{
    "count": 3,
    "next": null,
    "previous": null,
    "results": [
        {
            "id": 20408,
            "url": "https://svs.gsfc.nasa.gov/20408/",
            "result_type": "Animation",
            "release_date": "2025-08-22T09:00:00-04:00",
            "title": "Solar Particle Acceleration",
            "description": "The Sun constantly emits a stream of high energy particles that can be accelerated by magnetic fields and other processes to nearly the speed of light. These particles, made of protons, ions and electrons, can be damaging at Earth where they can impede the function of satellites and telecommunications. NASA’s IMAP (Interstellar Mapping and Acceleration Probe) studies particle acceleration to better understand the fundamental processes driving these particles. This information will help scientists better understand and prepare for their effects at Earth, collectively called space weather. || ",
            "hits": 116
        },
        {
            "id": 20320,
            "url": "https://svs.gsfc.nasa.gov/20320/",
            "result_type": "Animation",
            "release_date": "2020-08-14T09:00:00-04:00",
            "title": "Solar Energetic Particles",
            "description": "The Sun goes through phases of strong activity, during which eruptions can occur. Such eruptions can have multiple components, including X rays, coronal mass ejection plasma, and solar energetic particles – bursts or events of fast-moving particles.  These events can occur suddenly and have the potential to rapidly change the radiation environment of wide swaths of the inner solar system where they may create hazardous conditions.  Not only are such conditions dangerous for humans in space, but the intense ionizing radiation can also affect the interior of spacecraft, including sensitive electronics.  Solar energetic particles can reach all regions of near-Earth space, including the lunar surface, with the exception of  low-altitude and low-latitude Earth orbit, where the Earth’s magnetic field is strong enough to form a protective barrier. || ",
            "hits": 400
        },
        {
            "id": 13275,
            "url": "https://svs.gsfc.nasa.gov/13275/",
            "result_type": "Produced Video",
            "release_date": "2019-08-07T11:30:00-04:00",
            "title": "How NASA Will Protect Astronauts From Space Radiation",
            "description": "Today, the Apollo-era flares serve as a reminder of the threat of radiation exposure for technology and astronauts in space. Understanding and predicting solar eruptions is crucial for safe space exploration. Almost 50 years since those 1972 storms, the data, technology and resources available to NASA have improved, enabling advancements towards space weather forecasts and astronaut protection — key to NASA’s Artemis program to return astronauts to the Moon.",
            "hits": 734
        }
    ]
}