June 20, 2011
This morning we left Arequipa and the comforts of the tourist trail, driving east across the puna towards the Andes proper. Our route took us along the newly constructed Caraterra Interoceanica – a highway linking the Pacific coast of Peru to ports in Brazil – and up to elevations of 4700 m. Along the way we passed the smoking Volcan Ubinas, Peru’s most active volcano, and the enormous inland sea of Lake Titicaca. As we approached the Cordillera Carabaya, which bounds the puna to the east, the clouds increased and the landscape changed dramatically, from desert to grassland.
In recent weeks, social unrest related to the opening of a gold mine near the city of Puno has resulted in violent protests. Though we were able to avoid Puno as we travelled east, this sort of anti-mining sentiment underlines the importance of obtaining the blessing of locals to carry out our research on their land.
By mid afternoon we arrived in the small town of Crucero, located at 4100 m beneath Laguna Aricoma – our first site. This town is, frankly, a bit grim, consisting of grey concrete houses and rubble streets, and located on a windswept plain below the mountains. Nonetheless, we’ll spend the night here in order to meet with the governor tomorrow. Fingers crossed that he will remember us and grant us permission once again to roam around. To end on a light note, the Cordillera Carabaya happens to be the alpaca centre of the universe, and so there is a high chance that one of these cute fluffy camelids will end up on our dinner plates tonight.
19th June 2011
What a difference a day makes! We’ve said goodbye to the sprawling metropolis of Lima and now are happily settled in Arequipa – the White City. This name refers to the white sillar rock used in the construction of the old colonial city and which is in fact a pyroclastic deposit from the volcanoes towering above us. From our hotel room I can see the massive bell-shaped peak of El Misti (5800 m), the only active volcano of the group, and it’s looking particularly snowy this year. In fact, flying in to Arequipa, I was surprised to see so much cloud. Normally, with this being the dry season, the sky in this desert region is blue and the mountains dry. Perhaps we should prepare for some wet, snowy field work!
Thankfully, nothing has changed at La Casa de Melgar, our Arequipa base, and I dug out my sampling tools from where I’d stashed them last year, a little dusty but in perfect working order. The rest of our gear, due to its incredible weight, is making its way slowly from Lima by road and should be here tomorrow morning. As for Matt, we found him in the airport, looking surprisingly fresh-faced after his red-eye flight, and so our field team is now complete.
We’ll spend the rest of the day organizing our transport and, in the interests of science, sampling the rather incredible local cuisine.
Every field location comes with logistical hurdles, and the Alaska Peninsula is no exception. Weather, wildlife and modes of transport pose the greatest challenges. We are hardly the first scientists to encounter these: Lamont-Doherty Earth Observatory has a long, rich history of collecting seismic data in this region (e.g., Shumagin Seismic Network, which ran for >20 years), and many groups continue to collect geophysical data here today.
The Alaska Peninsula is too rugged and wild for a network of roads, so planes, helicopters or boats are the only transportation options. We opted for planes, which immediately imposed a restriction on the locations of our seismic stations: they must be near airstrips. Happily, the Peninsula is sprinkled with small communities and lodges with airstrips, most of which lie close to the Pacific or Bering coasts rather than in the remote interior. Back in the office before our deployment, we chose the most ideally located airstrips for our stations and connected the dots between them with the most efficient possible flight plans. But, our plans quickly changed once we were in the field. The weather dictates when and where you can fly each day, and it varies dramatically. We have been lucky enough to have several clear days (even saw some blue skies and sunshine!), but other days we have been grounded by weather and wiled away the time indoors at the inn in Nelson Lagoon.
Once we arrive in each location, we need a quiet, safe place to install our equipment and a ride from the airstrip. On both counts, local communities have been unwaveringly helpful and friendly. The two school districts here kindly granted us permission to install our seismic stations at any of their schools, and we also obtained permission to place equipment at various lodges and village offices. Residents volunteered to take our gear and us from the airstrip to our sites. In one town, our pilot made a general plea over the radio: “Is anyone listening on Channel 3? I’m here at the airstrip with scientists who need a ride to the school”. Someone answered immediately and picked us up 5 minutes later.
