Solar Dynamics Observatory sees 'Cinco de Mayo' solar flare

Solar Dynamics Observatory sees 'Cinco de Mayo' solar flare
Credit: NASA/SDO/Wiessinger

NASA's Solar Dynamics Observatory, which watches the sun constantly, captured these images of a significant solar flare – as seen in the bright flash on the left – peaking at 6:11 p.m. EDT on May 5, 2015.

Each image shows a different wavelength of that highlights a different temperature of material on the sun. By comparing different images, scientists can better understand the movement of solar matter and energy during a flare. From left to right, the wavelengths are: visible light, 171 angstroms, 304 angstroms, 193 angstroms and 131 angstroms. Each wavelength has been colorized.

Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however—when intense enough—they can disturb the atmosphere in the layer where GPS and communications signals travel. This flare is classified as an X2.7-class flare. X-class denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, and so on.


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Citation: Solar Dynamics Observatory sees 'Cinco de Mayo' solar flare (2015, May 7) retrieved 18 August 2019 from https://phys.org/news/2015-05-solar-dynamics-observatory-cinco-de.html
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