Southern Ocean GasEx Blog

Dispatches from the Southern Ocean Gas Exchange Experiment

Archive for March, 2008

ASIS – The Return of Big Bird

Posted by sogasex on March 31, 2008

By Will Drennan, University of Miami

ASIS, the University of Miami’s “Air-Sea Interaction Spar” buoy, was recovered by the Ronald H Brown over a week ago, after a week at sea. The comment most people make when seeing ASIS for the first time is “Wow, that’s big”. At 6 x 2 x 2 m (36 x 6 x 6 ft), and weighing close to a ton, it is indeed one on the larger pieces of kit on the deck. As Mike Rebozo can tell you, it can also be difficult to deploy and recover. While he’s likely lost count of how many times ASIS has gone over the side of various ships over the past decade, the real question is how many of Mike’s grey hairs are a result of ASIS ?

The role of ASIS in SO GasEx is to make measurements at, and close to, the ocean surface. Above the surface, we measure basic meteorological parameters, as well as the air-sea fluxes of CO2, water vapour, heat and momentum. In collaboration with Ian Brooks and Sarah Norris of the University of Leeds, we are also measuring aerosol fluxes and concentrations. At the surface, we measure surface waves and wave slopes at various scales. This is particularly important for gas transfer work, as small scale waves are thought to be significant control on gas transfer rates. Below the water, we measure temperature, salinity and energy dissipation rates (a measure of surface mixing, which acts as a control on gas transfer). There is also one of Mike DeGrandpre’s SAMIs (see Mike’s blog) measuring carbon dioxide, dissolved oxygen, and light (PAR). Finally we also measure how ASIS moves in the water. Equipped with three ARGOS beacons giving position, we wanted to make sure to find it again.

While many of these atmospheric measurements are also made on board the Brown, a ship disturbs the near surface too much to measure many air-sea processes, such as small scale waves. ASIS was designed precisely to fill the need for a platform for such high resolution near-surface measurements. On its previous cruise on the Brown, during Gasex-2001, ASIS was christened “Big Bird”, after its less than graceful flight over the deck during deployments. The bird is still big, but hopefully the flights are becoming more graceful.

asis-deploy-93.jpg

ASIS being deployed

pict3153.jpg

ASIS in the water

Posted in Cruise | Leave a Comment »

Primary Productivity

Posted by sogasex on March 30, 2008

By Veronica Lance, LDEO

If you have been following the science of the Southern Ocean GasEx project, you know that our major goal is to measure and better understand what controls the rates of exhange of carbon dioxide (and other gases) between the atmosphere and the surface ocean. Where do phytoplankton fit into this picture?

Phytoplankon, the microscopic single-celled “plants” of the sea function similarly to terrestrial plants – that is they take up inorganic carbon, then, using the energy of sunlight and an important enzyme (“RuBisCO”) form chemical bonds among carbon atoms leading to the production of simple organic carbon molecules such as carbohydrates. This “fixed” carbon plant material forms the base of the food chain – small metazoans and zooplankton feed on phytoplankton, which in turn feed fishes and marine mammals. In the Southern Ocean, this “food chain” has been found to be quite short and direct as compared with many other ocean environments…. As few as 3 links to the “top”: Diatoms … krill … whales!

Our understanding is, that over geological time scales, the ocean has been acting like a big sponge soaking up some of the high concentrations of atmospheric carbon dioxide during warm periods and perhaps ventilating carbon dioxide out of the oceans back into the atmosphere during cold, glacial periods. In modern times (the “Anthropocene Age”) the ocean has been soaking up some proportion of the huge amounts of carbon released into the atmosphere by the burning of fossil fuels and by other respiration processes accelerated by industrialized methods (for example, large scale agricultural practices). In an imaginary bathtub-in-a-closed-room model ocean, the gases in the atmosphere (room air) will equilibrate with those in the water (bathtub) – that is, the water will absorb the gases until it can absorb no more and the conditions will be steady or stable. If we make now make our bathtub very, very deep and add some phytoplankton, the conditions are no longer stable. The phytoplankton will use up some of that dissolved inorganic carbon. Eventually some of that carbon material (now in organic forms such as dead phytoplankton cells or fecal pellets from animals farther up the food chain or bacterial clusters of decaying matter) will sink very deep and become isolated from the surface waters where it was formed. As the organic carbon disappears from the surface ocean, more carbon dioxide from the atmosphere has a chance to be soaked into the surface ocean. The fate of the sunken carbon is that it could be respired again on a relatively short time scale (geologically speaking, years to hundreds of years) and be circulated back into the surface ocean (for example by upwelling) OR it could be buried into the sediments for relatively long time scales (thousands to hundreds of thousands of years). This process has been given the descriptive phrase “biological pump” (see picture below). 

