A brief introduction to... Ice Core Records (Part 1)

Bad form, but source: wikipedia

As promised, for today and the next couple of days I will be writing about the ice core records of Greenland and Antarctica. I'll start today with an introduction to ice cores and discuss isotope signals within them. Tomorrow I hope to explain other proxies in the ice cores such as dust, CO2 and methane (CH4) and finish with a post about the controversies surrounding the conclusions based on proxies within the records, with the arguments against the validity of solar forcing (I'll get to that). So, I hope you enjoy exploring the ice core records. I've got some graphs I produced for my course to help explain the concepts, there are some garish colours in there (you have been warned).

Ice cores are simply a core of ice extracted from areas where annual accumulation of snow has resulted in a consistent record of winter precipitation over an extended period of time. These are obtainable from mountain glaciers and the polar ice caps, but I'm only going to focus on the ice caps here as these provide the longest records, and therefore a greater insight into past climates throughout the Quaternary. We know from a previous post that ice accumulation is the result of a greater snow accumulation than summer melt for any given year. Because of this annual accumulation - melt, annual layers are visible within an ice core, with clear layers signifying the melt season and cloudier layers indicating the winter accumulation. We also know that the ice will flow down slope from an ice centre in the form of glaciers. For the purpose of obtaining a complete record, it is very important to take ice cores from areas where lateral movement of ice does not occur, as this would distort or remove some of the record. Ice centres are perfect for this, however in polar regions, they are obviously extremely difficult to get to.

The three most well known ice cores from polar regions are the Vostok and Epica Dome C ice cores from the East Antarctic Ice Sheet, where ice is known to flow extremely slowly in comparison to the West Antarctic Ice Sheet; and the GRIP ice core chronology from Greenland.

I'm going to jump off on a tangent now and start talking about isotopes. Don't get scared, it's a simple concept based on the relationship between the ocean and temperature. As we know, snow is made of water, H20. The H part, hydrogen, normally consists of one proton and one electron. However, an isotope of hydrogen known as Deuterium exists, containing one proton, one electron and one neutron. This neutron effectively doubles the mass of the hydrogen molecule. Still with me? Deuterium is far less common than normal hydrogen on Earth, around 99.98% hydrogen to 0.015% deuterium. So imagine that the ocean is made up of mostly normal water, but a tiny fraction of this water is made with deuterium, and consequently slightly heavier than the rest of the water.

During the colder periods (ie. glacial maxima), there is less energy to evaporate seawater into the atmosphere. Because it takes more energy to evaporate the heavier deuterium water the clouds, and consequently the snow that lands on the ice caps, are made up of a higher ratio of normal water to deuterium water (more than 99.98% to less than 0.015%). Therefore, the ratio of deuterium to normal hydrogen in the snow for that year is less than normal. The opposite is true when temperatures are warmer, with more energy, a greater proportion of deuterium can be evaporated and is deposited on the ice caps as snow. So for warmer years, the deuterium to normal hydrogen ratio is greater than colder years.

Ok, so we're back onto ice cores again. As I mentioned earlier, each years' snow deposition is recorded in a thin band of cloudy ice. This is made up of the ratio of deuterium to hydrogen that was deposited as snow all those years into the past. When we compare these with previous years, we can see that the ratio fluctuates year on year, indicating regional temperature increases and decreases back through time. The Epica Dome C ice core goes back an astonishing 800,000 years and the data extracted from this ice core (and numerous others) is available for free to download as a spreadsheet at ncdc.noaa.gov/paleo/data.html. I find it amazing that the average Joe Public (like me) can download this data and manipulate it, graph it and make their own decisions about the climates of the past. The graph below is exactly that. It shows the deuterium ratio (delta D) for the Epica Dome C ice core. The X axis is age, youngest at the left and oldest at the right, with the deuterium concentration on the Y axis. As you can see, a pattern emerges. Sharp warming events are followed by a gradual cooling to glacial conditions.

Click image for full size

So, you've been introduced to the ice core records and the concept of isotope ratios. The use of oxygen isotope ratios are used in the same way (18O / 16O), but all you really need to know is that water made with oxygen 18 is heavier than the normal water made with oxygen 16, and the ratio of these two are used to indicate temperature in exactly the same way. Tomorrow, I'll discuss the cycles of temperature changes, how they relate to the amount of sunlight the Earth receives. On Thursday we will discuss the other measurable properties of ice cores including CO2, CH4 and dust concentrations, and what they are likely to mean.