Category Archives: Space Weather

Listening to Coronal Mass Ejections, close to the source

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(photo: Spaceweather.com)

Shortwave radio listeners know that coronal mass ejections (CMEs) often disturbing our SWLing. More than once I’ve been in the middle of listening to a broadcast, or even chatting with a fellow radio amateur on the HF spectrum and the effects from a CME would, in essence, wipe us out.

CMEs, in fact, have been getting a lot of publicity as of late. Now’s your chance to hear whatone sounds like–a little closer to the source:

[The following video] is a sonification of the recent solar storm activity turns data from two spacecraft into sound. It uses measurements from the NASA SOHO spacecraft and the University of Michigan’s Fast Imaging Plasma Spectrometer (FIPS) on NASA’s MESSENGER spacecraft at Mercury. The creator is Robert Alexander, a design science doctoral student at the University of Michigan and NASA fellow.

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Another solar storm headed to Earth

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(photo: Spaceweather.com)

Even the Wall Street Journal picked up on the latest solar flare–the biggest in 5 years–which is headed towards Earth:

WASHINGTON—The largest solar flare in five years is racing toward Earth, threatening to unleash a torrent of charged particles that could disrupt power grids, GPS and airplane flights.[…]

“It’s hitting us right in the nose,” said Joe Kunches, a scientist for the National Oceanic and Atmospheric Administration. He called it the sun’s version of “Super Tuesday.”

The solar storm is likely to last through Friday morning, but the region that erupted can still send more blasts our way, Mr. Kunches said. He said another set of active sunspots is ready to aim at Earth right after this.

But for now, scientists are waiting to see what happens Thursday when the charged particles hit Earth at four million mph. [Continue reading at the WSJ]

And the latest update from Spaceweather:

GEOMAGNETIC STORM UPDATE: A CME propelled toward Earth by this morning’s X5-class solar flare is expected to reach our planet on March 8th at 0625 UT (+/- 7 hr). Analysts at the Goddard Space Weather Lab, who prepared the CME’s forecast track, say the impact could spark a strong-to-severe geomagnetic storm.

Expect some major geomagnetic disturbances and don’t be surprised if the shortwave bands are very quiet while we’re being blasted with electrons. On the plus side? If you live in Northern latitudes, look for some awe-inspiring auroras in the night sky.

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NPR explains space weather and the CME heading our way

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(Source: SpaceWeather.com)

I think this is one of the best, simple explanations of space weather that I’ve seen lately:

(Source: NPR)

Space weather, as it is called, originates with solar magnetic activity. The sun is a giant spinning ball of charged particles. In addition to its spin, the heat released from the core through nuclear fusion eventually sets the upper layers of the sun into a kind of boiling motion called convection. All that motion — spin and convection — means lots of charged particles streaming this way and that. Since current (the flow of charges) produces magnetic fields, the outer domains of the sun are ruled by magnetism. Magnetic fields are the source of all those cool images of giant flares erupting in planet-spanning arcades of super-hot plasma. It’s also the source of so-called Coronal Mass Ejections or CMEs, which are, essentially, the space storms that space weather is all about.

CMEs are eruptions of matter and magnetism from the sun into space. A typical CME will blow 10 billion kilograms (about 22 billion pounds) of solar plasma into space along with enough energy to represent a flotilla of 220 aircraft carriers moving at 500 km/s. The fact the CME’s are quite common says a lot about the power locked up in an ordinary star like the sun.

While 1 to 3 CMEs may occur every day, we only the notice the ones that slam into the Earth on their journey across the solar system. When a CME crosses the Earth it runs into our planet’s own magnetic field. Charged particles from the CME get trapped by the Earth’s magnetic field and stream down toward the planet’s surface near the poles.

When those CME particles, running down magnetic field lines, strike atmospheric gas atoms, the collisions cause the atoms to light up like Christmas tree bulbs. That is the origin of the simmering walls of color we called aurora. There was a time when pretty lights were all there was to space weather. Those days are over.

Read the full article on NPR’s website.

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