In 1952, Steeman-Nielsen described the method he developed for estimating organic carbon productivity in the sea using radioactive carbon (14C) as a tracer. In light of the many high-tech methods being used on this cruise, this one feels old-fashioned now – but the beauty and satisfaction of this method is that it pretty much always works! There are some finer details about what this method actually does or does not measure which I am not getting into here, but in a general sense, we can get a good estimate of the rate of net carbon uptake by phytoplankton throughout the depths of the ocean where sunlight penetrates (the “euphotic zone”) on a daily basis in a given water mass (“primary productivity”). These rates will go into the bigger carbon flux equations that the SO GasEx project is all about.

I’m sure my colleagues think I am nuts, but I enjoy doing these incubations. While we are at sea, I see almost every sunrise and many sunsets in all kinds of weather. Some of the scientists aboard collect water samples and bring them back to the lab for analysis. My 14C samples get analyzed “live” and so it is satisfying to be able to walk off the ship at the end of the cruise already knowing something about my observations and being able to start thinking about how they fit into the bigger pictures of the SO GASEX project and the regulation of primary productivity in the Southern Ocean (see Fig. 2 for example of data).

For the SO GasEx project, I do several different kinds of measurements, but I am doing the primary productivity work as a collaboration between my Lamont group (with Bob Vallaincourt and John Marra) and Pete Strutton (aka “bottle cop”) of Oregon State University. Basically, I collect water from the CTD rosette from several representative depths in the ocean into clear, polycarbonate, well-washed bottles. Next, I inoculate the water sample with a small amount of the radiotracer 14C and put the “spiked” jars into the on-deck incubator. The incubator (see pic below) is simply a plexiglass box which contains several tubes which are shaded to imitate light levels at the respective depths of the ocean from where we collected the samples. Seawater is pumped through the box to keep the samples at ambient temperatures. The spiked sample jars go into their respective light tube and there they will stay from dawn to dusk or from dawn to the following dawn (depending on the precise observation desired – I am doing both types on SO GasEx). The community of organisms trapped in the bottle are both “fixing” and respiring carbon – and some of the tracer 14C along with it. At the end of the incubation, the jars are gathered from the incubator and the seawater samples are filtered. The filters collect all the organisms in the jar – some of which have now incorporated some of the radiotracer. The filter goes through a few more procedures and then is placed into a liquid scintillation counter which is a way of determining the disintegration rates and ultimately the amount of the 14C tracer in the sample organisms. With a few more calculations, we end up knowing something about the rate of carbon uptake in the water column. A plot of an early station in SO GasEx is shown below. At the same time, Pete sets up similar dawn-to-dawn incubations using the stable isotope 15N as a tracer to determine the rate of nitrate fixation (perhaps the subject of another blog someday). The ratio of carbon uptake to nitrogen uptake gives us some clues as to how fast the fixed carbon might be sinking into that very deep bathtub ocean. Every morning at 0430, Pete knocks on the door of my rad van where I have been prepping my samples. Together in the pre-dawn greyness, we go out to the incubator to harvest our previous days’ samples and put out the next set (see pics below).

p.s. All this talk about radioactivity might provoke some health and safety concerns. We are concerned, but more for scientific reasons than health or human safety. This is why: First, the amount of radioactivity we work with is very small with respect to human health concerns. Second, humans are not plants, so any 14C tracer to which we might be accidentally exposed is not taken up into our bodies. Third, it is easily washed off of surfaces with a bit of soap and water – which is later properly disposed. Our biggest concern is not to leave any traces of 14C on surfaces of the ship. Why worry about the ship? Because other scientists who use the Ronald H. Brown measure ambient concentrations of carbon isotopes including 14C. Natural 14C concentrations are very low so that even miniscule contaminations, hardly noticed by our scintillation counting methods, could skew the measurements of the natural concentrations. So, out of respect for future science, we go through several steps to insure no radioactive carbon escapes out of our control. Our work is done inside a special container van (“rad van”) placed outside on the deck of the ship (see pic below). We wear special lab coats and booties which remain inside the rad van – it’s kind of like going through an air-lock. The samples which go out to the incubators have a short trip of only a few meters from the van to the incubator and are well-sealed.

