Showing posts with label X-class. Show all posts
Showing posts with label X-class. Show all posts

Friday, May 17, 2013

Sun Slings Four Major X-Class Solar Flares in 48 Hours (Video)



Solar Flare
The past 48 hours has been busy for our sun. The closest star to Earth has hurled a total of four major X-class solar flares into the depths of space as activity amps up for the end of the 2013 solar cycle peak. Four images from NASA's Solar Dynamics Observatory of an X3.2-class flare from late at night on May 13, 2013. (Photo : NASA/SDO)
The past 48 hours has been busy for our sun. The closest star to Earth has hurled a total of four X-class solar flares into the depths of space as activity amps up for the peak of the 11-year solar cycle in 2013.
Solar flares are powerful bursts of radiation that can sling the harmful material through space toward Earth. Fortunately, this radiation cannot pass through our atmosphere to impact humans on the ground. However, it can sometimes disturb the atmosphere enough so that it disrupts radio signals.
Like hurricanes, solar flares are classified based on their intensity. The weakest are known as A-class flares, followed by B, then C and M. The strongest solar flares are labeled X-class flares, and can pose a risk to astronauts and satellites in orbit when aimed directly at Earth. In order to categorize the strength of these flares within their classes, though, researchers also give them numbers. The higher the number, the stronger the flare is.
The first flare occurred on Mother's Day, May 13. A comparatively demure X1.7 flare, it was associated with a coronal mass ejection (CME). This solar phenomenon can send billions of tons of solar particles into space that can reach other planetary bodies days after the initial burst. When directed toward Earth, these CMEs can disrupt satellites and can supercharge the northern lights, creating spectacular displays. In fact, a solar flare that occurred in April did just that, sparking a geomagnetic storm that produced an impressive light show.
The second solar flare that the sun flung into space was a stronger X2.8-class flare, which was also associated with a CME. Experimental NASA models showed that solar particles sped from the sun at a terrific 1,200 miles per second. It was the strongest flare to have occurred all year--until the third flare came along.
The third solar flare occurred on the evening on May 13 and was classified as a X3.2 flare. It's the strongest to have occurred all year and also hurled a CME into space. Fortunately for us, none of these CMEs are Earth-directed, which means that they won't be causing issues with satellites.
The sun wasn't done yet, though. It ejected its fourth and final solar flare in the early morning hours of May 15. The X1-class flare was comparatively tiny to the other ones that the sun had belched out, but it shows that our star is currently more active than it has been in a long while. In fact, NOAA forecasters estimate a 50 percent chance of X-class solar flares and an 80 percent chance of M-class solar flares on May 15, according to spaceweather.com.
"These are spectacular events," said Robert Massey from the UK's Royal Astronomical Society in an interview with BBC News. "An X-class flare is equivalent to a billion hydrogen bombs. We're talking about a colossal amount of energy."
Until the sun reaches its solar peak at the end of 2013, though, we're likely to continue to see these spectacular events into the near future.
Check out the video of the flares, courtesy of NASA.

Tuesday, May 14, 2013

Sun releases another powerful Solar Flare with an X-ray Flux of X2.9 - Largest flare for 2013

Via transients.info

A day later, we have yet another record breaking solar flare for 2013. Yesterday I posted the following entry, 'Sun releases a powerful Solar Flare with an X-ray Flux of X1.8 - Largest flare for 2013' which discussed that subject in question along with information on past strong solar flares.

So is this flare Earth facing? The CME occurred on the west side of the sun, which is rotating towards the Earth. if these strong solar flares continue and as the Sun rotates around and the area they are erupting from faces us, thats when we should be paying a bit more attention.

Credit to spaceweather.com

This is yesterdays X1.8 solar flare above. You can find the animation of the event for yesterday here, http://spaceweather.com/images2013/13may13/xflare_anim2.gif

Credit to spaceweather.com

The above picture shows the location of where the flaring activity started yesterday. 

By my estimation, going by this website here, http://noschese180.wordpress.com/2013/05/06/day-145-how-does-the-sun-rotate/, I expect this area of the Sun where all this activity is occuring, to be fully facing the Earth within five to seven days time. That time frame would be from the 19th of may to the 21st of May.

I am just going to leave it at that for this one. =)

Thursday, October 25, 2012

X1.8 Solar Flare On Oct 22, 7th X Flare of 2012

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.

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 degrees Kelvin, as in a solar flare. The wavelength is typically colorized in teal, as it is here.

(Credit: NASA/SDO/Goddard)

“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

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.
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

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.

Contacts and sources:
Karen C. Fox