1 00:00:00,000 --> 00:00:04,000 Solar flare. A solar flare is a sudden, intense burst of energy from the Sun's 2 00:00:04,000 --> 00:00:08,000 surface, basically, a giant explosion. The Sun is magnetically 3 00:00:08,000 --> 00:00:12,000 charged, and solar flares are caused by tangles in the magnetic field lines on the Sun’s surface. 4 00:00:12,000 --> 00:00:16,000 Solar flares are the largest explosive events in our solar system. 5 00:00:16,000 --> 00:00:20,000 They’re classified by size, with the smallest flares called A-class, followed 6 00:00:20,000 --> 00:00:24,000 by B, C, M, and X. X-class flares can create loops 7 00:00:24,000 --> 00:00:28,000 a hundred times as big as Earth. Solar flares release 8 00:00:28,000 --> 00:00:32,000 large amounts of radiation into space. M- and X-class flares can actually release 9 00:00:32,000 --> 00:00:36,000 enough energy that they can interfere with some radio communications and satellites in Earth’s 10 00:00:36,000 --> 00:00:40,000 orbit when they erupt on the Earth side of the Sun. Fortunately, our atmosphere 11 00:00:40,000 --> 00:00:44,000 protects us from harm here on the ground. The Sun goes through periods of 12 00:00:44,000 --> 00:00:48,000 more and less activity, and solar flares are more common during solar maximum. 13 00:00:48,000 --> 00:00:52,000 At NASA, we work with our partners at NOAA to monitor the Sun and keep an eye out 14 00:00:52,000 --> 00:01:08,267 for magnetic storms caused by solar flares.