vl-1.jpg

The “biological pump” cartoon drawn by Zackary Johnson.

vl-2.jpg

Data! Yippee!

vl-3.jpg

Light tubes in incubator with flowing seawater.

vl-4.jpg

Harvesting an incubation just before sunset.

vl-5.jpg

Pete and I setting out our daily 24-h 14C and 15N sets at dawn.

vl-6.jpg

Rad van being set into place on the deck of the NOAA ship Ronald H. Brown.

vl-7.jpg

At work inside rad van. The red lights are to keep the phytoplankton “asleep” before they go into the incubator for the day.

Thanks to Bruce Hargreaves, Bob Vallaincourt and Paul Schmeider for photos.

Posted in Cruise | Leave a Comment »

L’aventure, c’est l’aventure…

Posted by sogasex on March 29, 2008

By Bertrand Lubac, Naval Research Laboratory

[Après donc Tocqueville et BHL, me voici à mon tour parti à la rencontre des Etats-Unis. Pour ma part, les USA se limitent pour le moment au bâtiment océanographique le Ronald H. Brown, à son équipage et à la trentaine de scientifiques participant à la campagne de mesures SO GasEx. Plus précisément, le noyau dur autour duquel je gravite est l’équipe d’optique marine, appelée aussi dans le cercle des initiés l’équipe « Espuma ». Cette équipe vous a déjà était présentée par Richard Miller, et un de ces membres éminents, Christopher Buonassissi, vous a tout dernièrement fait partager son grand enthousiasme à être de la partie. Aujourd’hui c’est à mon tour de m’allonger sur le divan du blog pour vous raconter dans les grandes lignes les événements qui m’ont conduit jusqu’ici].

The point of departure has been the “Laboratoire d’Océanologie et des Géosciences” in Wimereux, a small seaside resort in the North of the France, where I met Professor Hubert Loisel. This led me to a PhD on the remote sensing of ocean color from 2004 to 2007. The principle of ocean color is to extract information on the biogeochemical and optical parameters of the ocean surface water from a radiometric signal measured by a sensor onboard a satellite. To accomplish this, two general steps are necessary to develop algorithms that relate satellite measurements to in-water information: atmospheric corrections and bio-optical inverse models. My research is mainly focused on the second step (bio-optical inverse models) and has led to a particular study that examines the influence of the marine particles on the variability of remote sensing reflectance, which defines ocean color.

This research topic has now led me to Dr Zhongping Lee. In November 2007, just after my PhD defence, Dr Lee invited me to tour his laboratory, as part of the Naval Research Laboratory (NRL) located at the Stennis Space Center. My first feeling was a mix between astonishment and wonder being faced with such human and material richness combined at NRL. This visit provided us with the opportunity to define a common research project that will be conducted during a postdoctoral fellowship at the University of Southern Mississippi (USM), also located at the Stennis Space Center.

Following this initial journey, there has been a long battle to obtain all the documents necessary to come and work in the USA. Today these administrative steps are almost finished and my postdoc at USM should start at the beginning of May. In the meantime, Zhongping Lee has given me the great chance to take part in the GasEx expedition in order to familiarize me with my new toys such the multispectral volume scattering meter (MVSM) to measure the volume scattering function of the marine particles (see picture below), and get to know the USA research and culture, and to overcome my seasickness.

As some researchers have previously confided in you, there is no marked break between work and rest on the boat. So, when the weather is not too bad and doesn’t force us to remain prostrate in our lab, days go by quickly due to a very busy daily schedule. During the GasEX III cruise, my job is to collect remote sensing reflectance spectra using a handheld spectral radiometer (see picture below), the volume scattering function of surface seawater using the MVSM, and the aerosol optical density using a sunphotometer. With these measurements we hope to improve remote sensing algorithms for primary production and optical properties of the Southern Ocean. In addition to the science, I must in my case add English courses as part of my job. One course in particular with Dr. Richard Miller is teaching me the basics to survive in Mississippi: “how’s it going “ – “Peachy”… But all this work doesn’t enable us to forget what the ship’s rules don’t allow us to have – a cool beer and a tenderness time with our girlfriends that remain at home.

