The NASA FSG folks and the rest of the science crew on the US Repeat Hydrography P16S field campaign have experienced some weather delays, which can be expected when working the Southern Ocean close in time to the Southern Hemisphere winter. They encountered 45-knot winds (~51 miles per hour) sitting on top of their planned sampling area at around 60 degrees South latitude. For the safety of all they could not conduct science under those conditions. So they traveled ~200 miles north to escape the weather and then returned southward once the weather had settled. Below you will see some freeze frame clips from the movie Joaquin Chaves captured showing the large swells and the dramatic gray skies of the Southern Ocean. The movie was recorded through the porthole, safe inside the ship.
Stormy weather 1
Stormy weather 2
Stormy weather 3
Stormy weather 4
In spite of the rough weather, the FSG fellows have taken advantage of some calmer days to deploy a radiometer. A radiometer measures apparent optical properties or AOPs. You might recall from Blog #2 that we discussed Inherent Optical Properties or IOPS that characterize the absorption and scattering (reflecting) of light by dissolved and particulate materials in the water. The measurement of IOPs can be done at any time day or night. AOPs on the other hand must be measured during the daytime, preferable when there are clear skies and the sun is directly overhead. AOPs describe how the light is entering and exiting the water column. Remember that sunlight contains a whole spectrum of colors that are determined by their wavelength. We see what is called the “visible spectrum” like what is in the image below.
As the sunlight penetrates the water column, some of the light is absorbed, some is scattered (reflected) backward toward the sky and the rest is scattered forward into the depths of the ocean. Water itself absorbs most of the red light, so we never really see a red ocean (unless there is something unusual in the water).
The character of the light that is reflected back out of the water can be different than what went in. More specifically, the wavelengths or colors that are reflected back out are the colors that were not absorbed or scattered forward. Think about when you are at the beach, say Ocean City, MD or Rehoboth Beach, Delaware. The water typically looks brown or green, right? This is because particles, including both algae and sediment (and water), are absorbing all of the blue and red light, and the leftover colors of brown and green are reflected back out. Conversely, for those of you who have seen blue water in places like the Caribbean or around Bermuda, the circumstances are different. There are very few particles or phytoplankton in the water to absorb the blue light like in the coastal water. Therefore, that blue color is reflected back out , which is why the water looks so blue and pretty. A radiometer that the FSG is deploying on this field campaign measures the colors and amount of the light entering and exiting the water column. The radiometer is hand deployed and, I can tell you, it’s a lot of work!
Joaquin and Scott preparing to deploy the radiometer Photo credit: Isabella Rosso
Dropping the radiometer into the water Photo credit: Scott Freeman
Joaquin guiding the cable; Photo credit Isabella Rosso
Mike pulling the radiometer back to the surface
Satellite instruments, such as SeaWiFS (no longer operational) and MODIS-Aqua (operational) measures this light just like the radiometer so that we can get beautiful images that you can see below.
True color image of Chesapeake Bay http://oceancolor.gsfc.nasa.gov
True color image of Hawaii http://oceancolor.gsfc.nasa.gov
Our FSG fellas are working very hard during this field campaign. But every now and then you need to have a little fun. Mike Novak sent this picture of a snowman that was built on the bow of the ship. I think the eyes, nose, and buttons are raisins.
ACKNOWLEDGEMENTS: NASA’s Ocean Ecology Laboratory Field Support Group is participating in the US Repeat Hydrography, P16S field campaign under the auspices of the International Global Ocean Ship-Based Hydrographic Investigations Program (GO-SHIP). The US Climate Variability and Predictability Program (CLIVAR), NOAA and the NSF sponsor this campaign.
As many of you probably heard, there was an 8.2-magnitude earthquake off the coast of Northern Chile on Tuesday night. As with any earthquake around a coastal region or on the ocean floor, there is great concern about the formation of a tsunami. A Tsunami is series of waves with a very large wavelength. Think of a series of waves hitting a beach. The distance between each wave hitting the shore is the wavelength. Now picture a wavelength that is 100s of miles long! Because the wavelengths are so long, the waves travel at very high speeds, around 600 miles per hour, in the deep ocean. This is the speed at which a commercial jet plane travels! However, the wave height (the height from the base of the wave at the water line to the top of the wave) is very small, maybe a few feet tall. As you can imagine, a boat or ship in the open ocean wouldn’t even notice such a tiny wave.
Below is a screen shot from a CNN video report about the earthquake. In this video you can see how the waves propagate out from the source of the earthquake out into the ocean (red arrow).
