Observing a Gigantic Eruption of Solar Material

NASA | JUNE 1, 2014

A coronal mass ejection, or CME, surged off the side of the sun on May 9, 2014, and NASA's newest solar observatory caught it in extraordinary detail. This was the first CME observed by the Interface Region Imaging Spectrograph, or IRIS, which launched in June 2013 to peer into the lowest levels of the sun's atmosphere with better resolution than ever before.

A coronal mass ejection burst off the side of the sun on May 9, 2014. Image Credit: NASA/LMSAL/IRIS/SDO/Goddard.

IRIS must commit to pointing at certain areas of the sun at least a day in advance, so catching a CME in the act involves some educated guesses and a little bit of luck.

The IRIS imagery focuses in on material of 30,000 kelvins at the base, or foot points, of the CME.

The line moving across the middle of the movie is the entrance slit for IRIS's spectrograph, an instrument that can split light into its many wavelengths – a technique that ultimately allows scientists to measure temperature, velocity and density of the solar material behind the slit.

The field of view for this imagery is about five Earths wide and about seven-and-a-half Earths tall.

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