After this cruise, the adventure will go on in Slidell, Louisiana and in Mississippi and I hope the adventure will always be as exciting…

[Et là-bas, on murmure « Tiens bon la rampe ! »].

image-12.jpg

The Multispectral Volume Scattering Meter (MVSM) was developed at the Marine Hydrophysical Institute in Sevastopol, Ukraine (M. E. Lee and M. R. Lewis, 2003). The MVSM performs light scattering measurements at angles going from 0.5° to 179°, with a resolution of 0.3° at eight wavelengths (443, 490, 510, 532, 555, 565, 590, and 620 nm)

image-21.jpg

Remote sensing reflectance measurements made using a handheld spectralradiometer on the ship’s bow

image-3.jpg

Thanks to Scott Freeman for this English version of the French book “Voyage au bout de la nuit”

Posted in Cruise | Leave a Comment »

Disaster!

Posted by sogasex on March 28, 2008

By David Ho, LDEO

Being out at sea requires that we adapt to different situations and adjust our plans accordingly. Some of these adjustments are expected, while others are genuine surprises.

For instance, when we inject the tracer patch, we select an area that is relatively stable so we don’t end up chasing the tracer patch around the Southern Ocean. However, because there’s no guarantee that winds and currents won’t change, we really don’t know where the patch is going to go. As a result, we don’t have fixed survey lines and have to adjust them minute by minute. That’s expected.

During this cruise, we’ve had some surprises. For instance, what happened to the SuperSoar was a surprise (see Burke’s blog), but given the fact that they are pushing the cutting edge of water sampling technology, it’s not difficult to accept that it could happen.

What happened to us today topped that.

It was about 9:00 am, and time for our morning CTD. Paul and I were discussing something in the Hydro Lab and getting ready for sampling when we heard a loud thud. I said to him facetiously, “I hope that wasn’t the CTD going into the screws [the propellers].” I went to the Staging Bay to check things out, and ran into Carlos on the way who said to me with a panicked voice, “we just lost the CTD.”

I once heard an episode of WNYC’s Radio Lab about Stress, where they talked about what happens to us when we’re under stress. One of the common experiences that people under extreme stress has is that time slows down and thoughts become clear and lucid.

In the few steps that it took to get to the Staging Bay, all the different scenarios under which we could have “lost the CTD” crossed my mind. I was expecting to see the end of a frayed cable dangling in front of me; what I saw was more surprising.

The CTD was hanging off the side of the ship, and the block that used to hang from the CTD boom was laying on the deck. See pictures below for what I fail to convey with words. Apparently, the rosette was accidentally pulled into the block, breaking the block and sending the CTD crashing approximately 20 feet into the side of the ship. Disaster!

The good news out of all this is that nobody was hurt and the rosette/CTD package was eventually recovered. However, the rosette frame was severely damaged and eight sample bottles were crushed.

For the 9:00 am station, we adapted and went to our storm contingency plan, when we expected not to be able to deploy the CTD: Submersible pump. Even though the pump only had enough hose and cable to sample down to about 40 m, it was better than nothing. It was a nice sunny day and a communal atmosphere on deck as we took turns sampling water pumped up to the surface.

We’re working hard to put another rosette/CTD package together, but it will not be ready in time for the upcoming 9:00 pm station. This will be another pumped sampling station. We hope to have the CTD ready for the morning station tomorrow.

pict3283.jpg

Damaged rosette/CTD hanging off the side of the ship

pict3284.jpg

The broken block on deck

p1000316.jpg

Recovering the damaged rosette/CTD

pict3292.jpg

Close-up of the damage

pict3291.jpg

Preparing the submersible pump

p1000334.jpg

Sampling from the submersible pump

p1000351.jpg

A new rosette/CTD being assembled in the Staging Bay

UPDATE: Sara, Geoff, Jonathan, Clay, and Bob worked hard all day and assembled a new rosette/CTD in time for the 9 am morning cast the next day. We’re back in business. Nice going!

p1000363.jpg

The newly assembled rosette/CTD package, ready for the next cast

Posted in Cruise | Leave a Comment »

Pump and Dump

Posted by sogasex on March 28, 2008

By Dale Hubbard, Oregon State University

There are approximately 60 people, including the crew and the science party, aboard the Ronald H. Brown. The good folks in the galley serve three meals each day, there are snacks available after hours, and there’s a seemingly unlimited supply of things to drink. This is a very good thing (it certainly beats going hungry and being dehydrated), yet it poses a quandary: once we’ve metabolized all of that food & drink, what to do with all of our waste?

