroms, which highlights material at a temperature of about 50,000 Kelvin. This plasma is attracted to the magnetic fields and outlines them very clearly as it slowly falls back to the solar surface. This process of condensing plasma falling to the surface is called coronal rain.The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. SDO collected one frame every 12 seconds so each second in this video corresponds to 6 minutes of real time. The video covers 4:30 UTC on July 19th to 2:00 UTC on July 20th, a period of 21 hours and 30 minutes.Music—\"Thunderbolt\" by Lars Leonhard || ",
            "hits": 62
        },
        {
            "id": 4033,
            "url": "https://svs.gsfc.nasa.gov/4033/",
            "result_type": "Visualization",
            "release_date": "2013-02-11T10:00:00-05:00",
            "title": "Monster Prominences with an Earth Eclipse (September 16, 2012)",
            "description": "On September 16, 2012 the sun had a beautiful prominence (see Wikipedia) that slowly twisted and dissipated over several hours. It was captured in 304 angstrom light by the Solar Dynamics Observatory's AIA instrument at 4k resolution and 12s imaging cadence. The prominence was immediately followed by one of the many eclipses that SDO experiences during September, when its orbit places the Earth between it and the sun. || ",
            "hits": 52
        },
        {
            "id": 4034,
            "url": "https://svs.gsfc.nasa.gov/4034/",
            "result_type": "Visualization",
            "release_date": "2013-02-11T10:00:00-05:00",
            "title": "September 23, 2012 Solar Prominence",
            "description": "On September 23, 2012 the sun emitted a large blast of plasma in the form of a prominence (see Wikipedia). This was most visible in extreme ultraviolet light with a wavelength of 304 angstroms. This wavelength highlights plasma with temperatures of around 50,000 Kelvin. The Atmospheric Imaging Assembly on NASA's Solar Dynamics Observatory captured the event at 4k resolution and a high imaging cadence of one image every 12 seconds. || ",
            "hits": 52
        },
        {
            "id": 4037,
            "url": "https://svs.gsfc.nasa.gov/4037/",
            "result_type": "Visualization",
            "release_date": "2013-02-11T10:00:00-05:00",
            "title": "Sunspot Growth in June 2012",
            "description": "Groups of sunspots grow and die over a matter of days. This is a movie built from images taken by the SDO/HMI instrument over the course of 13 days during the rise of solar cycle 24. || ",
            "hits": 35
        },
        {
            "id": 4038,
            "url": "https://svs.gsfc.nasa.gov/4038/",
            "result_type": "Visualization",
            "release_date": "2013-02-11T10:00:00-05:00",
            "title": "Solar Prominence Dance - December 31, 2012",
            "description": "On the final day of 2012, the sun presented a beautiful twisting prominence that rose high into the corona for about 3 hours. It was most visible in extreme ultraviolet light with a wavelength of 304 angstroms. This wavelength highlights plasma with temperatures of around 50,000 Kelvin. The Atmospheric Imaging Assembly on NASA's Solar Dynamics Observatory captured the event at 4k resolution and a high imaging cadence of one image every 12 seconds. || ",
            "hits": 51
        },
        {
            "id": 4039,
            "url": "https://svs.gsfc.nasa.gov/4039/",
            "result_type": "Visualization",
            "release_date": "2013-02-11T10:00:00-05:00",
            "title": "SDO: September 13, 2012 Earth Eclipse",
            "description": "Twice a year, for three weeks near the equinox, NASA's Solar Dynamics Observatory (SDO) moves into its eclipse season — a time when Earth blocks its view of the sun for a period of time each day. Any spacecraft observing the sun from an orbit around Earth has to contend with such eclipses, but SDO's orbit is designed to minimize them as much as possible. On September 13, during the Fall 2012 eclipse season, SDO experienced on such eclipse followed by an unusually large, dark prominence that lifted up off the surface. The prominence was visible in extreme ultraviolet light with a wavelength of 304 angstroms. This wavelength highlights plasma with temperatures of around 50,000 Kelvin. The Atmospheric Imaging Assembly on NASA's Solar Dynamics Observatory captured the event at 4k resolution and a high imaging cadence of one image every 12 seconds. || ",
            "hits": 53
        },
        {
            "id": 4027,
            "url": "https://svs.gsfc.nasa.gov/4027/",
            "result_type": "Visualization",
            "release_date": "2013-01-31T13:00:00-05:00",
            "title": "A July 2012 CME from SDO",
            "description": "On July 18, 2012, a fairly small explosion of light burst off the lower right limb of the sun. Such flares often come with an associated eruption of solar material, known as a coronal mass ejection or CME — but this one did not. Something interesting did happen, however. Magnetic field lines in this area of the sun's atmosphere, the corona, began to twist and kink, generating the hottest solar material — a charged gas called plasma — to trace out the newly-formed slinky shape. The plasma glowed brightly in extreme ultraviolet images from the Atmospheric Imaging Assembly (AIA) aboard NASA's Solar Dynamics Observatory (SDO) and scientists were able to watch for the first time the very formation of something they had long theorized was at the heart of many eruptive events on the sun: a flux rope.Eight hours later, on July 19, the same region flared again. This time the flux rope's connection to the sun was severed, and the magnetic fields escaped into space, dragging billions of tons of solar material along for the ride — a classic CME. || ",
            "hits": 74
        },
        {
            "id": 3999,
            "url": "https://svs.gsfc.nasa.gov/3999/",
            "result_type": "Visualization",
            "release_date": "2012-10-26T00:00:00-04:00",
            "title": "The View from SDO: The August 31, 2012 Filament Eruption",
            "description": "The Solar Dynamics Observatory (SDO) observed a large filament eruption on August 31, 2012. This visualization was generated using high time resolution (12 seconds) data from the Atmospheric Imaging Assembly (AIA). Two datasets are used, the SDO/AIA 304 Ångstrom wavelength (orange color table) and the 171 Ångstrom wavelength (gold color table). These are wavelengths in the ultraviolet band of the electromagnetic spectrum. They are not visible to the human eye or to ground-based telescopes so coded colors are used in presentation.It is the source material for \"August 31, 2012 Magnificent CME\" visualization. || ",
            "hits": 92
        },
        {
            "id": 3963,
            "url": "https://svs.gsfc.nasa.gov/3963/",
            "result_type": "Visualization",
            "release_date": "2012-07-17T00:00:00-04:00",
            "title": "Active Region 1520 from SDO",
            "description": "This is source material for the SDO view of Active Region 1520 in July of 2012. || ",
            "hits": 17
        }
    ]
}