A year at South Pole - 2017/18

In May 2017, I accepted a job offer at the Wisconsin IceCube Particle Astrophysics Center (WIPAC) in Madison - a job that will send me to the bottom of Earth. IceCube is a giant Neutrino detector at South Pole, and it will be my job to keep its computers running. For an entire year (November 2017 to December 2018) I will live and work at the Amundson-Scott South Pole Station in Antarctica.
Being an IceCube "Winterover" has been my dream job for years - und now the dream is real. This page is my journal of this once-in-a-lifetime adventure.

Most of the content will be in English, but I will also drop some stuff in German occasionally. The journal entries are sorted by date (latest first).

[Go to first journal entry]

[Ice facts only]
[Science facts only]

Map of Antarctica
Map of Antarctica [Polar Geospacial Center]
  • Science facts #3     Askaryan Radio Array (ARA)

The Askaryan Radio Arrary ... pardon me, the Askaryan Radio ARRAY is a sister project of IceCube. Like the Cube, it is also looking for high energy Neutrinos, but instead of optical sensors it utilizes radio antennas to detect our favorite particles. The measurement principle of ARA is based upon the Askaryan effect, which describes the generation of charge anisotropies in bulk media (such as ice) caused by high-energy neutrino induced particle cascades. The anisotropy emits coherent radio waves which can be detected by the ARA antennas.

At the end of this summer season, the experiment will consist of six stations with four holes each, where every hole is holding 4 antennas. Once completed, ARA will cover an area far bigger than IceCube, although with a far smaller detector density. It's neutrino detection sweetspot is at energies even higher than IceCube's, which makes it an important addition to the South Pole Neutrino Club.

  • Science facts #2     IceTop Snow Measurements

If you paid attention in my IceCube facts #1, you might have noticed that IceCube does not only have in-ice optical sensors to measure the neutrinos, but also features some modules right beneath the surface - these are called IceTop stations. Each of the 86 strings that are deployed in the ice has one of them on top. All together, the IceTop stations are used to measure lower-energy neutrinos, and they also serve as a veto-mechanism for the in-ice DOMs.
The problem with stuff that is set up at the surface of South Pole ice plateau: It does not stay at the surface for very long. Things are being burried in snow drift faster than you can say "penguin". Since the amount of snow that covers IceTop has an affect on the measurements, every once in a while the IceCube winterovers have to go out and estimate the snow level on every single IceTop station. This can be a long and cold adventure, depending on the windchill and how many people can be motivated to help. Fortunately, the old winterovers Martin and James were still here (they belong to the handfull of toasty people who are still waiting for a plane to take them back to the real world) to help Johannes and me, so it took us only two afternoons.

  • Science facts #1     The IceCube detector

The IceCube South Pole Neutrino Observatory is a huge particle detector burried in the almost 3000 m thick Antarctic ice sheet at South Pole. IceCube is looking for ultra-high-energy neutrinos. Upon colliding with the atoms of the ice, these tiny particles produce a little flash of blue light. This is called the "Cherenkov effect". The light can be seen by IceCube's thousands of optical sensors, which have been deployed on long chains by drilling deep holes in the ice. The data collected by these sensors is sent to the surface, where it is recorded and forwarded to the Northern hemisphere for analysis.

To get a better idea of IceCube, you can have a look at the picture below (courtesy of the IceCube collaboration) or visit