There are basically two types of sewage generated aboard the vessel: grey water, which originates from sinks, showers, laundry, and the dishwasher; and black water, which originates from the toilets. (The engines also generate wastewater of a more industrial nature, e.g. oily waste, but this is contained separately and later pumped ashore when the ship is in port, as oily waste is illegal to discharge at sea.) Aboard the Ronald H. Brown gray water and black water are commingled and contained within a holding tank of approximately 5000 gallons capacity. Sewage aboard the Ronald H. Brown is not treated—it is mechanically ground up en route to the tank, then the contents are pumped overboard. Once the sewage tank has accumulated 4400 gallons, it’s time to break off from our study site and make a run for it.

Since our project involves continuously observing a relatively small patch of water in order to collect time-series measurements, we must move at least 3 nautical miles off-site before the ship evacuates the contents of its sewage tank. Sewage contains an assortment of compounds that serve as phytoplankton nutrients, so dumping the holding tank inside of our study area would drastically alter the biological and chemical processes within. Therefore, at least twice each day we must leave the patch to undertake what many aboard refer to as a “Pump and Dump.”

Unfortunately, several times during the course of a Pump & Dump, the ship’s underway seawater line entrained some of the sewage. This caused caused a great deal of excitement in the lab, as steaming through this particular hydrographic feature generates some of the most dramatic measurements observed during the cruise. This secondary “patch” is exemplified by elevated pCO2 and nitrate (both byproducts of the degradation of metabolic waste) and elevated temperature (see pictures below).

On at least one occasion we’ve been able to resolve a sewage signal in the data from our underway transmissometer, an instrument which essentially measures water clarity (or lack thereof) by passing a beam of light through a sample stream of water. Eeeewwww…

In order to pick these Pump and Dump events out when we’re processing the data long after the cruise is over, it’s important that we remember to log them carefully.

fig-1.png

Effect of “Pump & Dump” on pCO2 and temperature. Pump and dump signal, from approximately 12:00-12:30, manifested in approximately 20 ppm increase in pCO2 (white trace) and approximately 0.5o C increase in surface seawater temperature (red). “H2O” parameter is water vapor measured inside of shipboard pCO2 equilibrator and also reflects higher surface seawater temperature. The surface salinity values are highly variable (and rather irrelevant) because it had been raining.

fig-2.png

Effect of “Pump & Dump” on NO3 concentration. “Amplitude” values represent voltage generated by photodiode detector (note scale is reversed). The ~0.1 V decrease between approximately 12:00 -12:30 represents an approximately 3mM increase in NO3. The variation in amplitude at approximately 13:30 is a standard sequence—a blank, 20 mM, and 9.5 mM KNO3 solutions.

Posted in Cruise | Leave a Comment »

The Importance of Quenching

Posted by sogasex on March 27, 2008

By Bob Vaillancourt, LDEO

The most common measurement to make for a biological oceanographer is for chlorophyll a (abbreviated “Chl a”). This is the pigment that is common to all phytoplankton, so is a convenient proxy for the size of the plant crop in the ocean at a given time. We have two ways of measuring Chl a: by direct measurement of its concentration on discrete water samples captured in a bottle, or indirectly, by measuring the amount of fluorescent light the plants emit.

Fluorescence is a phenomenon by which a material (in this case, Chl a) absorbs light energy, then re-emits a portion of this energy as light at a lower energy. In the case of phytoplankton, their Chl a (and other pigments) absorb energy in the more energetic blue-green portion of the spectrum, and re-emit (or “fluoresce”) in the less energetic red portion. This light is too weak to observe with the human eye, so we use special instrument called fluorometers to measure it.

