Mary Cook, December 5, 2004

NOAA Teacher at Sea
Mary Cook
Onboard NOAA Ship Ronald H. Brown
December 5, 2004 – January 7, 2005

Mission: Climate Prediction for the Americas
Geographical Area: Chilean Coast
Date: December 2-5, 2004

Personal Log

This afternoon we will board the NOAA Research Vessel RONALD H. BROWN and depart from Arica, Chile and steam westward for the Stratus buoy. I look forward to this adventure with great anticipation and a little trepidation. I’ve never been out to sea for three weeks and can’t help wondering how I will react to this challenging environment. I’ve already met several of the crew and scientists, all of whom have been very cordial and hospitable. I look forward to interviewing them, working with them and just getting to know these incredible people who’ve dedicated themselves to this research effort that will help us better understand the Earth’s systems and benefit mankind in so many ways.

As I reflect upon the last few days since we’ve arrived in Chile, I am overwhelmed by all the wonderful experiences that have been bestowed upon me. First of all, I must mention my mentor Dr. Diane Stanitski. She is a great teacher and a sincere encourager. She is patient yet exudes an energy that’s contagious. Diane has already gained my trust and I look forward to her continued mentoring. Another person with whom I have worked closely is Dr. John Kermond. Dr. Kermond’s the movie-maker. He makes documentaries for NOAA. He’s a very good coach for a novice like me, and a fine tour guide, too. Both he and Diane have put me at ease, modeled proper on-camera techniques and given me advice that’s helped me considerably. I like being their student because I’ve witnessed their expertise and I know they genuinely have a love for this work. What more could a student ask for?

Well, let me tell about some of the sights we’ve seen in the last couple of days while waiting for the cruise to begin. We’re staying at the Hotel Arica. It’s a resort situated right on the beach. I can hear the big waves crashing on the rocks and smell the salty air from my room. It’s a very comforting sensation. The first morning here as I walked along the beach and out on the rocks looking at the ocean, I couldn’t wipe the smile off my face! There’s just something about it that causes my spirit to soar. It’s so mysterious and grandly beautiful.

Then Diane and I went to the ship to participate in a tour for school children from the Escuela America. The mayor of Arica and the local television station were there, too. The kids were great, well-behaved and asked interesting questions! They were third graders and eighth graders. This tour is part of the education efforts of the NOAA.

After the tour, we went to the top of El Morro, a hill that looks like a giant mound of sand. It stands guard over Arica with a statue of an open-armed Jesus overlooking the city and the harbor. We shot a movie clip of Diane and me giving a brief history of Arica.

The next day we journeyed into the Atacama Desert and Andes mountains to have a look. But first we stopped to get water and food because we were going into such a remote area. Wow! The Atacama Desert is one of the driest places on the Earth. It’s a stark yet breathtaking sight to behold. Even though this is a desert there’s abundant evidence of water erosion where a multitude of rounded rocks have been carried into gullies.

As we were driving we suddenly began to see some interesting cacti. These were the Candelabro cacti which grow only between 2500-2800 meters elevation. They have a narrow life zone and are fragile for that reason alone. We were told by a local Chilean woman that they grow very slowly and only after about 30 years will the cactus begin to grow the branches at the top. Diane and I also collected a few rocks to take back to my classes.

As we continued along the main highway that connects Bolivia to the ocean, we stopped at Pueblo de Mallku. This is a village of six! Actually, it’s a homesteaded property of a very interesting family who are conducting the Center for Renewable Energy Resources in conjunction with the university in Arica. They live out in the middle of the desert in a nearly subsistence lifestyle with their closest neighbors being several miles away. They were eager to show us their setup which was quite amazing. They have a solar oven, solar water heater, and a high-tech electrical generator. They have built their dwelling from hand-mixed adobe and cactus logs. They home school their children who’ve compiled a book of local plants and animals along with traditional indigenous Chilean instructional songs on cultivation and medical uses of the plants. During our visit they served us tea with bread and jam. It was quite tasty. The tea was a concoction of leaves and boiling water that will help a body adjust to the extreme altitude.