Many of our sites are in spectacular places near remote lodges or in towns nestled between mountains and the ocean. All of them are home to impressive wild life that poses a risk to our equipment, particularly bears. We can protect the equipment against curious small animals but fully bear-proofing a station for a short (two-month-long) deployment is not feasible. Instead, we hope that placing our stations in villages (rather than in the wild) will provide some protection, but we will also need good luck. Fingers crossed…
18th June 2011 Lima, Peru
Our 2011 field season is underway. After a full day’s travel from New York, we arrived in Lima, the capital of Peru. This sprawling city perched on the edge of the Pacific Ocean is home to more than nine million people and, after Cairo, is the largest desert city in the world. Being winter in the Southern Hemisphere, the Peruvian coast is swamped by fog rolling in off the cold Humboldt Current and the sky over Lima is grey with smog and cloud. It’s surprisingly cool, too. Only the palm trees, cacti, and spectacular Spanish colonial architecture remind you that this is indeed the tropics.
Since our work will focus on detailed mapping and sampling of glacial deposits, we are heavily reliant on high-resolution aerial photographs of the field sites. Therefore, our first port of call this morning was the Instituto Geografico Nacional, a cartographer’s dream where enormous collections of maps and imagery are stored. It’s a spartan building with a distinct military air – a real throwback to more austere times – but the personnel there were very helpful, dutifully returning from store rooms with stacks of black and white photographs for us to peruse. Incidentally, these photos were taken in the 1960s by the United States Air Force and it never ceases to amaze me just how much the has retreated over the past 50 years. Some of the glaciers have vanished.
With that chore done, we’re currently packing (and repacking) our equipment for the next leg of our journey. Tomorrow we fly to Arequipa, Peru’s second city, located at 2300 m at the foot of the famous Volcan Misti. There we’ll meet up with Matt, who’s on his way from Tacoma as I write. Though we’ve been here only a few hours, it’ll be great to leave the coastal smog for the blue skies of the Andes.
May 22: The 2011 field season has been a very very successful year, in fact the most successful one we have ever had. The weather has been great, the equipment proved to be mostly reliable, the people have been great and the samples are plenty. In the month to come, we will analyze the water samples and eventually end up with a tremendous amount of very exciting data. Thanks to everyone who made this happen.
We left Alert yesterday and are on our way back home. We are stranded in Kangerlussuaq, Greenland, for a couple of days until the Air National Guard can take us and our valuable freight back to the U.S.
The Switchyard Team.
We decide today is the last day for our camp, and we pack up and drive back to our base camp, the Central Transantarctic Mountain camp (CTAM). A sadness in a way, because it was our cozy home for a week. We ate, slept, and joked around here night after night. Also, we realize that packing up camp represents the end of the field season, except for one more day. For the last day of work we will fly by helicopter to the Achernar area from the CTAM camp.
The last day at Mount Achernar. We use the helicopter to go near the southernmost part of the area, near the Lewis ice tongue, which comes off the East Antarctic ice sheet. After a long day, we collect our last samples, and wait for the helo to pick us up – the end of the field work for this season. We realize we had a very successful field season. Not one day of work was lost at either Mt Howe or Mt Achernar (a very rare experience for Antarctica). We think about how we accomplished our goals in terms of getting to both remote sites and collecting samples.
Back at CTAM camp, we scramble to get all our stuff packed up ready to be shipped back to McMurdo. They are closing the CTAM camp for scientific work in a week because they need to take everything down by the middle of February. The middle of February represents the end of the field work for everyone in Antarctica. It starts to get too cold, and the sun starts setting in some areas farther north. People start to go home then and McMurdo gets ready for the winter.
We all fly back to McMurdo. A bed and running toilets (!) for the first time since we left for our camping trips. Also, the dorms have dark curtains that go over the windows. So, darkness, a bed, and a toilet – who would have known life can get so good!
Mike Kaplan (Lamont)
We set out on the snowmobiles with all the sleds to Mount Achernar with all our stuff. After about three hours we reach the site (crossing the flagged crevasse zone with no problem). We are joined by a fifth team member, Tim Flood, a Professor at St. Norbert College in Wisconsin. Tim has expertise in petrology or rock composition. So, we will have one additional person for the Achernar part of the trip.
At first we only find ‘blue ice’ to set up camp. Blue ice gets its name mainly because – in contrast to the typical situation of having a layer of snow on top of the ice sheet – there is only ice. The snow layer that normally covers the top of the ice sheet is blown away where the winds blow pretty fast and consistently. This means there is no good place for camp right in the Achernar area because all the blue ice is a sign of strong winds. We decide to back up a few miles to where the snow starts again and camp a little but away from Mount Achernar. This means we will have a ‘daily commute’ to get to where we want to work, but at least we have a nice place to live for the week. It is less windy where we decide to set up camp and a nice layer of snow in which to pitch the tents and walk around. Blue ice is very difficult to walk on – it is just what it sounds like – walking on ice!