Typically, we lower a submersible fluorometer over the side of the ship to measure the “vertical profile” of Chl a fluorescence. If we don’t have time to stop the ship, then we can make “underway” measurements by piping surface seawater into the ship’s lab and running it through benchtop fluorometers. We then look at this profile (or time-series) as a “proxy” or suitable substitute, for phytoplankton concentration. As chlorophyll concentration increases, generally so does the level of fluorescence- but not always. So it is important to realize the situations when chlorophyll fluorescence is not a good proxy for concentration. We most often see this in surface waters where light levels are highest.

Figure 1 shows a time series of surface sunlight (upper graph, blue line) measured on the deck of the ship, and Chl a (lower graph, green and black symbols) measured at a depth of 3 meters, near the surface. As sunlight increased throughout the day, we observe a suppression, or “quenching” of Chl a fluorescence by about a factor of nearly two between early morning and mid-afternoon (approx 15:00 GMT). We see this happening on rather short time scales too, as dips in sunlight, perhaps caused by the passing of clouds overhead, cause momentary relaxation of quenching in the fluorescence traces at approximately 1200 and 1700 hrs (red arrows). The Chl a concentration, meanwhile, showed a nearly constant level throughout the day. Quenching of Chl a fluorescence causes a huge departure from the normal co-variation between concentration and fluorescence. But does this happen at all depths?

The next figure shows similar data, but taken on two vertical profiles: one during mid-day (Station 7, left graph), and the other near mid-night (Station 4, right graph). You see that during the daytime, quenching of fluorescence occurs down to about 20 meters depth, and decreases fluorescence by a factor of about ten, when compared to Chl a concentration measurements made on captured samples. During night-time, however (right graph), the Chl a concentration data (green symbols) and Chl a fluorescence track each other nicely.

Another way of viewing these data is by property-property plots (see figure 3). Here we see that when plotted this way, the night-time data show a nice linear relationship (although over a limited range), but the day-time data, corrupted by fluorescence quenching show no such correlation. So, if one were to use the Chl a concentration data to calibrate their chlorophyll fluorometers, it makes sense to use nighttime data only.

image-1.png

Solar Irradiance (upper) and corresponding Chl a (lower) level changes through the day on March 16. Green symbols are concentration values (units of micrograms per liter) and black dots are fluorescence values (units of voltage). As sunlight increases through day, the fluorescence from chlorophyll is quenched, without a corresponding decrease in concentration.

image-2.png

Two vertical profiles of Chla fluorescence (black symbols) and corresponding concentration values (green symbols) for mid-day station 7 (left graph) and mid-night station 4 (right graph). During daytime, Chl a fluorescence in the upper 20 meters is quenched and does not track Chl a concentration. The quenching phenomenon disapears during the night-time.

image-3.png

Property-property plots of Chl a concentration (x-axis) versus Chl a fluorescence (y-axis) for mid-day (black symbols) and mid-night (red symbols) from Figure 2. Night-time fluorescence, devoid of quenching, shows linear relationship to Chl a concentration.

Posted in Cruise | Leave a Comment »

Down The Rabbit Hatch

Posted by sogasex on March 26, 2008

By Christopher Buonassissi, University of Connecticut

I am a graduate student from the University of Connecticut and this is my first long research cruise. While I have been to sea before, this voyage has been particularly interesting. As Chris alluded, the days of the week cease to have much meaning. While I may not be particularly concerned whether it is Friday or Monday, the constant activity does have its advantages. It has provided a great opportunity to interact with scientists from a variety of different fields. These are the people I began graduate school wanting to be like and discussing data and its implications with so many experts has been fascinating. It is remarkable to meet someone and then realize they were the author of a paper that explained a concept or inspired you in your own work. I realized that one of the books that I have used extensively as a resource in my graduate work had been written by one of the scientists onboard. To actually be working with and learning from him and many others has been an immensely enriching experience. Another aspect of being a graduate student is my inexperience deploying instruments from large ships. Some of the science team has accumulated years of sea time; I arrived with around two weeks and none of it in the conditions we have experienced on this cruise. So while hand lowering the buoy (see description below) certainly seems simple, in 15 foot waves it can get rather dicey. Being able to receive advice from people who have deployed instruments in similar situations is invaluable.

