The Atmospheric Mercury Flight Campaign
Transcription
The Atmospheric Mercury Flight Campaign
The Atmospheric Mercury Flight Campaign Aviation Av a o Sys Systemss Progra Program,, UT Space Spac Institute I s August 2010 Some of the Atmospheric Mercury Team from U. of Miami and the UT Space Institute The UT Space Institute Participates in At Atmospheric h i Mercury M Study St d From 31 July through 12 August 2010, The University of Tennessee Space Institute (UTSI) participated in an intensive field study to investigate the chemistry, chemistry transport, transport and deposition of mercury compounds in the atmosphere. Partners in this study included • • • • • • • • • The National Oceanic and Atmospheric Administration’s (NOAA) Air Resources Laboratory (ARL) The Georgia Institute of Technology Florida State University The University of Miami The Canaan Valley Institute, West Virginia Florida A&M University Th Mississippi The Mi i i i Department D t t off Environmental E i t l Quality Q lit NOAA's National Centers for Coastal Ocean Science (NCCOS) The UT Space Institute Aviation Systems Program Scientists and engineers converged on the Grand Bay National Estuarine Research Reserve (NERR) in Moss Point, MS where they could take advantage of the existing NOAA ARL mercury measurement facility. Specifically, the scientists measured the mercury in the atmosphere, in specific rainfall episodes, and in dew to determine the origin of the measured compounds. The role played by halogen species (bromine and chlorine) in the marine environment as well as in the upper atmosphere was also investigated using a variety of techniques. * Portions of above text is taken from a Press Release written by Dr. Winston Luke, NOAA ARL. UTSI Atmospheric Mercury Flight Campaign The UTSI Piper Navajo airborne science research aircraft (N11UT) was used in the study to measure mercury and other pollutants at altitudes ranging from the surface to 15,500 feet in the Gulf of Mexico region, in partnership with NOAA/ARL and the University of Miami. The aircraft was based at Trent‐Lott International Airport, Pascagoula, MS during the study. To support the aircraft measurements, NOAA/ARL scientists launched weather balloons from the NERR to measure the profiles of temperature, humidity, pressure, winds, and ozone concentrations from the surface to altitudes as high as 100,000 feet. Grand Bay NERR, Florida A&M University, and NOAA NCCOS scientists also measured mercury concentrations in biota and in water and sediment samples at various locations within the reserve. * Portions of above text is taken from a Press Release written by Dr. Winston Luke, NOAA ARL. More About the Atmospheric Mercury Study The study is intended to address key issues in atmospheric mercury research including the importance of transport from the middle atmosphere to the surface; the role of halogen compounds in mercury transformations; the specific chemical identities of individual mercury species; i the th relative l ti contributions t ib ti off natural t l and d anthropogenic th i (man‐made) ( d ) emissions i i sources; and the relationship between mercury concentrations in the air and in rainfall to the prevalence of mercury in the NERR ecosystem, including fish and other wildlife. In most locations, locations mercury merc r in aquatic aq atic ecosystems ecos stems results res lts from deposition from the atmosphere, atmosphere but the mercury in the atmosphere arises from both natural and man‐made sources. Data show that the Gulf of Mexico region is plagued by persistently high total mercury in precipitation. Once in the watershed, this mercury can enter the local food chain. Human exposure to mercury is primarily from the consumption of contaminated fish and other aquatic organisms. organisms Fish consumption in coastal areas is typically much higher than the national average, and every state along the Gulf of Mexico has widespread fish consumption advisories for mercury. This study will allow the scientists to better understand what is unique about the region and to address questions, such as: Are mercury concentrations high because of halogens in the marine boundary layer? Or, are mercury concentrations high because frequent and widespread convective activity and rainfall continually scrub the middle and upper troposphere of reactive gaseous mercury, mercury which may arise from halogen chemistry in the troposphere and the stratosphere? What role is played by local and regional anthropogenic mercury sources? * Above text is taken from a Press Release written by Dr. Winston Luke, NOAA ARL. The Grand Bay National Estuarine E Research R Reserve R (NERR) ( ERR) Moss Point, MS The NERR is a modern, state-of-the-art science and education facility. NERR Ground-Based Data Collection Inside the NOAA ARL mercury instrumentation trailer Florida State U. aerosol and precipitation collectors “On the Road” to Mississippi Mechanic Shane Porter and grad student Joe Young drove to Mississippi in the UTSI van, carrying much of our needed equipment… and Prof. Muratore’s luggage! Tullahoma, TN to Pascagoula, g MS We fferriedd th W the UTSI Navajo airborne b science researchh aircraft ft ffrom Tullahoma Airport to Trent-Lott International Airport on 31 