After we said our goodbyes, we continued to ascend toward the Chungara Lake area. As we went higher and higher on the winding road, two snow-capped volcanoes came into view! I noticed the air started to get very chilly and it was windy. We saw llamas and alpacas grazing in the mountain meadows along the snow-melt streams from the mountaintops. These animals are curious critters! When we stopped for a photo op, they’d perk up their ears, take a long look at us, chew for awhile as though they were thinking about us, then move away occasionally looking back to see if we were looking back. We were fortunate to get to meet a pet alpaca named Cookie. Cookie likes to eat cookies. She was owned by some merchants who had a craft stand near the border stop. John dug out the last of the coconut cookies and shared them with Cookie. She was a true blue friend after that! Cookie’s fur is thick wool and can sell for a high dollar in the U.S.

At this point we were at about 14,000 feet elevation and I was really feeling it. I had a headache, dizziness, and my leg muscles were quivering from fatigue only after a short walk. I didn’t drink enough tea back at Pueblo de Mallku! So we got back in our trusty Puegot and descended to a village called Putre. Putre is a town that caters to tourists. They were happy to see us and very outgoing. Everyone we saw said “Hola” and waved with a smile. We went into a tiny grocery store and purchased supper. We had meat, egg, and olive stuffed empanadas followed by a delicious fig and coconut pastry.

We then took the long and winding road in total darkness back to Arica.

Now I am aboard the NOAA Ship RONALD H. BROWN and we’ve been sailing for six hours. No land in sight. We’ve had two meetings and a delicious supper in the galley. They have an interesting sign in the eating area that says, “Eat it and beat it” There aren’t enough chairs to seat all 45 people at once so when we finish eating we must get up and go elsewhere. It seems everyone has lots of work to do anyway.

Our first meeting was about ship rules and regulations with a focus on safety. We will have our surprise fire drill tomorrow at 2:15 pm promptly! Our science meeting was about the several scientific endeavors and the logistical problems to solve. Our chief scientist Dr. Bob Weller of Woods Hole Oceanographic Institution, encouraged us all to be helpful and considerate.

Some members of the Chilean Navy and Concepcion University are on board to deploy a tsunami detecting buoy which will get underway tomorrow afternoon. We will be deploying CTDs (conductivity, temperature, and depth sensors), and ARGO floats which go down 2000 meters then float to the surface measuring salinity and temperature. Once they break the surface then they send the information to a satellite. These floats then go back down and do it all over again. We’ll also be sending up radiosondes (weather-balloons) and tossing out drifting buoys which measure temperature, pressure, and ocean current pathways. Then the “biggie” is the Stratus 5 buoy! We’ll be out into the Pacific Ocean about 800 miles off the coast of Chile when we do this work which will take about six days. All this stuff is so cool I can’t believe I actually get to witness and participate in even a small way! I’m amazed. I’ll be giving you more information as the time comes so stay in touch and don’t forget to look at the pictures.

Mary

Debra Brice, November 22, 2003

NOAA Teacher at Sea
Debra Brice
Onboard R/V Roger Revelle
November 11-25, 2003

Mission: Ocean Observation
Geographical Area: Chilean Coast
Date: November 22, 2003

Data from the Bridge
1.  221600Z Nov 03
2.  Position: LAT: 20-00.0’S, LONG: 083-44.8’W
3.  Course: 090-T
4.  Speed: 12.6 Kts
5.  Distance: 102.7 NM
6.  Steaming Time:  8H 06M
7.  Station Time:  15H 54M
8.  Fuel: 2583 GAL
9.  Sky: OvrCst
10. Wind: 140-T, 14 Kts
11. Sea: 140-T, 2-3 Ft
12. Swell: 130-T, 3-4 Ft
13. Barometer: 1015.9 mb
14. Temperature: Air: 20.0 C, Sea 19.4 C
15. Equipment Status: NORMAL
16. Comments: Deployment of surface drifter array #4 in progress.

