STEREO and SDO observes coronal mass ejection

On August 1st, the sun emitted a C-class solar flare that spawned what scientists call a coronal mass ejection, or CME, headed toward Earth. The CME impacted Earth's magnetic field August 3rd. CMEs occasionally hit Earth. This CME will have few noticeable consequences beyond producing an aurorae.

The CME hit Earth's magnetic field on August 3rd at 17:40 UTC. The impact sparked a G2-class geomagnetic storm that lasted nearly 12 hours -- time enough for auroras to spread all the way from Europe to North America.

CMEs are large clouds of charged particles that are ejected from the sun over the course of several hours and can carry up to ten billion tons of plasma. They expand away from the sun at speeds as high as a million miles an hour. A CME can make the approximately 150-million-km or 93-million-mile journey to Earth in just two to four days. Stronger solar storms could cause adverse impacts to space-based assets and technological infrastructure on Earth.

The sun goes through a regular activity cycle about 11 years long. The last solar maximum occurred in 2001 and its recent extreme solar minimum was particularly weak and long lasting. These kinds of eruptions are one of the first signs that the sun is waking up and heading toward another solar maximum expected in the 2013 time frame.


One of the fastest CMEs in years was captured by the STEREO COR1 telescopes on August 1, 2010. This movie, combining COR1-Ahead images with the simultaneous Helium II 304 Angstrom images from the STEREO EUVI telescope, shows the rapid explosion of material outward, followed by a slower eruption of a polar crown prominence from another part of the Sun. This CME is seen to be heading towards Earth at speeds well over 1000 kilometers per second. Credit: NASA/STEREO




High resolution image

On August 1st, almost the entire Earth-facing side of the sun erupted in a tumult of activity. There was a C3-class solar flare, a solar tsunami, multiple filaments of magnetism lifting off the stellar surface, large-scale shaking of the solar corona, radio bursts, a coronal mass ejection and more. This extreme ultraviolet snapshot from the Solar Dynamics Observatory (SDO) shows the sun's northern hemisphere in mid-eruption. Different colors in the image represent different gas temperatures ranging from about 1 to 2 million degrees K. Credit: NASA/SDO




High resolution image

These images taken by the STEREO Ahead satellite from 03:47 to 15:47 UTC on August 2nd show the movement of the CME cloud, on the right of the disc, as it expands toward Earth. Credit: NASA/STEREO Credit: NASA/STEREO

 

Source: NASA
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