The story changes, however, when the depth of the ocean decreases, such as when approaching land. All of that energy in that fast wave gets slowed down and subsequently the height of the wave gets bigger, and sea level near shore can rise at least 50 feet! Thankfully, our colleagues are out of harms way from tsunamis because they are in the middle of the deep, open ocean.
The ship and its inhabitants ARE, however, subject to waves that are created by storms and strong winds. Joaquin made a video of the wave action that you can see below. Here are some freeze frame ‘action shots’ from the video.
And, lastly, I thought it would be good to show some pictures of how cold it is that far south and how challenging it can be to work outside on deck in the cold. In this picture you can see icicles hanging off the ship during recovery of an IOP package deployment.
Water intrusion during recovery of the IOP package
Mike and Scott are having a conversation as they wait for the IOP package to return to the surface of the ocean. I wonder what they are talking about???
A very intense conversation ensues while waiting for the IOP package to return to the ocean surface
You can watch an entire IOP deployment below.
Lastly, when working so close to the continent of Antarctica, there must be a sighting of an iceberg.
At approximately 60° South and 174° East the FSG members sampled their first official station of the field campaign. The solid red line in the map below denotes the current ship track (as of March 27th). The ship has not yet reached the P16S line that begins at 150° West (the blue circles on the map below).
The FSG will deploy an IOP package at one station each day. The FSG IOP package is an assemblage of instruments that collect data for temperature, salinity, depth, absorption of particles and dissolved components, and particle scattering. The instruments are contained within a metal ‘cage’ that is lowered on a wire to a chosen depth in the water column. The data collected by the instruments are saved to a type of hard drive located within the cage. Before the cage can be deployed, weight must be added so that it can sink.
Adding weight to the IOP cage
Here, the cage with all of the instruments is being lifted off the deck of the ship and lowered into the water.
Deploying the IOP package off the side of the ship
And, sometimes, King Neptune decides to send a wave your way. But that is why we wear our safety gear!
Scott catching a wave-It’s all part of the job
The FSG also collects surface water samples in conjunction with the IOP package deployment. A weighted tube is lowered over the side of the ship, and a large peristaltic pump gently transfers seawater to a large container (carboy).
Lowering tubing over the side of the ship to collect surface water
Joaquin filling a carboy with surface water pumped off the side of the ship
The water is filtered and processed back in the laboratory on the ship.
Now, let’s take a moment to understand the significance and importance of hydrographic field campaigns. Oceanic and atmospheric processes are tightly coupled. Temperature and freshwater fluxes between the ocean and atmosphere are in control of climate variability. A good example of this strong ocean-atmosphere relationship is El Nino Southern Oscillation or ENSO. During an El Nino event, the temperature structure of the equatorial Pacific Ocean is disrupted. The central equatorial Pacific Ocean becomes warmer than normal affecting tropical rainfall in Indonesia and global weather patterns. The objective of the Climate Variability and Predictability of the ocean-atmosphere system, or CLIVAR, program is to understand this dynamic coupling and model future ocean-atmosphere variability by collecting and analyzing ship-based global observations. The International CLIVAR program is a continuation of its predecessors: the Tropical-Ocean Global Atmosphere (TOGA) and the World Ocean Circulation Experiment (WOCE). The TOGA program was formed in 1985 to study the relationship between the tropical ocean and the global atmosphere with the ultimate goal of predicting variability on various time scales. The WOCE program began in 1990 with the objective to study global ocean circulation and its relationship to the global climate system over long time scales using global observations. The US-CLIVAR program contributes to the international program as well as the World Climate Research Program. You can learn more about the US-CLIVAR program here.
The guys are finally on their way! The R/V Nathaniel B. Palmer set sail from Hobart, Tasmania on March 20, 2014 ( GMT +11 hours). The science party is made up of a total 29 scientists, 9 of which are graduate students. The first Go-SHIP station is located at 67°S, 150°W. While in transit, scientists will deploy the first Bio-Argo float of the campaign, 6 days from sail. An Argo float is a battery-operated, autonomous float that can move up and down the water column collecting temperature and salinity profiles up to a 2000m depth by pumping fluid into and out of a bladder to manipulate buoyancy. A Bio-Argo can collect measurements of chlorophyll-a and backscattering, in addition to salinity and temperature profiles. The deployment of Bio-Argo floats is particularly important for validating ocean color remote sensing data. For more information about Argo floats, you can proceed to the following links:
Setting up a scientific laboratory on a ship is no easy task. Space is usually limited and you must be able to play well with others. We have filtration equipment (the large wooden frames) set up to collect the biogeochemical parameters, i.e. phytoplankton pigments, particulate organic carbon and particle absorption. The parameters are collected onto small paper filters and frozen for future analyses back at NASA Goddard. We also have two instruments set up on board to measure colored dissolved organic matter (CDOM), which is like tea, compounds extracted from plant material that can flow out into the ocean via rivers. While in transit to the first station Mike, Joaquin and Scott are busy collecting samples.