We set up camp. Unlike at Mount Howe, here each person will have their own tent. In addition, we set up the bathroom tent and a huge kitchen tent, named the ‘Arctic oven.’ The arctic oven will act as a kitchen and dining area. It is about 25 feet long, enough to be comfortable. And, when we have two stoves going inside, the temperature gets up to a comfortable 60 degrees or even higher (hence, its name); comfortable enough to start peeling off all our jackets while eating. Two little speakers that Tim picked up in an airport, attached to ipods, means we even have a stereo system in the arctic oven cook tent.
The first day we drive out to where we want to work. It takes about an hour and a half each way by snowmobile. This is quite a bit of time. In addition, the glacier deposits we want to study are much larger in area compared to at our first site at Mount Howe. It is not practical for us to drive everywhere and get to all the places by walking. We realize we will need to utilize the helicopter from nearby CTAM. So, the next week or so we alternate: a “snowmobile day” when we commute by snowmobile from camp to the field site and “helo days”. On the helo days, the helicopter flies out to our camp (a short flight by helicopter from the CTAM camp) picks us up, takes us exactly where we want to go around Mount Achernar, and then at the end of the day, comes back out to bring us back to our camp. All these trips only take the helicopter folks about 75 minutes in total each day, given how fast they go.
We spend the next 8 days or so doing the same sort of work as at our first site Mount Howe. We map the glacier deposits (how red or oxidized are they – how do their elevations changes? How do the deposits themselves change in terms of shape and composition and other characteristics?). Mike K and Mike R (with occasional assistance from others) collect samples for the surface exposure dating, so they can eventually figure out how old all the deposits are. Kathy, Nicole and Tim study the composition and types of glacier rocks and sediments left behind.
Similar to our finding at Mt Howe, we find pronounced changes in the glacier moraine deposits around Mt Achernar. This indicates there are likely deposits of different ages, left behind at different times by the ice sheet when it was bigger. All the team members continue to collect samples that will be analyzed later in the lab.
Mike K, Kathy, Mike R, Nicole and Tim
We are back at the CTAM (Central Trans Antarctic Mountain) camp.
Over the last several days we take stock in that we accomplished the first major goal of our trip. That is, to study the glacier deposits at Mount Howe, the southernmost rock outcrop on Earth. We found (what we think are) deposits left behind by the ice sheet when it was bigger, at several different time periods in recent Earth’s history. We can tell in a preliminary way, before we have carried out the laboratory work back home, that the glacier deposits must be of different ages because they are different ‘colors’ – red for more oxidized (rusted). They also show other signs of varying in age such as the weathering of the rocks and landforms, which increases away from the ice sheet (=older). This means that there will be a record of the glacier leaving behind different types of rocks over a period of time, likely well before the last ice age. It was an important goal to find such deposits for our sampling.
We quickly regroup our stuff over the next few days at the CTAM camp and start to get ready for the next major camp move, to Mount Achernar. For this stage of our trip, which is only about 25 kilometers from the CTAM camp, we are hoping to get there by snowmobile. We will use 4 snowmobiles pulling 6 sleds (two snowmobiles will pull two sleds each). This will allow us to move our entire camp, set it up for more than a week near the site, work, and then come back to CTAM after 8 days or so. However, there is a small problem. There is a crevasse shear zone in the ice sheet between the CTAM camp and Mount Achernar. So, we must figure out where to cross the crevasse zone. We do this two ways. First, we take a helicopter trip from CTAM for an hour (they are quick) to scope out or reconnaissance the area (a “reconn”). On the helicopter, we think we figure out where we might be able to cross the crevasse zone. The helicopter trip also allows us to see the whole area of Mt Achernar and where we want to camp. Camp ideally has to be on a snow patch so we can stake the tents down and in a spot not too windy.
The second way we figure out how to cross the crevasse zone is to go to it, by snowmobile on just a day trip from CTAM (another “reconn”). Mike R (Roberts), our mountain guide, shows us how to link the snowmobiles by ropes, in case one falls into a crevasse. We also put on climbing harnesses and rope ourselves to a second set of ropes between the snowmobiles. This is so that if we fall in, we can either climb out or be pulled out by others.