Science and Technology Log

NOAA Climate Studies of Stratocumulus Clouds and the Air-Sea Interaction in Subtropical Cloud Belts. Today we are still underway and I am going to talk about another science group that is onboard and how their research is related to the Stratus Project. We are presently located along the coast of Northern Chile and I just finished interviewing scientist Chris Fairall with NOAA’s Environmental Technology Laboratory in Boulder, Colorado.  A group of 4 ETL scientists are participating in a study of oceanography and meteorology in a region of the ocean that is known for its persistent stratus clouds.

The Woods Hole Oceanographic Institution (WHOI) has maintained a climate monitoring buoy at this location for the last 3 years.  Each year they come out to take out the old buoy and replace it with a brand new one with fresh batteries and new sensors.  A year in the marine environment takes a toll on the toughest instruments.  This is a special buoy which is festooned with atmospheric sensors to measure air-sea fluxes and with a long chain of subsurface instruments to measure ocean currents, temperature and salinity.  If you go to the WHOI website ( http://uop.whoi.edu/stratus) you can read about this project and see the data from the buoy.  The data are transmitted via satellite everyday.  WHOI removed the old buoy on Nov 17 and put in a new one on Nov 19.

Why are these clouds so important?  Because the earth’s climate is driven by energy from the sun and clouds dominate how much solar energy reaches the surface.  On average, almost 40% of the sun’s energy is reflected back into space and half of that is reflected by clouds.  In the cloudy regions more than 60% of the sun’s energy can be reflected by clouds.  The surface temperature of the ocean is a result in a near balance between solar heating and cooling by evaporation and cooling by infrared (IR) radiation from the water surface into the sky.  The global circulation of the atmosphere and ocean are driven by region differences in this net heat input, so clouds have a direct effect on the winds and currents. Cloud effects on the ocean surface energy balance are very tricky because clouds affect both the solar flux (i.e., by reflecting energy back into space) and the IR flux.  It might surprise you, but the sky is ‘warmer’ when there are low clouds present than when the sky is clear.  Think about those cold clear nights in the winter and note the ‘cold’ often appears with ‘clear’. More specifically, the IR radiation coming down from the sky is higher when clouds are present than when skies are clear.  In the tropics and sub-tropics, the solar reflection cooling effect of the clouds is much stronger than their compensating IR warming effect.  Thus, these stratus clouds play an important role in keeping the subtropical oceans cool.

The region we are studying is one of 5 stratus regions around the globe (west coast of U.S.. west coast of S. America, west coast of S. Africa, west coast of N. Africa/Europe, and the west coast of Australia) that occupy vast expanses of ocean.  Both of the pictures I attached to this log show the stratocumulus clouds in this region.  Each of these cloud types has about the same area-average liquid water content but, because of the horizontal distribution, vastly different radiative properties.  The physical processes that lead to these different forms are one of the objective of the ETL studies.

Clouds are formed through various related mechanisms; most involve cooling air to below its dew point temperature so droplets condense ( i.e., clouds are suspensions of liquid water drops with typical sizes of about 10 micrometers radius).  Convective clouds are associated with cooling in strong updrafts; fog and many mid-atmospheric clouds form when an atmospheric layer cools by IR radiation.  The stratus clouds we are studying are quite different.  The key elements are a strong atmospheric cap that traps ocean moisture in a fairly thin ( about 1 km high) boundary layer over the surface.  The stratus clouds occupy the top of the trapped layer from just below the cap to down the altitude ( cloud base height) where temperature and dew point just meet.  Below that, the relative humidity is less than 100%.  The ‘cap’ on the atmosphere boundary layer is warm/dry air descending in subtropical regions, particularly on the western boundaries of continents.  This descending air is actually driven by deep convection in the tropics.  To meteo- nerds this is an amusing paradox – cool stratus clouds off Chile and California are essentially caused by thunderstorms near the Equator.

