{
    "count": 5,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 13714,
            "url": "https://svs.gsfc.nasa.gov/13714/",
            "result_type": "Produced Video",
            "release_date": "2020-09-15T13:00:00-04:00",
            "title": "Solar Cycle 25 Is Here. NASA, NOAA Scientists Explain What This Means",
            "description": "Solar Cycle 25 has begun. The Solar Cycle 25 Prediction Panel announced solar minimum occurred in December 2019, marking the transition into a new solar cycle. In a press event, experts from the panel, NASA, and NOAA discussed the analysis and Solar Cycle 25 prediction, and how the rise to the next solar maximum and subsequent upswing in space weather will impact our lives and technology on Earth.A new solar cycle comes roughly every 11 years. Over the course of each cycle, the star transitions from relatively calm to active and stormy, and then quiet again; at its peak, the Sun’s magnetic poles flip. Now that the star has passed solar minimum, scientists expect the Sun will grow increasingly active in the months and years to come.Understanding the Sun’s behavior is an important part of life in our solar system. The Sun’s outbursts—including eruptions known as solar flares and coronal mass ejections—can disturb the satellites and communications signals traveling around Earth, or one day, Artemis astronauts exploring distant worlds. Scientists study the solar cycle so we can better predict solar activity.Click here for the NOAA press kit.Listen to the media telecon.Participants:• Lisa Upton, Co-chair, Solar Cycle 25 Prediction Panel; Solar Physicist, Space Systems Research Corporation• Doug Biesecker, Solar Physicist, NOAA’s Space Weather Prediction Center; Co-chair, Solar Cycle 25 Prediction Panel• Elsayed Talaat, Director, Office of Projects, Planning and Analysis; NOAA’s Satellite and Information Service • Lika Guhathakurta, Heliophysicist, Heliophysics Division, NASA Headquarters • Jake Bleacher, Chief Exploration Scientist, NASA Human Exploration and Operations Mission Directorate || ",
            "hits": 274
        },
        {
            "id": 13706,
            "url": "https://svs.gsfc.nasa.gov/13706/",
            "result_type": "Produced Video",
            "release_date": "2020-09-11T06:00:00-04:00",
            "title": "NASA/NOAA Interview Opportunity: Space Weather live shots",
            "description": "Click here for NOAA's Solar Minimum Press Kit with downloadable imagery and b-roll.Cut b-roll for the live shots will be posted Tuesday, Sept 15 by 4:00 p.m. EST || SolarBanner5.jpg (382x2448) [463.6 KB] || SolarBanner5_print.jpg (1024x159) [164.0 KB] || SolarBanner5_searchweb.png (320x180) [93.2 KB] || SolarBanner5_thm.png (80x40) [18.1 KB] || ",
            "hits": 42
        },
        {
            "id": 40271,
            "url": "https://svs.gsfc.nasa.gov/gallery/live-shots-gallery/",
            "result_type": "Gallery",
            "release_date": "2015-11-27T00:00:00-05:00",
            "title": "Live Shots Gallery Collection",
            "description": "Collection of live shot pages of b-roll and interviews!",
            "hits": 550
        },
        {
            "id": 10817,
            "url": "https://svs.gsfc.nasa.gov/10817/",
            "result_type": "Produced Video",
            "release_date": "2011-09-07T12:00:00-04:00",
            "title": "SDO EVE Late Phase Flares",
            "description": "Scientists have been seeing just the tip of the iceberg when monitoring flares with X-rays. With the complete extreme ultraviolet (EUV) coverage by the SDO EUV Variability Experiment (EVE), they have observed enhanced EUV radiation that appears not only during the X-ray flare, but also a second time delayed by many minutes after the X-ray flare peak. These delayed, second peaks are referred to as the EUV Late Phase contribution to flares.The solar EUV radiation creates our Earth's ionosphere (plasma in our atmosphere), so solar flares disturb our ionosphere and consequently our communication and navigation technologies, such as Global Positioning System (GPS), that transmit through the ionosphere. For over 30 years, scientists have relied on the GOES X-ray monitor to tell them when to expect disturbances to our ionosphere. With these new SDO EVE results, they now recognize that additional ionospheric disturbances from these later EUV enhancements are also a concern. || ",
            "hits": 73
        },
        {
            "id": 10733,
            "url": "https://svs.gsfc.nasa.gov/10733/",
            "result_type": "Produced Video",
            "release_date": "2011-03-03T16:00:00-05:00",
            "title": "SDO First Light Media",
            "description": "A compilation of some of the videos and stills used during the SDO First Light press conference.There are more video and stills available. || ",
            "hits": 74
        }
    ]
}