Mike Novak filtering samples
Particles on a filter pad
Joaquin Chaves preparing samples for storage
A major addition to this year’s field campaign is a ‘souped-up’ underway-sampling system built by none other than Scott Freeman, our optics expert on board the Palmer. The set-up contains multiple instruments that collect dissolved and particulate absorption, CDOM fluorometry, chlorophyll and particle scattering at 660nm. The system is connected to the ship’s seawater system that pumps clean seawater from <10m depth through the ship and then to faucets at which the water can be accessed. The term ‘clean’ means the plumbing that facilitates seawater pumping to the laboratories is routinely checked for clogs and algae growth.
Scott Freeman and the underway sampling system
Lastly, a blog post isn’t complete without a gratuitous photo of macrofauna. Here is a photo of a petrel taken by Joaquin Chaves. Can anyone identify what kind of petrel this is?
Three members of the Ocean Ecology Laboratory’s Field Support Group (FSG; Code 616) will embark on a 45-day journey from Hobart, Tasmania to Papeete, Tahiti on the icebreaker R/V Nathaniel B. Palmer (NBP). The field campaign is part of the US Repeat Hydrography, P16S, 2014 under the auspices of GO-SHIP and sponsored by the US Climate Variability and Predictability Program (CLIVAR). You can find more information about the program here. The FSG will collect biogeochemical samples and bio-optical data across the South Pacific. These data will eventually be ingested into NASA’s SeaWiFS Bio-optical Archive and Storage System (SeaBASS) and subsequently used for ocean color satellite validation activities.
During the next six weeks, I will be helping my colleagues chronicle their journey over the high seas. They will share not only information about the science but also describe the daily life of a sea-going scientist. I, too, participate in many of these campaigns and am very familiar with the NBP having sailed on it three times during my career. Alas, I could not participate in the journey so must live vicariously through my colleagues. Below, you will find the biographies of the three NASA scientists that are participating on this cruise: Joaquin Chaves, Scott Freeman, and Mike Novak. You can also follow the ship track here.
Joaquin Chaves, received his PhD in oceanography from the University of Rhode Island in 2004. For his graduate work he conducted research on estuarine biogeochemistry. He held postdoctoral positions at the Marine Biological Laboratory in Woods Hole, MA, and at Brown University, in RI, where he focused on the biogeochemistry of land use change in tropical forests, particularly in the Amazon region. He’s been a contract scientist at NASA-GSFC since 2009, where he has focused on ocean color satellite remote sensing and marine bio-optics. He has participated in ocean-going field campaigns to the Atlantic, Pacific, and Arctic Oceans, as well as the East China Sea.
A native Californian, Scott Freeman grew up in Salinas, near the Monterey Bay, and attended the University of California, San Diego. After a lengthy hiatus in New York City, he returned to college and received a B.S. in Biology from the City University of New York. He then attended the University of Rhode Island’s Graduate School of Oceanography, completed a master’s degree, and stayed in Rhode Island to work first for the URI, and then for Wetlabs, a manufacturer of oceanographic optical instruments. While in Rhode Island, he participated in many cruises and coastal exercises, including NASA’s Southern Ocean Gas Exchange Experiment (SO GASEX) and ONR’s Radiance in a Dynamic Ocean experiments (RADYO).
Since joining SSAI in 2011, Scott has participated in several field campaigns for NASA’s Ocean Ecology Laboratory, and is responsible for AOP and IOP data collection and processing. He lives in Alexandria, VA with his wife Heidi and sons Charles and Adrian. When not engaged in field research, one can find him playing bass for the Washington Metropolitan Philharmonic Orchestra.
Mike Novak grew up in Piscataway, New Jersey, about 30 miles southwest of Newark. After graduating high school he attended the Richard Stockton College of New Jersey where he earned a B.S. degree in marine science. After college, he attended graduate school at the University of New Hampshire where he earned an M.S. degree in Oceanography. He worked as a researcher at UNH before relocating to the Washington D.C. area where he now works as an oceanographic researcher at NASA-GSFC. When he is not sailing the high seas, he is also an avid musician playing at various venues around the D.C. area with his band Novakaine.