Clouds are a pain to study because they are so inaccessible.  To get into clouds with sensors you need a really tall tower, a tall building or an aircraft.  Most of these are hard to come by 500 miles from land. Thus, most climate studies of clouds rely on remote sensing methods using satellites and surface based sensors.

ETL has deployed a suite of remote sensors on the R/V Revelle to study clouds from the bottom. The showcase sensors are a special high frequency cloud radar and a 2-frequency microwave radiometer system (this system is the attached picture of the large, white van).  This is the 6th time such sensors have ever been deployed from ships and only the second time to a stratocumulus region.  The first time was to this same spot in 2001; see the web site: http://www.etl.noaa.gov/programs/2001/epic for information on that cruise.

The radar has a wavelength of 8mm, which is so small that it is sensitive enough to receive  detectable signals from scattering cloud droplets.  With this device the ETL group can determine profiles of cloud properties ( such as size of the droplets) through the entire cloud.  The microwave radiometer uses the emissions from the atmosphere at 2 frequencies ( 21 and 31 GHz, or wavelengths of 14 and 9mm) to determine cloud base height and, most importantly, we also measure IR and solar radiative energy reaching the surface.  Instead of just looking at the cloud, they collect megabytes of data every minute.  The beauty of this set up is that they can simultaneously measure the effect the clouds have on the surface energy budget of the ocean and the cloud properties ( liquid water content, thickness, soiled versus broken, number of cloud droplets per unit volume) that go with the radiative effects.  The ETL group are only out here a few weeks each year, but their detailed measurements provide vital information to interpret long-term continuous time series measured by the buoy or inferred from satellite overpasses.

Personal Log

We are surveying for a location for the PMEL Tsunami buoy and the weather is beautiful.  Due to our heading we have lost internet connections periodically.  The food on the REVELLE  is really amazing; last night we had steak and King crab for dinner and a group of the crew and science party met in the lounge to watch a movie.  Card games and cribbage are popular in the dining room and some of us just sit outside and enjoy the sunsets.  I’m going to sleep early as I have the late watch.

Cheers

Debra Brice, November 21, 2003

NOAA Teacher at Sea
Debra Brice
Onboard R/V Roger Revelle
November 11-25, 2003

Mission: Ocean Observation
Geographical Area: Chilean Coast
Date: November 21, 2003

Data from the Bridge
1.  211600Z Nov 03
2.  Position: LAT: 20-00.0’S, LONG: 083-44.8’W
3.  Course: 090-T
4.  Speed: 12.6 Kts
5.  Distance: 102.7 NM
6.  Steaming Time:  8H 06M
7.  Station Time:  15H 54M
8.  Fuel: 2583 GAL
9.  Sky: OvrCst
10. Wind: 140-T, 14 Kts
11. Sea: 140-T, 2-3 Ft
12. Swell: 130-T, 3-4 Ft
13. Barometer: 1015.9 mb
14. Temperature: Air: 20.0 C, Sea 19.4 C
15. Equipment Status: NORMAL
16. Comments: Deployment of surface drifter array #4 in progress.

Science and Technology Log

Today we are underway to the next location which is the area of deployment for the PMEL Tsunami buoy.  I want to talk a little bit about what a Cruise Plan is and why you need one.  I have attached a picture of our latest cruise plan from Dr. Weller.  He had a very nice one ready to go well before we even boarded the ship and everyone in the science party (yes, including me) was given a copy.  Consider this the “game plan.” It can and does change  due to weather or other unforeseen factors and it is very important that the Chief Scientist makes sure that it gets revised as it is necessary to make sure we will have enough time for all of the different deployments and data collections that are planned or to modify as needed.  These cruises are very expensive; from the cost of the ship itself, to the equipment and science party, to the value of the data collected.  For the Stratus Project,  (http://uop.whoi.edu/stratus) this is the big event of the year, everything leads to this moment when the buoy and instruments are recovered and the new buoy is deployed.  Any mistakes made now could potentially result in the loss of data for a whole year.  This brings to mind the importance of really good planning for an expedition of this magnitude.  The Chief scientist has to know how much time he/she need to accomplish their project, build in a few days extra in case of weather or delays, know how much equipment to bring for the project including spare parts (just in case Murphy’s Law kicks in…which it does more often than not!).  Redundancy of equipment is essential from the project itself to the ship which has to be able to repair while on the move with extra parts it has with it or to make a part as needed (yes, they can do that!).  There are no stores out here, if you forget it or run out, you’re out of luck!  That means a year’s work and a big grant could be in danger!

