WEBVTT FILE 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.