{
    "count": 11,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 4051,
            "url": "https://svs.gsfc.nasa.gov/4051/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "Boiling Solar Prominence from February 2013",
            "description": "A long-lived prominence (see Wikipedia) hovers over the limb of the Sun (about the 4-5 o'clock position) before breaking up. || ",
            "hits": 24
        },
        {
            "id": 4065,
            "url": "https://svs.gsfc.nasa.gov/4065/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "The X-Class Flare of January 2014",
            "description": "Early January of 2014 saw one of the largest sunspot groups of solar cycle 24 and some X-class flares near the center of the solar disk from active region AR 11943. These flares launched a few small coronal mass ejections towards the Earth. || ",
            "hits": 22
        },
        {
            "id": 4066,
            "url": "https://svs.gsfc.nasa.gov/4066/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "SDO's Multi-wavelength View of a May 2013 Solar Flare",
            "description": "An active region on the left limb of the Sun launches a large flare and coronal material in this sequence from early May 2013. || ",
            "hits": 50
        },
        {
            "id": 4089,
            "url": "https://svs.gsfc.nasa.gov/4089/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "June 2013's 'Busy Sun'",
            "description": "June of 2013, near the maximum of solar cycle 24, while not extremely active from a solar flare perspective, presented a range of diverse phenomena. We have a couple of solar 'tornadoes' (the twisted protrusions off the limb of the Sun in upper and lower left quadrants), which we eventually see erupt material into space. There are also a number of coronal loops in active regions which are incredibly stable but still exhibit much fine detail. || ",
            "hits": 27
        },
        {
            "id": 4090,
            "url": "https://svs.gsfc.nasa.gov/4090/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "Solar Prominence from SDO: July 1, 2013",
            "description": "A large solar prominence, caught in a tug-of-war between solar gravity pulling it downward and magnetic gradients lifting upward, hovers over the limb of the Sun (left) before eventually launching into space. || ",
            "hits": 35
        },
        {
            "id": 4121,
            "url": "https://svs.gsfc.nasa.gov/4121/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "October 2013 X-Flare from Solar Dynamics Observatory",
            "description": "Another Halloween space weather fest? October-November 2003 of the previous solar cycle saw some of the most energetic solar events since space flight (see Halloween Solar Storms 2003: A Multi-Mission View. Halloween of 2013 has seen a similar round of high solar activity, with energetic flares and coronal mass ejections (CMEs). || ",
            "hits": 37
        },
        {
            "id": 4123,
            "url": "https://svs.gsfc.nasa.gov/4123/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "SDO Eclipses & Transits: March 2013",
            "description": "The Solar Dynamics Observatory (SDO) orbits the Earth in a geosynchronous orbit (see The 2012 Earth-Orbiting Heliophysics Fleet and RBSP & SDO: Newest Heliophysics Missions) which keeps the spacecraft in contact with the ground station. This motion of the spacecraft around Earth, combined with the motion of the Moon around Earth, and the motion of Earth around the Sun creates opportunities for eclipses and transits involving these other bodies (see Lunar Transit from Solar Dynamics Observatory (2010). On rare occasions, SDO can see an eclipse and transit on the same day, as illustrated in these images collected from March 11, 2013.These eclipses and transits are not just visually interesting, but important for mission planners as SDO receives much of the electrical power needed to function through solar panels. During these times, SDO needs to operate safely with power from onboard batteries until the time that full solar power can be restored. || ",
            "hits": 28
        },
        {
            "id": 4132,
            "url": "https://svs.gsfc.nasa.gov/4132/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "May 2013: 'Light bulb'-shaped prominence",
            "description": "The active region on the solar limb (left side) generates a large bulb-shaped prominence before demonstrating more energetic activity. See SDO View of a May 2013 Solar Flare. || ",
            "hits": 24
        },
        {
            "id": 4133,
            "url": "https://svs.gsfc.nasa.gov/4133/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "February 2013: The Busy Sun",
            "description": "Even near solar maximum, with sunspots dotting the photosphere, the Sun can look tranquil and serene in visible light. In the case of these images from the HMI instrument on the Solar Dynamics Observatory, the only obvious changes are the constant shimmering of the solar disk due to the bubbling of solar granulation.But in ultraviolet light, in particular the 30.4 nanometer line of the helium ion, we see much more activity. Dark, wispy lines of cooler solar filaments (the term used for solar prominences when seen against the disk) stretch across the disk. The same structures, seen against the fainter glow of the solar corona, resemble slowly evolving flames on the limb of the Sun. Solar active regions surrounding the sunspots, appear bright in ultraviolet light. || ",
            "hits": 35
        },
        {
            "id": 4136,
            "url": "https://svs.gsfc.nasa.gov/4136/",
            "result_type": "Visualization",
            "release_date": "2014-02-11T10:00:00-05:00",
            "title": "More Solar Excitement - October 2013",
            "description": "Solar activity in October 2013 continues with several active regions, particularly on the limb, launching solar material into space. || ",
            "hits": 25
        },
        {
            "id": 4101,
            "url": "https://svs.gsfc.nasa.gov/4101/",
            "result_type": "Visualization",
            "release_date": "2013-09-20T10:00:00-04:00",
            "title": "August 2013: SDO Observes Large Coronal Hole",
            "description": "On the Sun, coronal holes represent regions where the solar magnetic field does not connect back to the Sun. In these cases, the magnetic field guides the charged particles of the solar wind into distant space, forming the fast solar wind. || ",
            "hits": 27
        }
    ]
}