Prior planning is not just a good idea, it is essential and a good Chief scientist has foreseen almost any extenuating circumstance.  There is also the importance of remaining calm and being able to come up with creative solutions to problems in the middle of an important project.  Everyone is watching the Chief scientist and takes their cues on behavior from him/her.  If something happens, they watch to see how he reacts.

The technicians and research associates in a science party need to work well together as they may be at sea for long periods of time (could be a month to several months) .  When you are at sea, 8 hour days doesn’t mean much.  You work whenever there is work to do, deployments or data collection can and do happen around the clock.  The time out here is expensive and data collection is sensitive to many different parameters.  You work seven days a week, but everyone is doing the same and it builds a sense of comradeship to be sharing the work.  Scrabble and Cribbage tournaments in off time are a big event.  Even though they work really hard out here, they all realize the value of what they do and they are here because this is what they wanted to do in life: science.  It is pretty exciting too, you never know what you might see and no matter how long you have been going to sea or how many cruises you do a year, it is still exciting to see whales or dolphins, and beautiful sunset still makes you pause.

Sometimes, as in this cruise, there may be more than one project and multiple scientists.  However, there has to be a Chief scientist to determine priorities and the scheduling concerns so that everyone gets their data, specimens or deploys their equipment.  To be a chief scientist you need to be detail oriented and having workaholic tendencies (at least during a cruise) doesn’t hurt!

This does not mean they don’t have fun after all the hard work is done.  Dr. Weller plans a few days at the beginning and end of a cruise after all the work is done (his group have been working everyday for a month!) to see some of the sights and enjoy the culture of the ports they visit.  Sometimes these days get used for unforeseen circumstances, like extra time for loading, unloading and shipping. Actually that’s why they are put in there.  But if everything gets done in a timely manner, there is a little bit of down time.  He even organizes the tours and had guide books for each of the ports we visited (it’s that detail oriented thing I mentioned!).  He understands the value of appreciating the quality of work your group produces.

Many times the group will consist of one or more grad students under the Chief scientist and this is how they learn to be a chief scientist. It is not a class they take as part of their Ph.D. program, it comes from observation and personal experience.  So mentoring is another important component of the job description.  Seeing the bigger picture is also part of the equation; Dr. Weller really wanted a Teacher at Sea as part of this cruise to help share this experience with younger students and hopefully give a small peek at real scientific research to both k-12 teachers and students.  Many scientists today see the value of this and NOAA has been doing this for 13 years.  Woods Hole Oceanographic Institution has some outstanding education outreach programs such as “Dive and Discover” (check out that WHOI web site!)  Scripps Oceanographic Institution has additional resources at the SIO web site. Please check out the attached picture of the latest cruise plan, as well as a picture of one of the cups that the science party sent down to 4000m on the CTD.  I think the sentiment on the cup is a good reflection of the esteem in which they hold Dr. Weller and I wholeheartedly agree!

Hasta manana

Debra Brice, November 20, 2003

NOAA Teacher at Sea
Debra Brice
Onboard R/V Roger Revelle
November 11-25, 2003

Mission: Ocean Observation
Geographical Area: Chilean Coast
Date: November 20, 2003

Data from the Bridge
1.  201600Z Nov 03
2.  Position: LAT: 19-46.2’S, LONG: 085-32.5’W
3.  Course: On Station
4.  Speed: 0 Kts
5.  Distance: 0 NM
6.  Steaming Time:  0H 00M
7.  Station Time:  24H 00M
8.  Fuel: 1477 GAL
9.  Sky: OvrCst
10. Wind: 140-T, 12 Kts
11. Sea: 140-T, 2-3 Ft
12. Swell: 160-T, 3-5 Ft
13. Barometer: 1018.1 mb
14. Temperature: Air: 21.3 C, Sea 19.7 C
15. Equipment Status: NORMAL
16. Comments: On station in vicinity of WHOI buoy.