We get to the crevasse zone which starts at about 15 miles from the CTAM camp. The first few crevasses seem quite bad – each about 2 to 5 feet cross. Although they all seem to have natural ‘snow bridges’ that cross the top of the crevasse, which we can drive across, we need to be confident that they will not collapse due to the weight of the machine. Mike R slowly investigates each crevasse we cross to see how strong the overlying snow bridges are and how wide each crevasse is. After about an hour, we start thinking maybe there are just too many crevasses (every few hundred feet we are finding another one) and it would take too long to figure out how to get across the entire crevasse zone. Mike R suggests we park and get off the snowmobiles, link up with ropes and slowly walk for a while to see how much longer the bad crevasses continue. This seems easier at the moment then stopping and starting the snowmobiles every time we reach another crevasse. To our surprise, the crevasses quickly get smaller and disappear just as we start walking! We did it ! We found a reasonable and quick way to get across the crevasse zone which is less than a 1 mile wide at its bad part. We put flags next to each one so that we can easily see where they are when we come back through on the way to Mount Achernar site to do our work.
Mike Kaplan, Kathy Licht, Nicole Bader and Mike Roberts
The first day of geologic work at our Mt Howe field camp. We start walking on the moraines (piles of debris left by a glacier, just like around NY, Indiana, Wisconsin, where we are from) and we have to put on crampons. These are spikes that go on the bottom of our boots. This is because the moraines are really hummocky to walk on and right under just a few inches of dirt is ice, making us slip and slide and do more leg splits than we can remember!
But, we quickly identify roughly where we think the ice was during the last ice age. We can do this because the deposits are ‘grey’ in color as they do not have time to oxidize (like rust on a car). The stuff left behind by older ice ages is red in color – because it has had time to oxidize. We start collecting our first samples. Kathy and Nicole collect material to figure out the type and chemistry of the glacier deposits left behind, which will help tell them which way the ice must have been moving in the past and what kind of rocks it brought up from below. Mike K and Mike R start measuring the elevations of all the glacial deposits and more important start collecting samples from the tops of large boulders. These samples will help us figure out the time at which they were left behind. Once back home, we will use a method called cosmogenic surface exposure dating. We will use our lab facilities at Lamont-Doherty Earth Obsservatory to date the rocks, using the cosmogenic nuclides Beryllium-10 as well as Helium-3.
Over the next 6 days or so, both teams just systematically collect samples from each set of ridges or moraines that the ice sheet left behind in the past. The idea is that each distinct moraine ridge represents a different time period or glacial period when the ice sheet was bigger. The weather holds up well, an important fact when you are only a couple hundred miles from the South Pole. The temperature remains about -10 to 0 during the day. Anytime the wind picks up thought, the wind chills causes it to get colder fast. Often exposed skin has to be covered quickly. Only a few days are cloudy, otherwise the sun adds a little bit more warmth. Fortunately, the tents are warmer, especially when we run the coleman stoves. So, eating dinner is way more comfortable than being outside.
Mike K., Mike R., Kathy and Nicole
We fly from McMurdo to our first base camp, named CTAM, which stands for Central Transantarctic Mountains. This camp is set up by the US National Science Foundation every 5 to 10 years, with input from scientists on the cutting edge research that can be done in the region where it is set up. An idea for having the camp is to make central Antarctica more accessible every once in awhile to scientists who want to carry out research in remote parts of the continent, such as our team. Otherwise, many of these areas are too hard to get to from the larger more permanent bases and camps such as McMurdo.
Here we will gather all our things, organize our gear for the final time, and then go to our remote ‘deep’ field sites to work. This is the third largest camp on the Antarctic continent this season, and is helping various science teams carry out research, such as in biology and on fossils, geology, and on the ice sheet (for example, how it flows). The camp allows teams such as ours to reach by helicopter and twin otter plane more remote locations this year in central Antarctica, which is normally very difficult.
First, Kathy and Mike R fly to the first of our major camps, at Mount Howe. The next day, Mike K and Nicole fly.
We use a twin otter plane to take all of our gear, including a snow mobile, and only two people can go at a time. The trip takes about two hours each way. This is the first time Mike K and Nicole really get to see Antarctica. The flight is one of those unique experiences of a lifetime as we fly over the mountains high enough to poke through the Antarctic ice sheet. Upon arriving, camp is set up (fortunately Mike and Kathy get much of this done the first day), including two three Scott tents and a mountain tent. One Scott tent is our bathroom – one of the most important tents to go up! Mike K’s tent will act as a dining room and kitchen.
