The leading edge of the March 6 coronal mass ejection, or CME, reached NASA’s Advanced Composition Explorer, or ACE satellite at 5:42 a.m. EST this morning. ACE sits just outside of Earth’s magnetic environment, the magnetosphere. As magnetic fields from the CMEs connected up to the magnetosphere, instruments on Earth began to measure changes in our planet’s magnetic fields – indicating the onset of a geomagnetic storm.
NASA models using data from the Solar Terrestrial Relations Observatory, or STEREO, and the Solar Heliospheric Observatory, or SOHO have now provided more information about the two CMEs associated with the March 6 flares. The first is traveling faster than 1,300 miles per second; the second more than 1,100 miles per second. NASA’s models predict that the CMEs will impact both Earth and Mars, as well as pass by several NASA spacecraft – Messenger, Spitzer, and STEREO-B. The models also predicted that the leading edge of the first CME will reach Earth at about 1:25 a.m. EST on the morning of March 8 (plus or minus 7 hours). Such a CME could result in a severe geomagnetic storm, causing aurora at low latitudes, with possible disruption to high frequency radio communication, global positioning systems (GPS), and power grids.
This movie of the March 6, 2012 X5.4 flare was captured by the Solar Dynamics Observatory (SDO) in the 171 Angstrom wavelength. One of the most dramatic features is the way the entire surface of the sun seems to ripple with the force of the eruption. This movement comes from something called EIT waves – because they were first discovered with the Extreme ultraviolet Imaging Telescope (EIT)