Science and Technology Log

We are still in the vicinity of the WHOI buoy and will stay here for 24 hours to check and compare the sensors on the Stratus 4, Stratus 3 and the ship.  We will then leave for the area of deployment of the Tsunami buoy.  We will do 2 CTD casts before leaving.

During our cruise we have been deploying radiosonde weather balloons and the ETL group has been collecting cloud data. I am going to give a brief description of the ETL Cloud Radar and Radiometer Package that they brought with them and are using to collect their data. Clouds play vitally important roles in climate and and water resources by virtue of their ability to transform radiant energy and water phase in the atmosphere.  NOAA?ETL uses microwave and infrared radiometers for ground based cloud observations. ETL designed and is using the Millimeter-wave Cloud Radar (MMCR).  These radars are intended to operate in remote locations and for field experiments.  The radar is joined in a sea container by a dual- channel microwave radiometer (MWR) and a narrow-band infrared radiometer IRR).  Simultaneous data from these instruments provide the input for retrieving microphysical features of the overlying tropospheric clouds.

Instrument Package Characteristics:

Cloud Radar: Ultra high sensitivity, doppler
Primary uses: vertical profiles of clouds. drizzle, snow and very light rain

Microwave Radiometer:
Primary uses: Monitoring vertical water vapor path and liquid water path.

IR Radiometer:
Primary uses: Sensing presense of cloud overhead, estimating base temp. of optically thick clouds.

Collectively, the instruments are called the MMCR Package. Each observes the senith and does not scan, hence, the system is a vertical profiler. This is the second time that ETL has come out with the Stratus Project and it is hoped that through additional funding it will become a permanent partner in this long term study.  ETL is doing these measurements and calibrations not only to verify some of the meteorological data collected from the sensors on the WHOI buoy, but also to do profiles on the cloud structures of the stratus clouds in this area to campare the data to the mathematical models.  They are also using the data to compare and calibrate the mean and the flux calculations used in the Stratus project.  ETL came out during the second year of the Stratus project to do a similar survey.

Personal Log

The WHOI science group are doing their calibrations and measurements all day and the ETL group continues to collect data.  PMEL/NOAA is waiting to deply their buoy at the next site.  The weather is beautiful, warm, sunny, some clouds (stratus!) I am doing a lot of reading and talking with different science groups and crew members to prepare for interviews.  Tonight we will be interviewing the ETL group about their cloud studies. E-mail will be sporadic from now on as we will be on heading that will not allow us satellite communication.  We will turn for 30 minutes once a day to send out and receive e-mail. Tomorrow and the day after will be travel days to the Tsunami deployment site.We still have a couple of boobies following us….obviously hopeful that we will toss out another floating cafeteria for them.  Learning a great deal about how these large oceanographic research vessels run.  They are all owned by different facilities but they are assigned by one entity that schedules all of the science cruises for best efficiency of the vessels.  The scheduling entity is UNOLS.  So a Scripps scientist could be schedules to go out on a Woods Hole vessel one year and a NOAA vessel the next based on the science needs for size, equipment and location.  This means that for example the REVELLE came into its home port of San Diego in September and picked up a science group; did their leg, dropped them off in Manta, Equador, where we met them and loaded equipment for our project and left.  We will arrive in Arica, disembark, ship the equipment back to its various labs and the new science party will board and leave for their project.  This will continue until sometime in April until REVELLE briefly returns to San Diego, where it will pick up another science party and go out again.  It may only come into San Diego two or three times a year.  These ships are almost constantly out working and the crews fly in and out of various ports to meet the ships and change crews.