Using a GPS, we figure out the South Pole is only 184 miles from our camp. Less than 3 hours if we are driving on an interstate in the US.
Mike, Kathy and Nicole
We survived Happy Camper survival school! This is essential training for anyone who goes into the field on the coldest most remote continent on Earth. Kathy took hers 4 years ago. We learn to build snow trenches for survival and all things related to camping in the cold, although we still appreciate that it is warmer here than back home (in the 30s, dry and sunny). Also, everyone goes through snowmobile basic repair and use, rock climbing 101, and crevasse rescue training.
Tomorrow is the last day before flying out to the remote CTAM (central Transantarctic Mountains) camp that we will use a base for getting to Mt Howe and Mt Achernar. Mike Roberts, our mountaineering guide, uses the last day to give one more crevasse-rescue training course.
We learned how to stop a fall down a steep slope, set up rescue systems and traversed around an ice fall to learn to recognize and avoid crevasses. Upon our return, we found out that our flight will be delayed a day. Very typical for Antarctica!
Mike and Nicole
It’s great to be back on this amazing continent. I certainly never tire of the beauty of this place. Well, I wouldn’t call McMurdo a beautiful place, but it is buzzing with activity and provides great support for the scientists. Things are much the same here as 4 years ago when I was last on the ice. Dozens of science groups work out of McMurdo station, which acts as a hub of activity for a wide range of scientists, including geologists, biologists, glaciologists and atmospheric scientists.
Many groups, like ours, utilize McMurdo as a place to organize field gear for camping trips to distant sites on the continent to collect samples. Others groups stay in McMurdo to conduct experiments on samples collected nearby. All the science groups have small offices and some work on high tech equipment here in the Crary Lab. This is an amazing resource, particularly in terms of support staff who really work hard to help us out.
An exciting new addition to the local scenery is the small group of windmills erected to generate power for this energy hungry place. My understanding is that this effort was led by the New Zealanders, whose base (Scott Base) in only about a mile away. Luckily, the international cooperation between the NZ and US Antarctic programs means that McMurdo is benefitting from this great ‘green’ experiment in power generation.
McMurdo station rests on the South West tip of Ross Island, which is dominated by the active volcano, Mt. Erebus. As a current resident of the rather flat state of Indiana, I take pleasure in temporarily living on the flanks of a volcano rising more than 12,000 ft above sea level, with its nearly perpetual puff of smoke at the summit.
Kathy Licht, IUPUI
We left Christchurch in the rain – the last we will see for awhile! After a 5 hour flight on a US air force plane, we land on the McMurdo Ice Shelf.
We get off the plane in Antarctica – and – it is beautiful – in the 30s (Fahrenheit) sunny and dry. When it is this dry and sunny, it is light jacket weather. Some people are working around in short sleeves and fleeces. Just like the weather in New York (as family tells me on email the next day), and significantly warmer than the weather in Wisconsin (where Nicole came from). This is Mike Kaplan and Nicole’s first time here, but Mike Roberts and Kathy have been here before.
The planes land on snow, which is groomed with a special compacting machine so that a normal plane can land and take off on the snow.
The next 10 days are for packing, coordinating, and most important, taking safety classes of all types, including the most important – happy camper. Nicole and Mike need to do a two day/1 night class where we camp outside, learn about all the camping equipment, and show we can deal with the elements, before they send us out into the unknown. We also need snow mobile school, helicopter safety school, environmental safety and awareness, crevasse training, and on and on…With all the gear and packing to put together, including food, this will take well over a week before we can even think of leaving McMurdo and heading out to the next stage and field work.
Most of our time is getting our gear together, making wood ‘rock boxes’ (see photo) for storing our geologic samples after we collect them, choosing our tents, food, and other things we are taking. We need to make sure we have two of many things, such as stoves, for safety. Just planning our food for when we are working takes all afternoon and half the evening.
Mike K and Nicole are also starting to learn their way around McMurdo Sound, which is a really interesting place. It is like a small town with a library, general store, three gyms, a coffee shop and wine bar. We all room in dormitories like we are students again. Of course, Kathy and Mike R are old hats here. McMurdo is the base for the United States Antarctic Program (USAP). During out time here, we can see planes and helicopters coming and going, as they take supplies and scientists to various places, including the South Pole. We all eat in one big cafeteria for everyone, buffet style. Fortunately, for Mike K, they are two ice cream machines, in case one breaks down!
