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</a> “This is the first time we’ve seen the entire, detailed structure of this process, because of the high-quality data from SDO,” Su said. The new evidence will lead to a better model of magnetic reconnection, how fast the process happens and the energy involved in the process, NASA notes. The newer models will help scientists observe other stars, as magnetic reconnection occurs in stars throughout the universe, and can help create better advanced warning systems for space weather. Coronal mass ejections and solar flares can send particles and radiation toward Earth. While the radiation cannot get through the Earth’s atmosphere, space weather can affect satellites and radio communication.
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</a> “This is the first time we’ve seen the entire, detailed structure of this process, because of the high-quality data from SDO,” Su said. The new evidence will lead to a better model of magnetic reconnection, how fast the process happens and the energy involved in the process, NASA notes. The newer models will help scientists observe other stars, as magnetic reconnection occurs in stars throughout the universe, and can help create better advanced warning systems for space weather. Coronal mass ejections and solar flares can send particles and radiation toward Earth. While the radiation cannot get through the Earth’s atmosphere, space weather can affect satellites and radio communication.
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