Coronal mass ejection to pass Earth, Messenger and Juno

Jul 16, 2013
The European Space Agency/NASA Solar and Heliospheric Observatory captured this image of a coronal mass ejection as it left the sun in the direction of Earth and Mercury on July 16, 2013, at 4:24 a.m. EDT. Credit: ESA&NASA/SOHO

On July 16, 2013, at 12:09 a.m. EDT, the sun erupted with an Earth-directed coronal mass ejection or CME, a solar phenomenon that can send billions of tons of particles into space that can reach Earth one to three days later. These particles cannot travel through the atmosphere to harm humans on Earth, but they can affect electronic systems in satellites and on the ground.

Experimental NASA research models, based on observations from NASA's Solar Terrestrial Relations Observatory, show that the CME left the sun at speeds of around 560 miles per second, which is a fairly typical speed for CMEs.

Earth-directed CMEs can cause a space called a , which occurs when they funnel energy into Earth's magnetic envelope, the magnetosphere, for an extended period of time. The CME's magnetic fields peel back the outermost layers of Earth's fields changing their very shape. Magnetic storms can degrade communication signals and cause unexpected electrical surges in power grids. They also can cause aurora. Storms are less frequent during solar minimum, but as the sun's activity ramps up every 11 years toward solar maximum – currently expected in late 2013—large storms occur more frequently.

The CME may also pass by the Messenger and Juno spacecraft and their mission operators have been notified. If warranted, operators can put spacecraft into safe mode to protect the instruments from the solar material.

In the past, geomagnetic storms caused by CMEs of this strength have usually been mild.

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GSwift7
5 / 5 (1) Jul 17, 2013
but as the sun's activity ramps up every 11 years toward solar maximum – currently expected in late 2013—large storms occur more frequently


The latest news on the current solar cycle might indicate that it's slowing down, having already reached the peak. If so, then this will have been the calmest maximum in a very long time, with a peak level of activity that didn't even equal the minimum of some previous cycles (depending on which set of measurements you're looking at).

Looking at only sunspot counts can be deceptive though, because once it reaches zero, that's as low as it gets. The factors driving the activity continue to fluctuate below the threshold of zero sunspots.

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