Friday, 13 July 2012

Sunspot AR 1520 releases a powerful Solar Flare.

On Thursday 12 July 2012 at 4.52 pm GMT, NASA's Solar Dynamics Observatory witnessed a sunspot labeled AR 1520 (Active Region 1520), currently facing towards the Earth, produce one of the largest Solar Flares so far this year. This has been classed as an X1.4-class flare, potentially large enough to cause disruption to communications networks and electricity supplies on Earth, though in this case highly unlikely to do so. The flare caused the release of a coronal mass ejection (stream of plasma) that is traveling towards us at 1400 km per second, and will reach the Earth on Saturday 14 July, at about 5.00 am, GMT. This is likely to produce some spectacular auroras in the polar regions, but not to cause any serious harm.

An X1.4 class flare erupted from the center of the sun, peaking on 12 July 2012 at 4.52 GMT. It erupted from Active Region 1520 which rotated into view on July 6. NASA/Solar Dynamics Observatory/Atmospheric Imaging Assembly.

Sunspots are magnetic storms on the face of the Sun. These inhibit convection currents in the Sun's photosphere, causing localized cooling; the surface of the Sun can drop from its usual 5778 K to as low as 3000 K in a Sunspot, causing them to darken compared to the rest of the Sun (though they are in fact still pretty bright). Since Sunspots are magnetic they have magnetic poles, with positive and negative charges. These can be connected by coronal loops, streams of magnetic flux carrying plasma above the surface of the Sun. This can lead to a short circuit in which a large amount of magnetic energy is released suddenly, producing a brightening we perceive as a Solar Flare.

Image of coronal loops over the eastern limb of the Sun, taken on 29 June 1999 around 2.00 am, GMT. NASA/Transition Region and Coronal Explorer.

This in turn can lead to the release of a coronal mass ejection, a stream of charged particles, mainly electrons and protons but with some ionized atoms of heavier elements such as helium or oxygen. This travels out from the Sun, typically taking about two days to reach the Earth's orbit.

A coronal mass ejection breaking away from the Sun. Universe Today/JAXA/Hinode.

When these streams of charged particles reach the Earth they can cause magnetic storms. These are usually harmless, with the energy being released in spectacular displays of light near the Earth's poles known as the Aurora Borealis (north) and Aurora Australis (south), but occasionally large events cause problems for electrical systems on Earth, such as the March 1989 event that knocked out electrical distribution networks in Quebec (such distribution networks are now generally better safeguarded against these events).

An Aurora Borealis display over Sommarøya in Norway in January 2011. Thilo Bubek/National Geographic.

Aurora displays come in a variety of colours, caused by electrons from the coronal mass ejection striking different atoms in the Earth's atmosphere. This is because the energy of the atoms increases each time it is struck by an electron, but atoms can only absorb so much energy before they must release some, and each atom always releases energy as light (photons) at a specific wavelengths. In the Earth's atmosphere this is effected by altitude, thus Oxygen releases either green or red light and Nitrogen releases either blue or violet light. Typically auroras shimmer as different reactions occur, photographs do not really do them justice.

Gasses release light at specific wavelengths in response to other stimuli besides coronal mass ejections. Thus the blue colour of the daytime sky is the colour of Nitrogen in the lower atmosphere reacting to the (steady) energy input from sunlight, whereas the red colour of sunrises and sunsets is the colour of oxygen higher in the atmosphere reacting to the same; we see this at dawn and dusk because the sun is no longer in line of sight with the lower atmosphere. Neon lights are red because Neon gas releases red light in response to electrical charge, and Sodium lights orange for the same reason. Molecules made up of more than one sort of atom, such as Carbon Dioxide (CO₂), Water (H₂O) or Methane (CH₄) release light in the infra-red part of the spectrum, which can lead to warming of the atmosphere (the Greenhouse Effect), hence the current concerns about the release of such gasses into the atmosphere by industrial processes, and the effect this might have on our climate.

The colours of a sunset are caused by our being able to see the upper atmosphere, once the Sun is out of line of sight with the lower atmosphere. Joe Bauwens.

See also The Earth reaches its aphelionSolar flare may hit Earth on 4 July 2012NASA's Solar Dynamic Observatory observes the transit of VenusComet C/2011 W3 (Lovejoy) survives a close encounter with the sun and Two solar flares coming our way.

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1 comment:

  1. I'm curious where you found the 5:00 GMT estimate, as other sources I've read seem to be pointing to about 5 hours later than this (give or take 7 hours). I'd prefer that your estimate were right, as the other 10:20 GMT estimates would be entering twilight where I'm at, but just wondering if you could verify this estimate please.

    Thanks!

    ReplyDelete