Activity continues on the Sun

May 15, 2013
NASA's Solar Dynamics Observatory captured this image of the X1.2 class solar flare on May 14, 2013. The image show light with a wavelength of 304 angstroms. Credit: NASA/SDO

(Phys.org) —Solar activity continued on May 14, 2013, as the sun emitted a fourth X-class flare from its upper left limb, peaking at 9:48 p.m. EDT.

This flare is classified as an X1.2 flare and it is the 18th X-class flare of the current . The flare caused a radio blackout – categorized as an R3, or strong, on NOAA's space weather scales from R1 to R5—which has since subsided.

The flare was also associated with a non-Earth-directed CME. CMEs and flares are separate but related : solar flares are powerful bursts that send light and radiation into space; CMEs erupt with billions of tons of solar material. They often, but do not always, occur together. Any time we can see a solar flare from Earth's view, than at least some of its light and radiation must be directed at Earth. CMEs on the other hand may or may not be Earth directed. NASA observes CMEs, however, even when they are not traveling toward Earth, because they may impact spacecraft.

NASA's Solar Dynamics Observatory captured an image of the X1.2 class on May 14, 2013.

These images from NASA's Solar Dynamics Observatory show four X-class flares emitted on May 12-14, 2013 -- the first four X-class flares of 2013. Each panel is a blend of two images one showing light in the 171 Angstrom wavelength and the other in 131 Angstroms. Credit: NASA/SDO/GSFC

Experimental NASA research models show that this CME left the sun at around 745 miles per second, beginning at 10:18 p.m. EDT. It is not Earth-directed, however it may pass the Spitzer and orbits, and their mission operators have been notified. If warranted, operators can put spacecraft into safe mode to protect the instruments from solar material.

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