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Notes from the Field

Ice Coring Mondays

April 21st, 2020 by Steven Fons/NASA GSFC

The MOSAiC Leg 3 Ice Coring Team. Photo by Calle Schönning.

The main task I am involved with here on MOSAiC is the drilling of sea ice cores. Each week, a group of 10 scientists from the Sea Ice, Ecology, and Biogeochemistry teams goes out to two different “Dark Site” locations on the floe to drill ice cores that will be used in a variety of different experiments back on the ship. We call this large weekly effort “Coring Monday.” Here’s a sense of what this day looks like:

Sunday

Night: Coring Mondays always start the night before with the preparations and packing of the gear. We need lots of equipment: drills (with many, many extra batteries), saws, shovels, core barrels, and storage containers, just to name a few. I am responsible for preparing the data sheets for the next day and working with the team leaders to decide which – and how many – ice cores we will plan to drill. Most coring days we aim for between 30 and 40 cores total from the two sites.

Steven inspecting the blades on a coring barrel prior to packing. Photo by Michael Gutsche.

Monday

07:30: Breakfast time. The whole team generally eats right away in the morning, and makes sure to have enough for the long day in the field. We also pack some food to eat for lunch out on the ice.

08:00: After a quick breakfast, the team meets to load all the coring gear onto the ice floe. Our whole operation requires 4 snowmobiles, each one pulling two 10-foot-long sleds filled with coring equipment. By 9:00, our teams are packed and ready to go. We are joined by two polar bear guards from the logistic team, and set off for the Dark Site. My team heads to the First Year Ice site (FYI) while the other group goes to core at the Second Year Ice (SYI) site. If you’re lucky, you can get a seat on the snowmobile. Otherwise, it’s a long bumpy ride sitting on the wooden sled.

All the gear needed for coring packed onto sleds that are pulled by snowmobiles. Photo by Aleksei Niubom.

09:30: After arriving to the site, our work immediately begins. I start with a snow pit analysis, measuring the depth, temperature, and density of the snow pack. The rest of the team prepares the gear and sets up the 2 working tents and 1 “warming-up” tent.

The FYI coring site. The two tents on the left are for coring and sectioning, while the tent on the right is for warming up and eating lunch. Photo by Steven Fons.

9:45: The ice coring begins. Two people work on drilling the cores, two people examine the drilled cores, note down features, and slice some for later processing; one person works between both groups, transferring the cores and facilitating communication. About half of the cores that are drilled get sliced up in the field into 5- or 10-centimeter sections, while others stay as full cores and get put into 1-meter-long bags. 

The cores are drilled with a hollow barrel that has blades on the bottom and threads around the outside. As the blades cut into the ice, the barrel drills down, filling up the hollow space with a long cylinder of ice. The ice core can then be removed for slicing or packaging.

Steven drilling an ice core. Photo by Laura Wischnewski.

13:00: After a few hours of coring, it’s time for a lunch break. Sandwiches and hot chocolate/tea help keep the energy up! 

Lunch time at the FYI site! Photo by Steven Fons.

13:30: The coring continues. At the FYI site, the ice is typically around 1.7 to 1.8 meters thick at this time of year. This is ice that has grown since the end of last summer. The SYI site, on the other hand, is ice that started growing after two summers ago (hence the name) and did not completely melt at the end of last summer. The SYI, therefore, is generally around 2.2 to 2.6 meters thick. Most of the ecology and biogeochemistry teams’ work is focused on FYI, so more cores are drilled there. The sea ice team is interested in the physical properties of the ice (salinity, temperature, density) and therefore takes an equal number of samples from both sites.

Steven recording notes about an ice core. Photo by Laura Wischnewski.

17:00: After roughly seven hours working in the field, we finally reach the end of our list. We start the clean-up by packing up the sleds and all of our gear, which is more or less the same procedure as the morning. The largest change, however, is that we’ve typically added around 40 meters worth of ice cores, which can weigh a few hundred pounds. 

17:30: We arrive back to the ship to unpack all of the gear and distribute the ice cores to the various teams. 

18:00: What we’re most looking forward to by now: dinner!

19:00: After dinner, the work continues. We need to clean all of the gear that was used during the day, so that it will be suitable to work next week. This means rinsing off the salty seawater from all of the equipment.

Chris (right) and Adam (left) rinse off the coring equipment after a day out on the ice. Photo by Steven Fons.

20:00: Processing begins. Some cores need to be processed the same day, so many of us head to our labs to work on the samples that we drilled. I run some core sections through a centrifuge to remove and analyze the brine, and measure the ice density on other sections.

Steven weighing an ice core section in the -15 degree freezer lab. This is done to calculate the density of each ice core section.

22:00: After a long day of work, it’s finally time for bed. 

The next few days will be filled with more processing of the ice core samples and entering data. Before long, it’s Sunday night and we get to start the process over again. 

MOSAiC Meets ICESat-2

April 7th, 2020 by Steven Fons/NASA GSFC

Robert Ricker (AWI) looking out the window of the helicopter at the sea ice below. Photo by Steven Fons.

