Classifying solar eruptions

Jan 26, 2012 By Karen C. Fox
The Solar Dynamics Observatory (SDO) captured this image of an X 1.9 class solar flare on November 3, 2011. Credit: NASA/SDO

(PhysOrg.com) -- Solar flares are giant explosions on the sun that send energy, light and high speed particles into space. These flares are often associated with solar magnetic storms known as coronal mass ejections (CMEs). While these are the most common solar events, the sun can also emit streams of very fast protons – known as solar energetic particle (SEP) events – and disturbances in the solar wind known as corotating interaction regions (CIRs). All of these can produce a variety of "storms" on Earth that can – if strong enough -- interfere with short wave radio communications, GPS signals, and Earth's power grid, among other things.

The amount of solar activity increases approximately every 11 years, and the is currently moving toward another , likely in 2013. That means more will be coming, some small and some big enough to send their radiation all the way to Earth.

The National Oceanic and Atmospheric Administration has devised categories for the flares and various storms. The biggest flares are known as "X-class flares" based on a classification system that divides according to their strength. The smallest ones are A-class (near background levels), followed by B, C, M, and X. Similar to the Richter scale for earthquakes, each letter represents a 10-fold increase in energy output. So an X is ten times an M and 100 times a C. Within each letter class there is a finer scale from 1 to 9.

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C-class and smaller flares are too weak to noticeably affect Earth. M-class flares can cause brief radio blackouts at the poles and minor radiation storms that might endanger astronauts.

And then come the X-class flares. Although X is the last letter, there are flares more than 10 times the power of an X1, so X-class flares can go higher than 9. The most powerful flare measured with modern methods was in 2003, during the last solar maximum, and it was so powerful that it overloaded the sensors measuring it. The sensors cut out at X15, but the flare was estimated to be as high as an X28.

Fast-moving protons from a solar energetic particle (SEP) event cause interference that looks like snow in these images from the Solar Heliospheric Observatory taken on January 23, 2012. Credit: SOHO/ESA & NASA

The biggest X-class flares are by far the largest explosions in the solar system and are awesome to watch. Loops tens of times the size of Earth leap up off the sun's surface when the sun's magnetic fields cross over each other and reconnect. In the biggest events, this reconnection process can produce as much energy as a billion hydrogen bombs.

As the sun moves towards its next solar maximum and heats up, we are already seeing an increase in activity. The first X-class flare of the current solar cycle erupted on February 15, 2011, and there were more over the summer. On January 23, 2012, the sun unleashed an M8.7 flare accompanied by a CME and an SEP that created one of the strongest radiation storms since 2005.

If they're directed at Earth, such flares and associated solar events can create long lasting radiation storms that can harm satellites, communications systems, and even ground-based technologies and power grids. NASA and NOAA – as well as the US Air Force Weather Agency (AFWA) and others -- keep a constant watch on the sun to monitor for X-class flares and their associated magnetic storms. With advance warning many satellites, spacecraft and technologies can be protected from the worst effects.

Explore further: Cassini sees sunny seas on Titan

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