Hasta Luego

 

Debra Brice, November 18, 2003

NOAA Teacher at Sea
Debra Brice
Onboard R/V Roger Revelle
November 11-25, 2003

Mission: Ocean Observation
Geographical Area: Chilean Coast
Date: November 18, 2003

Data from the Bridge
1.  181700Z Nov 03
2.  Position: LAT: 19-43.5’S, LONG: 085-15.0’W
3.  Course: 000-T
4.  Speed: 12.5 Kts
5.  Distance: 38.8 NM
6.  Steaming Time:  3H 06M
7.  Station Time:  20H 54M
8.  Fuel: 1565 GAL
9.  Sky: Ptly Cldy
10. Wind: 130-T, 11 Kts
11. Sea: 130-T, 2-3 Ft
12. Swell: 150-T, 3-5 Ft
13. Barometer: 1018.5 mb
14. Temperature: Air: 21.3 C, Sea 19.2 C
15. Equipment Status: NORMAL
16. Comments: Survey in progress.

Science and Technology Log

Today the REVELLE spent the day surveying an area for deployment of the STRATUS 4 buoy.  We traveled 50 miles from the STRATUS 3 site with the hopes of getting out of the GPS mapped area of the fishing boats to prevent the fouling of the instruments with fishing line.  Fishing boats target buoys as they become areas of fish aggregation in the open ocean.  The ship took a zigzag pattern most of the day surveying the bottom topography ( see photo of survey and course). Dr Weller explained that he needed to find a relatively long, flat area on the bottom as we will be underway during the deployment of the instrumentation and we need to travel is a straight line to lay out the instruments.  Due to the wind direction we will not be exactly following the straight line of the flat bottom area, but coming in at a slight angle. Jeff Lord and Jason Smith of Woods Hole Oceanographic Institution, Upper Ocean Processes group spent the day preparing the cables, laying out the instrumentation  and spraying various parts with de-fouling paint.  It was a very detailed all day procedure.  Moving the buoy and other heavy instrumentation requires good skills in rigging and crane operations.  The Upper Ocean Processes Group of which Dr. Weller is the head, are highly trained and make this complicated and potentially dangerous work look so easy.  This is part of the job as an oceanographer that you don’t learn in the classroom, but are taught by watching and doing with another professional. The STRATUS 4 buoy will have a slightly different instrumentation than the STRATUS 3.  The Seacat current meters with the rotating fan blades that were fouled with the fishing line will be moved deeper on the mooring and acoustical current meters will be moved to a more shallow spot.  Unfortunately the Seacats are more accurate than the acoustical current meters, but they can’t collect data if they are fouled.  The acoustical meters have no moving parts to foul.  Dr. Weller will also be comparing and calibrating some of the radiation sensors with Dr. Chris Fairall of the ELT group using they cloud radar data.  Deployment will begin after breakfast (approx. 7:45 am) tomorrow morning.

Personal Log

I didn’t help very much with the science activities today other than to stand watch and take hourly temperature readings.  Dr. Kermond and I spent the day filming several interviews.  We toured the extremely impressive engine room on the R/V REVELLE with the Chief Engineer Paul Mauricio.  Please check out our tour on the web.  We also resumed our “Fantail Interviews”  with Jason Tomlinson, Meteorologist from Texas A&M who is doing aerosol research out here with us.  I will spend an entire log in the next couple of days on Jason’s aerosol research.  Tonight on the Fantail we will be interviewing Dr. Chris Fairall of NOAA Environmental Technology Laboratories and NOAA/PMEL Tsunami buoy deployment group, Mike Strick and Scott Stalin.  be sure to tune in:)I need to work on my survey of good sunscreens and/or stronger aloe vera lotions!  The boobies from the STRATUS 3 buoy are following us wanting to know when their new “cafeteria” will be installed.  Much to do tomorrow, it will be another long day doing the deployment and I am very interested as to how they are going to get that 9000 lb anchor in the water!

hasta la vista