One of my responsibilities on this cruise is to deploy the Hyperspectral Tethered Spectral Radiometer Buoy (HTSRB) or the buoy for short. This buoy is a collection of instruments that measure the amount of light at many wavelengths. There is one sensor that detects the amount of light hitting the surface of the ocean and three that are underwater to measure the amount of light coming up towards the surface. We can measure how the light field changes in the upper few meters of the water column and also determine the light that a satellite overhead detects. These data will allow us to determine how bubble injection by waves affects light in the ocean and how it impacts the signal that satellites detect. This is particularly important in high wind areas such as our current study area. The buoy has also proven popular with the local wildlife. We have frequent visits from the penguins and birds in our neck of the ocean. The animals seem to be checking out this strange object bobbing about in their seas and contemplating how best to eat it. While their contemplations make for a great photo op, some of the albatross are a bit too eager in their inspections (photos below). My initial fears were allayed as the birds only cause minor damage by picking out a few bits of foam from the buoy’s floatation collar. Such are the perils of science on the high seas.

buonassissi-1.jpg

Birds on the stalk

buonassissi-2.jpg

An albatross swoops in for a peck (for a sense of how large these birds are the yellow float is roughly a foot across)

buonassissi-3.jpg

The results of a ferocious albatross assault

Posted in Cruise | Leave a Comment »

Chalk Talk Part Deux, The Revenge

Posted by sogasex on March 25, 2008

By Dave Drapeau, Bigelow Laboratory for Ocean Sciences

Since a lot of you have probably been wondering since my last entry (see Chalk Talk) “How does he figure out how much calcium carbonate is in the water?” I figured I’d talk a little about the instruments we use for this. Most of our sampling uses the ships ‘Uncontaminated Seawater line’ which is has an outlet in most of the labs aboard. This is constantly pumping seawater from about 10 feet below the surface (we call it surface water because it’s very difficult to sample closer to the top without occasionally sucking in air, especially in an area where 10’ waves are the ‘little’ ones). So instead of putting our instruments in the water, several of us (Burke, Steve, Roberta, Matt, Bob, and myself) are bringing the water to our instruments, using this constant stream of surface water to map various properties as the ship steams around both inside and to and from the ‘patch’.

Our system (see picture below) starts with some basic oceanographic measurements like temperature, salinity and chlorophyll fluorescence. Then the water passes by an instrument which measures amount of optical backscatter from particles in the water. The reason we can estimate the amount of calcite in the surface ocean from satellites is because these particles reflect a lot of light. After the instrument gets a good idea of the amount of total backscatter in a sample a computer turns on a pump which adds a weak acid into the seawater stream. Just like a TUMS after dinner will get rid of your indigestion, any calcite in the water will dissolve as we drop the pH and the amount of backscattered light will decrease. We look at the difference in the backscattering at normal and low pH to determine what we call the ‘acid labile backscattering’. The computers which collect all the data are also connected to the ships navigation system which allows every data point to have a time and position to go with it.

We combine this continuous flow-thru measurement with water samples we filter and analyze for particulate calcium back at the lab. One assumption (generally true) we make is that all of the particulate calcium we see in our analysis is bound to carbon as calcite (CaCO3, aka calcium carbonate, aka chalk). This represents the amount of Particulate Inorganic Carbon (PIC) in the water as opposed to the carbon tied up in the cellular material of plants and animals which is labeled as POC, or organic carbon. This can be an important distinction as I mentioned in the previous blog because of the different fates of these two types of ‘fixed’ carbon in the ocean.

So is there a lot of PIC in the surface waters of the Southern Ocean???

Remember that satellite imagery showed what appeared to be a large band of high calcite surface water in the circumpolar area (see first blog), but that there were several possible explanations including whitecaps and bubbles from the constant high winds down here. Well, the unofficial answer is yes. Preliminary results show substantial amounts of PIC in surface waters both along the transect from Punta Arenas to the study site and in the study sites themselves (see picture below). The data need to be looked at more closely and correlated with chemical analyses so don’t tell anyone, yet, but the implication of these findings suggest that the Southern Ocean could represent one of the largest pools of marine PIC on earth making it even more important to study the fluxes of carbon between the ocean and atmosphere and how they might be changing.