One of my scientific objectives while on MOSAiC is to make measurements that will help validate sea ice data collected by NASA’s ICESat-2 satellite. Using a helicopter, a laser, precise GPS coordinates, and some chocolate, we were able to do just that.

On the Morning of March 22, I looked into the upcoming ICESat-2 orbits and noticed that the satellite would be passing almost directly overhead of Polarstern the following day, a little over 24 hours from that moment. This presented a unique opportunity: If we could fly a helicopter (mounted with a laser scanner) directly underneath the ICESat-2 orbit at the exact time that the satellite was passing over, we would effectively have two independent sources of the same measurement – sea ice elevation detected by a laser – taken at the same time over the same sea ice. This method has been done previously during NASA’s Operation IceBridge campaigns, and has proven incredibly useful for validating the ICESat-2 data.

I checked with Robert Ricker, a remote sensing scientist with AWI and the operator of the helicopter-based airborne laser scanner (ALS), to see if this would be possible. He was excited to give it a shot…provided the flying conditions were favorable.

Our view of the inside of the helicopter, featuring Daniel (co-pilot, left) and Harold (pilot, right). The screen is where we monitor our position and the laser scanner operations. Photo by Steven Fons.

When we awoke on March 23, the weather was perfect. There was just one snag: The Captain of Polarstern wanted to ground all helicopter flights so that the ship’s crane could be used to move cargo on board. We quickly jumped in and explained the importance of our flight and just how time-sensitive it is. After a bit of convincing, he agreed to let our flight be the only one of the day.

A little after 12:30 p.m., we took off in the helicopter. Robert was manning the ALS and my eyes were fixed on the GPS, making sure that we stayed on the orbit track. Since ICESat-2 has six beams, we planned to fly beneath the middle two beams, which are spaced 90 meters apart. The footprint of the ALS  is about 300 meters wide, so we aimed to capture both of the middle ICESat-2 beams within the ALS footprint. It sounds easy in theory, with about 100 meters of buffer room on either side. In reality, it was like walking a tightrope. Any slight gust of wind would cause the helicopter to drift off track, prompting Robert or I to inform the pilots to veer slightly back along the orbit. We did our best to stay in line, and after around 45 minutes of flying on the orbit track ICESat-2 passed directly overhead!

A map showing the ICESat-2 beam footprints (6 green lines) and our ALS footprint (light blue swath). The plot is elevation data taken from ICESat-2 along the orbit. Map by Steven Fons, plot by Nathan Kurtz/NASA.

Overall, we flew around 75 nautical miles away from Polarstern along the ICESat-2 orbit before turning around and heading back to the ship the way we came. Of course, we shared a celebratory chocolate bar with the helicopter pilots on the way home. By performing this underflight, we collected valuable data that will not only be used to help validate the ICESat-2 sea ice algorithms, but also will help to scale up the measurements taken on MOSAiC to the larger Arctic sea ice cover.

A lead winds through a web of ridges in the Arctic sea ice pack. Photo by Steven Fons.

Instrument Rescue Operation

April 2nd, 2020 by Steven Fons, NASA GSFC

A helicopter lifts the remote sensing hut to a new location away from the growing ridges. Photo by Eric Brossier.

The leads that formed the last weeks throughout the floe continue to have an impact here on MOSAiC.

The wide lead that split off two sites from the rest of the central observatory started to close again, forming a large ridge that threatened some of the instruments and huts that were out on the ice. Knowing that a storm could re-open the leads or force the ridge to grow even larger, we decided to hold a rescue operation to move any instruments that were too near to the ridge to safer ground.

That morning, the logistics team scouted the ridge and eventually found a safe location to cross it on snowmobile. With the go-ahead from logistics, a large team of almost 20 people headed over to save the instrumentation. It was just in time – one instrument was beginning to be crushed, while others were too close to the ridge for comfort. I was working at the Remote Sensing site, where we employed shovels, snowmobiles, and even a helicopter to move everything to safety.

A ridge growing much too close to the remote sensing hut. Photo by Eric Brossier.

It took all day and a lot of heavy lifting, but we managed to disconnect power lines, dig out sensors that were beginning to be covered by snow, and move all the equipment back away from the ridge. Some sensors that were not working and couldn’t be accessed for a few days because of the lead were able to be returned to near the ship where they could be fixed. The Met city team also had a successful instrument rescue day, saving a 25-meter tall tower that was just a few feet from a lead.

Met city surrounded by (and filled with) ridges. Photo by Markus Frey/BAS.

It’s tough to call today a “success,” since many instruments had to be powered off and many measurements had to be stopped to complete this work. In the long run, however, this action may have saved many sensors from total loss, allowing measurements to continue throughout MOSAiC.

Leads Everywhere

March 20th, 2020 by Steven Fons, NASA GSFC

A lead running beneath Polarstern and through the
MOSAiC floe, captured from a drone. Credit: Manuel Ernst/UFA

In the last post, we took a brief tour of some of the sites that make up MOSAiC. In the days since, much has changed with the MOSAiC floe. Specifically, leads have formed in the ice pack that have altered our floe map and impacted our daily schedules drastically.

