See, scattered throughout the year, there are really cool things that happen. Such as the first time getting off the plane and seeing Antarctica (definitely had some butterflies in the stomach), standing at the South Pole marker the first time, seeing the last plane leave, seeing the sun go down knowing you wouldn’t see it for 6 months, the beautiful polar night skies, and this Friday the mid-winter mark.

Shoveling out a path to ARO (Atmospheric Research Observatory) just after station closing

And there are still some to come like the sun rising, the first plane landing and taking a flight out of here. So there are all these milestones that are exciting which add up. Yeah, the day-to-day is pretty boring here, but the sum of all the milestones make the entire time down here an amazing experience. That’s what helps me anytime I’m feeling a bit homesick or anxious to move on. And that is what I’m going to remember when I leave in 5 months. (Wait, why am I talking like I’m almost done? Hehe.)

April weather was somewhat significant being the coldest April on record averaging -80.7F which was lower by 0.2F than the previous record set in 1998 (records began in 1957). On top of that, we set the second earliest mark in reaching -100F ever recorded dipping to -100.7F on April 13th. It’s only typical that as soon as April ended, we are on a streak of warm and unsettled weather. For instance, temperatures today are supposed to rise into the -30s Fahrenheit. It’s amazing to me that you can have a range of about -65 degrees without any daily help from the sun. If things keep up, which they look like they will for the near future, we are on pace for the warmest May ever! I wonder what is in store for the rest of the winter?

Taking in the sky from the Atmospheric Research Observatory

The station atmosphere was much quieter however. We only really had only one major event which was a glycol leak in the power plant. The power plant uses a 60/40 glycol to water ratio to cool the diesel generators. The waste heat from the generators transferred to the glycol mix is then run throughout the station to heat the building. My knowledge of how the whole system works is very limited but as I understand it, a thermostat broke open and created a geyser of glycol. It then landed on some of the exhaust manifolds causing it to vaporize and create a huge cloud in the power plant. This triggered the fire alarm. Luckily it wasn’t one of the loops that carry the bulk of the glycol or it could have been a much worse mess. Over the summer, we had so many false alarms that you kind of become desensitized to it always thinking it’s a false alarm. But when you hear the automated alarm system say that smoke was detected in the power plant, and that it’s not a drill, it really gets the adrenaline pumping. As you can imagine, the power plant is one of the locations on station where you could have things really go wrong.

Everyone on station is assigned to an emergency response team and mine is the fire team. Because we are on are own down here, it is our responsibility to deal with these situations. The fire team had some firefighting training back in Denver before we came down Antarctica and we also try to do some training on our own once a week to keep methods fresh. But we are by no means professionals. Needless to say, I was very relieved to find that the power plant was not engulfed in flames and nobody was injured in the incident. The heart rate definitely jumped initially with the thought that I might actually have to go in and drag someone out of a flaming building. We don’t have fire hoses so all we have are fire extinguishers to use on station (there are fixed water and CO2 suppression systems at various locations however). With all the luxuries that the station has, it’s easy to slip into a false sense of security. These types of incidents are reminders that we are still in a dangerous environment.

There are not any traces of the sun on the horizon any more. When the moon is out, it is like a floodlight on the South Pole. It’s amazing how bright it is. It sure makes walking to the observatory every day much easier. Now the moon has gone below the horizon and it’s extremely dark but the stars are incredible. Yesterday walking back from the Atmospheric Research Observatory (ARO), I was lucky enough to see an iridium flare coupled with a really nice aurora. An iridium flare is when the solar panels of a satellite are at just the right angle that it reflects the sun’s light at you. It does it for just a few seconds as it passes overhead. Unfortunately I did not have my camera ready for a photo.

Well that about does it for the update. Seven months down, six to go!

The Final Flight: February 14th, at 2:30am New Zealand time.

We have just barely over two weeks until the sun sets and temperatures are already starting to drop quickly. The day of station closing, temperatures were around -40F. Today it is the coldest since I’ve been here at -63F, and tomorrow it’s suppose to bottom out at almost -70F. It’s amazing how quickly it drops when that sun gets low. The cold temperatures also make everyday things difficult to deal with. We had an emergency response drill today that took place outside and I volunteer on the fire team. You have to be really conscious about your gear because the SCBA (Self Contained Breathing Apparatus) hoses start to freeze and can crack easily. A fire fighter isn’t much good without a working SCBA. Frostbite is a big concern as well. The fire gear gloves and boots are not insulated for cold and do a very poor job of keeping your fingers and toes warm.