I’d like to send a ‘Shout Out’ to Mrs. Jones’ 3rd grade class at Boothbay Region Elementary School. You guys have kept me busy with all the great questions and it’s been fun telling you about the cruise. And finally, Happy 7th Birthday to Henry Drapeau! I miss you buddy and wish I could be there.

image-1.jpg

Where the ‘Magic’ happens. Underway temperature, salinity, chlorophyll fluorescence, and total and acid labile optical backscattering.

image-2.jpg

The percentage of acid labile backscattering over the area of the first ‘patch’. Values greater than 0.1 (10%) are generally considered significant.

Posted in Cruise | Leave a Comment »

The Limey’s Lament

Posted by sogasex on March 24, 2008

By Steve Archer, Plymouth Marine Laboratory

Us Brits are always talking about the weather, so here goes:

Mercury, that’s what the sea looks like today in the sunshine, albeit fast moving mercury. Somehow the cold makes it look even more metallic. The weather’s very ‘British’ in this part of the world, changing by the hour, four seasons in one day, ‘don’t forget your brolly’; that sort of weather. What’s driving this? At the moment we are sandwiched between a low pressure system tracking around the Southern Ocean and a high pressure system that has drifted east, off Argentina. This has compressed the isobars, increased the pressure gradient and we had some quite high winds last night, getting into the 35 knots region for sustained periods. Ideal for sea-to-air flux measurements. Interestingly to me, the increased wind and deteriorating weather at the time, coincided with rising barometric pressure; not something that happens in Britain very often. The southerly wind dropped the temperatures and made sampling the 11 pm CTD a f’f’f’f’freezing-fingers experience. Today’s sunshine made it feel less cold at 11 am.

How cloudy it is may be determined to some extent, by the cocktail of gases produced by the microbial biology in the surface oceans. Byron and I are interested in DMS a sulphur gas that may promote cloud formation (see earlier blogs: here and here). Other organic gases may also contribute to our changing weather. A substance called isoprene, is thought to be produced in large amounts by phytoplankton off the Patagonian coast, possibly enhancing cloud formation in this region. Forests produce isoprene and it’s responsible for the blue in scenic views, hence the Blue Ridge Mountains. Iodine-containing compounds may also help create clouds and importantly organic-iodine compounds produced in the oceans are transported onto the continents where life, including us before we added iodine to our table-salt, requires it. It’s obviously important to understand these links between ocean biology and the weather but tying the two together is tricky. The gases produced by the ocean biology here, today, will probably have more impact on the weather 1000s of miles east of us. Hopefully, not before England have beaten New Zealand in the cricket.

Here’s a joke for Maddy and Nicky, and their Welsh mum back in snow-bound Britain: Why don’t penguins come to Britain? Because they are scared of Wales!

metallic-sea-scaled.jpg

Today’s metallic seas

cimg0436-scaled.jpg

Contrasting water sampling conditions last night

11amctd-scaled.jpg

and this morning..

Posted in Cruise | Leave a Comment »

Cinnamon Toast Crunch and Vegemite

Posted by sogasex on March 23, 2008

By David Ho, LDEO

As Chris mentioned in his blog, life on a ship basically consists of working, sleeping, house of pain, and eating. Breakfast, lunch, dinner are served at 7 am, 11:30 am, and 4:30 pm, respectively. Because we eat dinner so early, those of us who stay up late to sample the 11 pm CTD are usually roaming the ship by about 9 or 10 pm trawling for any edible morsel of food. This search inevitably leads us to the mess.

Since we both sit in the Computer Lab when we work, Pete Strutton (aka Crikey) and I usually go on these missions together. His and my choices for late night snacks are Vegemite and Cinnamon Toast Crunch, respectively. In fact, we use those words interchangeably to signal that it’s snack time.

In a big step for US-Australia relations, Pete has been seen eating Cinnamon Toast Crunch and I had my first (and second) Vegemite sandwich recently. It wasn’t too bad, although Carlos Del Castillo, who tried it a while ago said, “I honestly don’t know how to feel about it”. For those who don’t know what Vegemite is, I refer you to an excellent article I read a few years ago in the New York Times about Marmite (a similar brown substance that the Brits are addicted to). I think this quote from Marmite’s plant manager captures the essence: “Our research shows that if you haven’t been exposed to it by the time you’re 3, it’s unlikely you’ll like it”

p1000250-scaled.jpg

Pete Strutton, getting ready for a sugar rush

p1000305-scaled.jpg

David Ho, doing his part for US-Australia relations

Posted in Cruise | Leave a Comment »