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CBC TV And Radio Signals May Be Disrupted By The Sun

The Sun's Power May Disrupt The CBC -- For Real
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On several occasions in the past, intense solar flares from the sun have disrupted broadcast signals here on Earth. Bursts of radiation from the sun have the ability to impact radio communications.

Over the next couple of days, CBC may be experiencing such outages, affecting both radio and television signals.

The electromagnetic interference from the sun is at a heightened level right now due to what is known as a "sun transit" season, which occurs around the equinoxes (these happen two times a year, around March 20 and September 22).

During these "sun transit" seasons, the sun produces high levels of microwave radiation which can overwhelm signals coming from satellite transponders.

When communications satellites travel in front of the sun for a substantial period of time over the course of several days, the signal is likely to be disrupted.

CBC is reporting that the worst of the interference is expected to happen over the next four days, roughly between 3:30 p.m. AT and 3:50 p.m. AT.

Solar Flare Myths Explained
MYTH: Solar flares have no effect on Earth.(01 of09)
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REALITY: Solar flares can release electromagnetic radiation that's strong enough to disrupt electric power grids, satellites, GPS, and radio communications. Pictured: Coronal mass ejection as viewed by the Solar Dynamics Observatory on June 7, 2011. (credit:NASA/SDO)
MYTH: A solar flare could kill us all.(02 of09)
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REALITY: Only a tiny fraction of the energy liberated by a solar flare reaches the Earth, because we're protected by our planet's atmosphere. "We have a very long record that shows that even the strongest flares can't blow out the atmosphere," Antti Pulkkinen, a research scientist at NASA's Goddard Space Flight Center, told CNN.Pictured: A solar eruptive prominence as seen in extreme UV light on March 30, 2010 with Earth superimposed for a sense of scale. (credit:NASA/SDO)
MYTH: Solar flares occur at random.(03 of09)
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REALITY: Solar flares follow an 11-year cycle.Pictured: Full-disk images of the sun's lower corona during solar cycle 23, as it progressed from solar minimum to maximum conditions and back to minimum (upper right). (credit:SOHO/ESA/NASA)
MYTH: 'Aftershocks' are rare.(04 of09)
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REALITY: About one in seven flares is followed by an aftershock -- the flare springs back to life, producing an extra surge of ultraviolet radiation.Pictured: Sunspot 1112, crackling with solar flares, spotted by NASA's Solar Dynamics Observatory on October 16, 2010. (credit:NASA/SDO)
MYTH: Solar flares were discovered only recently.(05 of09)
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REALITY: Solar flares were first observed in 1859 by English astronomer Richard Carrington.Pictured: Sunspots of September 1, 1859 as sketched by Richard Carrington. (credit:Wikimedia: Public Domain)
MYTH: Solar flares are small compared to other explosions in our solar system.(06 of09)
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REALITY: Solar flares are among the biggest explosions in our solar system. "They erupt near sunspots with the force of a hundred million hydrogen bombs," Robert Lin of UC Berkeley's Space Science Lab said in a written statement.Pictured: Solar and Heliospheric Observatory (SOHO) spacecraft image of a solar flare on October 28, 2003. (credit:NASA/SOHO)
MYTH: Solar flares can knock satellites from orbit.(07 of09)
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REALITY: When satellites do fall out of orbit, it's because Earth's gravity is pulling them down.Pictured: Solar Dynamics Observatory (SDO) image of an M7.9 class solar flare on March 13, 2012. (credit:NASA/SDO)
MYTH: Solar flares produce sunspots.(08 of09)
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REALITY: It's actually the other way around. Magnetic fields associated with sunspots -- cool, dark regions of the sun's surface -- can sometimes give rise to solar flares.Pictured: NASA's sun-observing TRACE spacecraft image shows a large sunspot group from September 2000. (credit:NASA/TRACE)
MYTH: Solar flares and solar prominences are different names for the same phenomenon.(09 of09)
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REALITY: Solar flares and prominences are different. A prominence is a loop of plasma traveling along magnetic field lines. Sometimes this loop collapses back into the sun -- or, if the prominence erupts, a solar flare can result.Pictured: A solar prominence on October 19, 2012, captured by NASA's Solar Dynamics Observatory (SDO). (credit:NASA/SDO/Steele Hill)
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