On February 15, solar region 1158 produced the strongest solar flare of solar cycle 24 to date, rated X2.2. The flare began at 1:44am (UTC), peaked at
1:56, and ended at 2:06. For 22 minutes radio waves, infrared, visible light, ultraviolet, and x-ray radiation poured out of a cluster of sunspots
covering an area on the surface of the Sun more than 2.5 times the surface area of the Earth.
This burst of electromagnetic energy was produced by complex interactions between conflicting magnetic fields reaching across the region and between
the individual sunspots within it. The energy of a solar flare is not directional. A flare occurring anywhere on the hemisphere of the Sun facing
Earth is "Earth directed".
The energy raced at the speed of light across the solar system in an ever widening hemispherical shell. It arrived at Earth a bit more than 8 minutes
after leaving the Sun. Flashing unaffected through the shell of the magnetosphere, the powerful radio waves were still intense enough to produce a
burst of VHF radio noise on the daylit side of the planet (Asia and Australia) temporarily interfering with communications. The ultraviolet and x-ray
radiation struck the upper atmosphere, ripping electrons from their atoms. This ionization can, if strong enough, cause problems for satellite
communications but it also can strengthen the reflectivity of the ionosphere, allowing ham radio operators in the high frequency bands to communicate
over long distances for a while afterward.
At about the same time the flare occurred and eruption of material from Sun's corona was hurled into space by the same release of magnetic forces
which produced the flare. Unlike the flare, this fast moving cloud of hot ions (plasma) was sent in a particular direction away from the Sun. This CME
(coronal mass ejection) was directed toward Earth. We know this because of the expanding halo of material which can be seen in the coronograph images
from the SOHO satellite which lies on a direct line between the Sun and the Earth. Because the expanding material forms a complete circle, spreading
evenly, the cloud must be moving directly toward us.
Here's a combination of the two.
This wispy cloud of protons and electrons was moving much slower than the energy from the flare which accompanied its creation, taking very close to
three days to reach Earth. By the time the products of the CME reached us they were hardly detectable, notable by mostly by an abrupt increase in the
speed of the solar wind and a rise in its temperature.
So ephemeral was the CME that it has had little effect, causing only slight fluctuations in the Earth's magnetic field, easing worries of those
fearing power failures.
The solar wind maintained a mostly strong north alignment, producing that "balled up" look in the magnetosphere simulator which some get concerned
about. That doesn't mean the magnetosphere is in trouble, it means the magnetosphere is turning its back on the solar wind rather than welcoming it
with open arms. This alignment prevents solar particles from entering the Earth's upper atmosphere, disappointing those hoping for an auroral
display.
To get a better idea of what may be a real cause for concern, here is what a non-wispy CME looks like when it's headed our way. July 14, 2000, the
"Bastille Day Event".
Notice how much denser this CME was than the one from this week. The speckles which appear at the end of the animation are the result of high energy
protons striking the sensor, a "proton storm". The flare associated with this CME was an X5 (much stronger than the recent X2.2). Aurora were visible
as far south as El Paso, Texas. It was a direct hit. We survived.
Region 1158 is now rotating away from our direction so that any future CMEs from it will not impact Earth (on this rotation). But Region 1161 has been
growing a bit and is exhibiting some characteristics which may lead to vigorous activity.
The STEREO B satellite reveals a fairly calm face around the corner. So, barring a burst from 1161, it looks like there may be a lull in activity for
at least 10 to 14 days but it is certain that we will have more opportunities to sit on the edges of our seats.
edit on 2/18/2011 by Phage because: (no reason given)