Kathy and Mike
After months of waiting, we leave Los Angeles on a non stop 12 hour flight to New Zealand. We ‘are’ Mike Kaplan at Lamont Doherty, Kathy Licht a professor at Indiana University-Purdue University Indianapolis, and Nicole Bader a student from St. Norbert College in Wisconsin. Nicole is finishing her undergraduate at St. Norbert but will be doing her Master’s thesis research with Kathy starting in the fall. Her project will focus on what we do in Antarctica.
It is hot and humid when we landed in Auckland. We went through customs and had the customary 15 minute walk to the domestic terminal. We noticed the heat and humidity not just because we just came from the ‘winter’ in the United States, but we are soon to go to the coldest part of the planet.
We stayed in Christchurch a day. This is to get our gear at the CDC (clothing distribution center). All the extreme cold weather clothing is issued here. We try things on, ask for more (and more!) clothing, and pack everything for our trip. We wait, and walk around Christchurch, including their beautiful Botanical Gardens, have a great Thai meal – knowing thesis will be the last of such sights and greenery (and hay fever!) we will see for a month. We also meet Mike Roberts here, a New Zealander originally, who is our mountaineering guide and new companion. He will be an integral part of our field season and our team and we are happy to meet him finally.
Mike, Kathy and Nicole
The annual American Geophysical Union (AGU) meeting is an all-you-can-eat buffet of the most current scientific knowledge available on the planet. Name your pleasure: space, climate change, geomagnetism, nonlinear geophysics, volcanology, biogeosciences, etc. You have to be careful to indulge in moderation over the five-day event, or risk unseemly bloating.
The Columbia Water Center contributed its own tasty dishes to the feast, mostly under the hydrology section of the menu. (but enough of the food analogies)
Several CWC scientists and affiliated researchers gave talks at this year’s event, December 13 – 17, in San Francisco, and several more had posters representing their work on display. The CWC contribution drew heavily on our research projects in India, but also explored other water issues. Detailed slideshows and posters, along with videos (some filmed in dark presentation rooms) are available on a web page devoted to CWC at AGU 2010.
Upmanu Lall started the week with a presentation called ‘Why is it Flooding Everywhere this Year? Coincidence or a Predictable Climate Phenomenon, and How Can We Respond?’ Without going into the technical material here, Lall concluded that a project on understanding and predicting global flood and drought patterns could facilitate flood risk management and climate change adaptation activities. These would benefit local, state and national planners, and also corporations and financial industries such as insurance.
Shama Perveen and Naresh Devineni are working on a project to develop an in-depth assessment of the growing water shortages in India, as discussed in an earlier post by Perveen. At AGU she spoke about ‘Quantifying the Dimensions of Water Crisis in India: Spatial Water Deficits and Storage Requirements’. Preveen showed a series of diagrams that demonstrated the rapidly falling Indian groundwater levels, population pressure and agricultural demands. Devineni followed up with a look at the water storage capacity in different parts of India, relating them to crop water requirements. This work will help Indian policy makers decide which crops can be grown in each geographic region to maximize food production while minimizing water use.
PhD student Ram Fishman addressed ‘How Low Can It Go? – Scenarios for the Future of Water Tables and Groundwater Irrigated Agriculture in India’, which looked at the relationship between energy use, water use and agricultural production, and their combined effect on the water table. He also presented a poster, ‘Does Irrigation Buffer Agriculture from Climatic Variability – Evidence from India’, which further elaborates on this research.
Tobias Siegfried offered five posters, which ranged from water stress and conflict in Central Asia to groundwater sustainability in India, to climate change impacts in the western US.
Chandra Krishnamurthy, Christina Karamperidou and visiting professor Francesco Cioffi also used posters to explain their research projects, and IRI’s Paul Block gave a presentation on ‘Statistical Dynamical Climate Predictions to Guide Water Resources in Ethiopia’.
Lall then finished up the week with two more presentations. One, ‘Will Hydrologists Learn from the World Around Them?’, was a critique of climate research that doesn’t adequately address the issues of bias in modeling.
In the other, ‘Exploring Oceanic Source Regions and Moisture Transport of Extreme Floods over Large Basins in the Contiguous United States’, Lall talked about the statistical analysis of atmospheric moisture circulation patterns, which may be able to help predict large flooding events in specific geographical regions.