South Pole Station from ARO.

As for the science here at ARO (Atmospheric Research Observatory), not too much has changed. I’m still coming out here every day to check to make sure everything us running as it should be and taking air samples in flasks every week. One thing that is starting to change is our ability to do Dobson observations. The Dobson Spectrophotometer is an instrument that uses sunlight to measure total column ozone in the atmosphere. When the sun is this low on the horizon, there is a lot of stray refracted light that affects the measurements and can give us bad results. You may ask, “How do you take measurements in the winter?” Well this is done by using the reflected sunlight off of the moon. So we are able to take sporadic observations to coincide with our balloon flights through the winter. The solar radiation instruments on the roof will be coming down soon after sunset as well, which will be a small project for us. Here is a brief description of the solar radiation measurements we have at ARO and why we are measuring it.

Incoming solar radiation is the backbone of what drives our climate. Changes in the amount of radiation reaching the earth from the sun can be the difference between being in an ice age or not. It is important for us to know how much radiation is a) reaching the surface, b) what type of radiation it is (wavelength), and c) how much is bouncing back off the surface. This is what’s called the “Radiation Budget” in its most basic form. The “Radiation Budget” involves many other processes but the pictures and descriptions below show how we break down the “Radiation Budget” into its basic components at ARO.

The Solar Tracking NIP (Normal Incidence Pyroheliometer)

The NIP tracks the sun in all 360 degrees. It measures direct incoming solar radiation of specific wavelengths.

Diffuse Pyranometer

The diffuse pyranometer blocks out the incoming direct solar radiation and measures any radiation that is getting reflected and refracted from substances in the atmosphere (or any radiation taking an indirect path to the surface).

Pyranometers

These pyranometers detect all incoming solar radiation both direct and indirect. The two outer ones have filters on them to divide it up into shortwave (UV) and longwave (infrared) radiation.

Albedo Instruments

The “Albedo Rack” is basically exactly the same as the pyranometers except that they are turned upside down. They then measure the amount of solar radiation that is reflected off of the earth’s surface. Roughness and color play a role in Albedo meaning that a smooth surface is going to reflect more than a rough surface, and a white surface is going to reflect more than a black surface.. Therefore, it is important not to disturb the snow under these instruments because we want the natural state of the surface. In addition to reflected radiation, it monitors infrared radiation emitted by the earth.

A more complex version of the “Radiation Budget” or “Energy Balance” pulled from the IPCC Fourth Assessment Report.

As you can see, in the above figure, there is a lot that really goes into the “Radiation Budget” and it is a very complex system. When the solar energy comes into the atmosphere, it can take a variety of paths. It can get interrupted by clouds, gases, aerosols and other substances. Two of these processes in the system we observe at ARO as well such as Aerosols, and Greenhouse Gases which I will talk about in a later post.

Hopefully this explains a little bit what’s behind the solar radiation observations that we take at ARO. The South Pole and Mauna Loa have the longest continuous running solar radiation observations of this kind. It’s extremely important that we understand what happens to solar radiation as it passes through the atmosphere and hits the earth’s surface if we want to gain a good understanding of how earth’s climate works. It is even more important as we try to predict future climates.

The previous winter-overs running the Atmospheric Research Observatory, LTJG Marc Weekley and engineer Patrick Cullis (aka Cully), were there to greet me at the ski-way, and help me with my bags. Winter-overs are people who stay on station for the 8-9 long months in which there are no flights into or out of the Pole. Temperatures are just too cold during this period for flights. Many winter-overs like Marc and Cully spend the S. Hemispheric summer months here as well making it a full year. After a few days of turnover with Marc and Cully (who were extremely patient and helpful for having just spent a winter in isolation), I was able to catch up with Marc for an interview on his thoughts, feelings and advice on spending a year at the South Pole.

Photos courtesy of:

Patrick Cullis, all aurora shots
Brian Vasel, the tower with low sun
Emrys Hall, view of ARO from tower
ME, the plain looking shot of the tower