Put simply, a lead is just a crack in the ice. It’s never that simple, however. There are many complex processes that determine where and when leads form, how wide they can become, and whether or not they close back up or just re-freeze. Although leads are common features in sea ice and are vitally useful for satellite measurements of sea ice thickness, they still serve as a not-so-gentle reminder that the sea ice can be extremely dynamic, and that we have to be prepared for anything when working out on the ice.

A few days ago, a small crack formed near the ship that was just a few inches wide when it was first noticed. We were still able to go out on the ice, but it was being monitored closely. About an hour later, everyone out on the ice got a radio call from the ship that it was time to return. The crack had grown to a few meters wide, and ran directly under the ship and out in both directions. It continued to widen for a few hours, but luckily this first crack didn’t form under any installations or sensitive instruments. This lead, however, was just the start.

MOSAiC scientists watch the lead grow from the deck of
Polarstern. Credit: Steven Fons

In the next hours and next days, many other leads formed off of that initial crack. Some stayed only 1 meter wide, while others grew to 10 meters or more. Almost all work on the ice has been limited, and the leads are monitored closely. The most critical lead formed between the Central Observatory and two important sites: Met City and the Remote Sensing Site. It shifted the sites a few dozen meters from their previous location, to the point where the power cables had to be disconnected before they snapped.

While the leads themselves pose threats to the instruments and infrastructure on the ice, they are only half of the concern. When (and if) the leads close again, there is a possibility that ridges could form when the two sheets of ice collide together again. Ridges can grow to several meters tall and would crush anything that was caught in the middle. For now, we are keeping an eye on everything that is on the ice in order to limit any impact that the leads or ridges may have. We also keep our fingers crossed that the ice stabilizes soon!

A large (about 3m tall) ridge that formed in the vicinity of Polarstern. The unconsolidated nature of the ice blocks shows that this ridge formed relatively recently. Credit: Steven Fons

The MOSAiC Floe

March 16th, 2020 by Steven Fons, NASA GSFC

The Central Observatory of MOSAiC, with a few prominent landmarks noted. This photo was taken while the Kapitan Dranitsyn was stationed nearby. Credit: Steven Fons

Floe | flō | n. A sheet of floating ice.

Central to the entire MOSAiC Expedition is the MOSAiC Floe: a large sheet of sea ice that was carefully selected back in October as the ideal place to anchor Polarstern for an entire year. It was chosen due to its size, structure (a mix of thick multiyear sea ice and thinner first year sea ice), and forecasted drift trajectory. Over the past five months, it has become a second home for many scientists. Here’s a brief tour of our workplace:

The Central Observatory (CO):
Nearest to Polarstern, the CO is the primary place where measurements are taken, both from continuously operating instruments and from sampling trips off of Polarstern. It houses many installations, from small stakes just a few inches tall, to larger huts and tents that can comfortably fit a few people inside, to 25-meter-tall towers with dozens of instruments installed. Most installations are grouped into ‘cities’ by scientific discipline. There is MET (meteorology) City, Ocean City, Balloon Town (for weather balloons – not clowns), the Remote Sensing Site, and the ROV (Remote Operated Vehicle) Site, to name a few. There are also clean areas dedicated to the sampling of snow, measuring ice strength, and studying biogeochemical processes. 

Throughout the CO, there are carefully placed roads that lead from Polarstern through the Logistics area (where snowmobiles and other gear are parked) and to the different cities. Perhaps most importantly, there is also a ‘trip wire’ alarm around the CO that is able to send up a signal flare if a polar bear walks into it, providing an additional safety measure when out on the ice.

A map of the MOSAiC Floe, focused on the Central Observatory. Credit: AWI

Area II:
Outside of the CO is known as Area II. This mainly houses the “Dark Site” – a place where sea ice cores are taken each week. The Dark Site consists of two different locations from which cores are drilled: a first year ice site and a second year ice site. This area is located far from the lights of Polarstern and kept as dark as possible, so as not to disturb some of the ecological work that is going on. During the winter darkness, anyone visiting the Dark Site had to use a red headlamp, which has been proven to have the least impact on the organisms living below the ice. Due to the distance away from the CO and Polarstern, visiting Area II requires additional preparation and safety gear. My main task on MOSAiC is drilling sea ice cores, so I will venture to Area II at least once per week during leg 3.

The Distributed Network (DN):
Furthest from Polarstern is the Distributed Network, which is home to exclusively autonomous instrumentation. The DN sites are not part of the MOSAiC Floe, but instead range from around 5 kilometers to over 30 kilometers away from Polarstern. Almost all sites require a helicopter to visit, an usually these visits consist of fixing broken instruments or changing batteries. The purpose of the DN is to have measurements far from Polarstern, in order to determine the representativeness of the MOSAiC floe with respect to the ice in the rest of the Central Arctic. 

Together, these areas make up the field sites of MOSAiC. It’s a pretty cool place to work!