As a group, the work presented was a significant contribution to the AGU meeting, which gave all the researchers the opportunity to interact with scientists in related fields, and keep increasing our collective knowledge and understanding of critical global climate and water issues.
Next year’s AGU feast may be even more lavish….
Columbia Water Center AGU 2010 resources page here.
A major factor in predicting future climate change and its impact on the planet is the response of the Earth’s ice sheets to warming temperatures. Understanding the historical context and dynamics of Antarctica’s massive ice sheets is critical for modeling future changes that have the potential to impact the globe, including significant contributions to sea level rise.
Michael Kaplan and Gisela Winckler, two climate scientists from Columbia University’s Lamont-Doherty Earth Observatory, along with Kathy Licht and Jeff Swope from Indiana University-Purdue University Indianapolis, have recently started a new project, funded by the National Science Foundation, to study the timing and extent of advances of the East Antarctic ice sheet in the past. Integrating field work, geochemical analyses and cutting-edge isotope-based dating tools will allow the scientists to develop a record of fluctuations in the East Antarctic ice sheet and to identify past changes in both ice sheet flow direction and bedrock composition.
On December 13th, Kathy Licht and Mike Kaplan, along with Tim Flood and undergraduate Nicole Bader, both from St. Norbert College, left for their exciting trip to the East Antarctic plateau to collect samples to address these research objectives. Their route will take them via Christchurch, New Zealand, to the Antarctic station McMurdo and on to the East Antarctic ice sheet. It will take them about two weeks to get to the field site.
Accompanied by mountaineer Mike Roberts, they will work from two remote field camps at the edge of the Transantarctic Mountains. The satellite image shows the study region with the major outlet glaciers from East Antarctica crossing the Transantarctic Mountains and flowing northeastward into the Ross Ice Shelf and West Antarctic Ice Sheet. The sites noted in purple will be the location of the two small field camps where the group will be collecting samples. The blue star shows the location of a large field camp, which will be the jumping off point for transport to the smaller camps. The green and yellow dots show the locations of samples collected during two previous expeditions to the region. Over the course of a month, the team will sample boulders and glacial sediments that have accumulated on the ice sheet surface over thousands of years.
Kathy and Mike will report from their adventurous trip on this blog while I will facilitate communication with the field camp and answer questions about the laboratory side of the project.
If you have any questions or comments, please feel free to ask. I will field questions and send them over to Antarctica from where Kathy and Mike will, whenever possible, send back answers.
Stay tuned for exciting dispatches from Antarctica.
If climate change proceeds apace, summer sea ice in the Arctic is projected to nearly disappear by the end of this century. But a group of researchers predicts that ice will continue to collect in one small area, perhaps providing a last-ditch stand for ringed seals, polar bears and other creatures that cannot live without it. The findings were presented yesterday at a heavily attended press conference put on by the American Geophysical Union by polar oceanographers Stephanie Pfirman and Robert Newton of Lamont-Doherty Earth Observatory, along with colleagues from Alaska and Canada.
Studies of ice formation patterns, water currents, winds and the arrangement of arctic land masses has led the scientists to project that even as summer sea ice nearly disappears from the northern ocean by about 2050, floes will continue to pile up and persist along the northern flanks of the Canadian Archipelago and Greenland. This region is currently clogged with heavy ice, some of it drifting in from as far away as Siberia.
“We wanted to look at the tail end–what will happen after the arctic moves to largely ice-free state?” said Pfirman. “Where will the [last] ice be located? If it collects in one area, it could maintain a sea-ice ecosystem for decades.” Brendan Kelly, a polar biologist with the National Oceanic and Atmospheric Administration in Juneau, Alaska, explored the ecological implications, but cited potential problems, including declines in the snow cover needed by seals, and the genetic dangers of having declining populations of rare creatures crammed into shrinking areas. Bruno Tremblay, a climatologist and oceanographer at McGill University, in Montreal, ran an animation showing the shrinkage of warm-season sea ice in the recent past, and a projection into the future . The scientists said that sea ice will continue to cover the ocean in the winter for the foreseeable future–but that arctic creatures need the ice during warmer seasons as well to breed and eat.
Newton said that if there is to be a remnant area, the “first step” is to identify where it might be. With this information, a wide community of governments and native peoples would then at least have information available to consider whether or how to manage such a place in the face of shipping, oil exploration, tourism and other activities that are expected to increase as the arctic becomes more accessible. “We’re hoping to provoke this conversation,” said Newton.
