Friday

Survived the darkest day



Yesterday december 21st was the winter equinox, which translates to the darkest day of the year. Doesnt mean a lot in most places around the world but here in Icealand we are talking about darkness, since our little island is creeping real close to the north pole. This adds up to about 4 hours of daylight, from 11-15 and the chances of seeing the sun are slim.

I was fortunate enough to see the sun yesterday on my way to work, that is right before a hail storm hit the highway and I ended up going about 40kmh since the visibility was none.

here is another picture of the sun around these parts in winter



This brings me to another fascinating part of living next door to santa claus is this ...



Just the other night i was peeking out my window in the city and saw the most amazing northern lights. The color waves were just ripping through the atmosphere at blazing speeds. I dont remember ever seeing such a site. Wish I had a good camera with me to capture this. I have a feeling that santa is going to give me one this year :)



some wikipedia info for those who have no idea what causes this masterpiece

Auroral Mechanism

Auroras are now known to be caused by the collision of charged particles (e.g. electrons), found in the magnetosphere, with atoms in the Earth's upper atmosphere (at altitudes above 80 km). These charged particles are typically energized to levels between 1 thousand and 15 thousand electronvolts and, as they collide with atoms of gases in the atmosphere, the atoms become energized. Shortly afterwards, the atoms emit their gained energy as light (see Fluorescence). Light emitted by the Aurora tends to be dominated by emissions from atomic oxygen, resulting in a greenish glow (at a wavelength of 557.7 nm) and - especially at lower energy levels and at higher altitudes - the dark-red glow (at 630.0 nm of wavelength). Both of these represent forbidden transitions of electrons of atomic oxygen that, in absence of newer collisions, persist for a long time and account for the slow brightening and fading (0.5-1 s) of auroral rays. Many other colors - especially those emitted by atomic and molecular nitrogen (blue and purple, respectively)[1] - can also be observed. These, however, vary much faster and reveal the true dynamic nature of auroras.
As well as visible light, auroras emit infrared (NIR and IR) and ultraviolet (UV) rays as well as X-rays (e.g. as observed by the Polar spacecraft). While the visible light emissions of auroras can easily be seen on Earth, the UV and X-ray emissions are best seen from space, as the Earth's atmosphere tends to absorb and attenuate these emissions.

finding some upsides of winter
mar