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Active Region on the Sun Emits Another Flare
10.23.12
 
The sun emitted a significant solar flare on Oct. 22, 2012, peaking at 11:17 p.m. EDT. The flare came from an active region on the left side of the sun that has been numbered AR 1598, which has already been the source of a number of weaker flares. This flare was classified as an X1.8-class flare.

solar flare on Oct. 22, 2012 as captured by NASA's Solar Dynamics Observatory (SDO) in the 131 Angstrom wavelength
A solar flare on Oct. 22, 2012, as captured by NASA's Solar Dynamics Observatory (SDO) in the 131 Angstrom wavelength. This wavelength of light is used for observing solar material heated to 10 million Kelvin, as in a solar flare. The wavelength is typically colorized in teal, as it is here. (Credit: NASA/SDO/Goddard)
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"X-class" denotes the most intense flares, while the number provides more information about its strength. An X2 is twice as intense as an X1, an X3 is three times as intense, and on. An X-class flare of this intensity can cause degradation or blackouts of radio communications for about an hour.

Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth's atmosphere to physically affect humans on the ground, however -- when intense enough -- they can disturb the atmosphere in the layer where GPS and communications signals travel. This can disrupt radio signals for anywhere from minutes to hours.

Video of the Oct. 22, 2012, solar flare as captured by NASA's Solar Dynamics Observatory (SDO) in the 131 and 304 Angstrom wavelengths. (Credit: NASA/SDO/Goddard)
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The National Oceanic and Atmospheric Association, which is the United States government's official source for space weather forecasts and alerts, categorized the radio blackout associated with this flare as an R3, on a scale from R1 to R5. It has since subsided.

Four views of solar flare on Oct. 22, 2012 as captured by NASA's Solar Dynamics Observatory (SDO). Clockwise from top left: 171 Angstrom wavelength, 335 Angstroms wavelength, magnetogram showing magnetically active regions on the sun, 304 Angstrom wavelength.
By observing the sun in a number of different wavelengths, NASA's telescopes can tease out different aspects of events on the sun. These four images of a solar flare on Oct. 22, 2012, show from the top left, and moving clockwise: light from the sun in the 171 Angstrom wavelength, which shows the structure of loops of solar material in the sun's atmosphere, the corona; light in 335 Angstroms, which highlights light from active regions in the corona; a magnetogram, which shows magnetically active regions on the sun; light in the 304 Angstrom wavelength, which shows light from the region of the sun's atmosphere where flares originate. (Credit: NASA/SDO/Goddard)
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Increased numbers of flares are quite common at the moment, since the sun's normal 11-year activity cycle is ramping up toward solar maximum, which is expected in 2013. Humans have tracked this solar cycle continuously since it was discovered in 1843, and it is normal for there to be many flares a day during the sun's peak activity. The first X-class flare of the current solar cycle occurred on Feb. 15, 2011 and there have been 15 X-class flares total in this cycle, including this one. The largest X-class flare in this cycle was an X6.9 on Aug. 9, 2011. This is the 7th X-class flare in 2012 with the largest being an X5.4 flare on March 7.

This flare did not have an associated Earth-directed coronal mass ejection (CME), another solar phenomenon that can send solar particles into space and affect electronic systems in satellites and on Earth.

Updates will be provided as needed.



Related Links

› Related multimedia from NASA Goddard's Scientific Visualization Studio

What is a solar flare? What is a CME?

For answers to this and other space weather questions, please visit the Spaceweather Frequently Asked Questions page.


 
 
Karen C. Fox
NASA's Goddard Space Flight Center, Greenbelt, Md.