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The 125 million people of the Caribbean/Gulf of Mexico region are highly exposed to hurricanes, floods and landslides–and it is not only because of bad weather. Increasing numbers of the poor are crowding into confined areas that are most prone to destruction–low-lying flood plains, too-steep hillsides, and the like. Robert Chen, director of the Center for International Earth Science Information Network (CIESIN), will describe this alarming trend in an AGU talk on Friday, the last day of the meeting.
CIESIN specializes in creating maps that show humans’ interaction with the natural environment. Ones for this region show deadly combinations of poverty and physical vulnerability to weather. (Blues signal low numbers; greens moderate; yellow to red, progressively more.) Hotspots are clustered across Cuba, Haiti, the Dominican Republic and Jamaica. Along the coast of Latin America are wide swaths of danger spanning Colombia, Costa Rica, Nicaragua, Honduras, Guatemala and Mexico. Not surprisingly, low-lying parts of Texas, Louisiana and southern Florida also stand out.
Many scientists believe climate change will worsen extremes of weather. The CIESIN research suggest that even if this never happens, as the population of dangerous areas grows, these hotspots will continue to get more dangerous.
All day long a flood of thousands scientists and students ebbs and flows across San Francisco’s 4th Street and Howard Avenue, coursing between the cavernous Moscone West and Moscone South convention buildings. The AGU is like a supercomputer of earth science, with human currents of data swapping information, heading from one talk to another, processing what they’ve heard, who they’ve met, what’s coming next.
What’s coming next in New York City, sooner or later, is a long dry spell, according to research by Lamont-Doherty’s Neil Pederson. The city has seen repeated shortages of water over the past 20 years — even though the climate has been relatively wet over the past few decades, and despite a decline in overall water use. Pederson says the water system emergencies of recent years suggest that “maybe the system is not in tune with the climate.”
Ultimately, he said in a talk today at AGU, New York City “is not prepared for the next significant drought.”
Pederson and his colleagues looked at 12 species of trees along the Hudson River Valley and, combined with research by Ed Cook, director of Lamont’s Lamont’s Tree Ring Lab, and others, constructed a record of rain and drought going back into the 1500s. There are still a few trees around who’ve seen four or more centuries pass, Pederson said, including on in the Hudson Valley dating to the early 1500s. Additional records researched by Cook come from the beams cut for now-historic homes built in the 18th century, Pederson added.
The use of 12 species has expanded the accuracy of the chronology, Pederson believes, though it’s hard to gauge by how much just yet. He found that the region has suffered severe droughts in every century through the 1800s. But except for a short period in the 1960s, the dry periods over the past 120 years have been relatively minor. Is the New York City region due for another paleo-scale drought?
David Walker, a professor of geochemistry at Lamont-Doherty Earth Observatory, will be honored tonight by colleagues at the American Geophysical Union for decades of groundbreaking work to understand the early formation of the moon and Earth. Walker will receive the AGU’s Harry H. Hess Medal, awarded for “outstanding achievements in research of the constitution and evolution of Earth and other planets.”
Walker began his career as a student at Harvard University in the late 1960s and early 1970s, as samples of the moon were being returned by the Apollo space missions. Walker was into experimental petrology, a field in which lab scientists try to re-create and understand the conditions under which natural rocks form. With the aid of the moon samples, Walker helped helped piece together much of the story of lunar history accepted today. “Much of what we now take for granted about the formation of the lunar crust and mantle came out of the Harvard experimental petrology lab in the 1970s, clearly with Dave Walker’s intellectual stamp on it,” said Carl B. Agee, a planetary geologist at the University of New Mexico who wrote the citation for the award.
After coming to Lamont a few years later, Walker began working on questions about Earth, including its early separation into chemically distinct layers, and the genesis of magmas that flow out at mid-ocean ridges to form the seafloors. He is currently working on experimental studies to elucidate the formation of earth’s core, and its interaction with the overlying mantle.
Walker also played a key role in developing devices that could duplicate the extreme high-pressure conditions found deep within planets, simplifying designs so that any decent machine shop could turn out the equipment cheaply. “Walker-type” anvils, used to compress experimental solutions to these extreme pressures, are now standard in labs across the world.
Along the way, Walker also has found time to become a popular teacher who has helped students explore topics as diverse as alternative energy sources; radioactive waste, and mineralogy. Agee wrote that Walker “is a true leader in experimental petrology, in both designing and improving experimental equipment, and pioneering new ideas of the evolution of the Earth, Moon and planets.”