July 2010. Ready for (Scientific)Action! Tucked away in its new temporary hangar home at Trent-Lott Airport, the UTSI Navajo is ready for atmospheric mercury flights. UTSI Piper Navajo Airborne Science Aircraft Our “little” little Navajo was packed with scientific instruments instruments, including mercury denuders, a TekRan mercury analyzer, ozone and sulphur dioxide detectors, a hygrometer, digital video, and a laser altimeter. Air Inlet Tubes Three air inlet tubes were mounted through the right-side cabin window. The large, forward-facing tube was for mercury and the two smaller, aft-facing tubes were for ozone and sulphur dioxide. Keeping these tubes “sterile” on the ground was very important for getting good quality airborne b data. TThe mercury tube b was continuously flushed with nitrogen gas on the ground. The mercury air inlet tube fed a system of denuders – glass tubes that collected aerosol pparticles – mounted in the box at the topp off the rack. There were 8 denuders loaded into the box and the Scientist opened valves allowing air to enter each denuder. At the end of each flight, the denuder tubes were carefully removed and analyzed at the NERR. Flying Backwards The view from the Scientist seat (left) and Flight Test Engineer seat (right) in the aircraft main cabin. Both of these seats face backwards, so these folks had to have strong stomachs… if you’ve ever ridden backwards, you’ll know what we mean! Dr. Phil Swartzendruber, U. of Miami atmospheric mercury scientist, t t flflew with th us on all ll off our science missions. Long Hours and Late Nights in the Mississippi Heat Everyone workedd day E d andd night h as required, d 7 ddays a week. The heat index in the daytime and into the night was often over 100 degrees! Science Mission Flight Planning This aeronautical map gives you some idea of the flight paths (in red) that we flew around the Gulf region. It took quite a bit of planning and coordination with Air Traffic Control. Earlyy Morningg Flight g Prepp We started our days y veryy earlyy to help beat the heat and to avoid the typical y afternoon build-up of thunderstorms. We usually started our flight preparations at around 6 a.m. and tried to take-off by about 8:30 a.m. Mark Cohen, NOAA ARL, provided the team with a huge amount of atmospheric data on a daily basis to help us determine where to fly. Balloon Launch NOAA scientists i ti t P Paull K Kelly ll andd Wi Winston t L Luke k llaunched hd high altitude balloons from the NERR to gather atmospheric data on flight days. The balloons would transmit data to the ground from up to over 100,000 100 000 ft altitude. altitude Research Professors and Aviators John Muratore and Borja Martos before a Mercury flight Mechanic Shane Porter assists Prof. John J Muratore prior to boarding for a flight. Engine g Start Our aircraft mechanics, Shane Porter (left) and Greg Heatherlyy (right), did an incredible job keeping us flying, despite propeller governor and engine ignition problems that required a lot of “extra effort” on their part to fix. Taxi ffor Takeoffff UTSI Piper Navajo 11UT taxiing for takeoff with Trent-Lott tower in the background. W received We i d many comments t ffrom the th Air Ai Traffic T ffi C Controllers t ll about b t our “UT” UT airplane, i l many ending their radio transmissions to us with the words, “Roll Tide!”… seems there are a few Alabama fans down there! Of course, we responded, “Go Vols!” Takeoff… ff in Search off Mercury! y “Sniffing” for Mercury Along the Gulf Coast Note the mercury air sampling tube on the right. View of the Beautiful Gulf Coast Shoreline Looking to the East View of the Gulf Coast View to the South into the Gulf of Mexico Flying Over the Gulf of Mexico Note the oil slicks in the water. We saw many vessels in support of the oil spill recovery. We flew as low as 500 ft above the water taking measurements in the marine boundary layer. One of the Barrier Islands off the Gulf Coast Since we were beyond gliding distance to the shore if our engines quit at low altitude, we wore personal floatation gear and had a life raft on board. High g Altitude Flight g We flew as high as about 16,000 ft, measuring significant atmospheric mercury in the clean, high air. These types of airborne mercury measurements are quite unique, having been made onlyy once or twice in the past. We think we mayy have even sampled airborne dust that came all the way from the African continent. Dark Skies on the Horizon Flying around the Gulf Coast in the late Summer, there was the constant threat of violent thunderstorms. Careful flight planning and excellent aircraft avionics equipment kept us safe. Landingg After f a Science Flight F g The flights were about 3 hours long and although we were pretty hot and tired when we got back, we were always excited to discuss our scientific findings. Headingg Home Departing the Gulf Coast as a tropical storm approaches. The UTSI Av Systems Atmospheric Mercury Flight Campaign Team Chief Mechanic Greg Heatherlyy G and Mechanic Sh Shane P Porter t Research Professor and Flight Test Engineer JJohn Muratore Grad Student and Flight Test Engineer Joe Young Research Professor and Pilot B j M Borja Martos t Associate Professor and Pilot Stephen Corda This Was a Team Effort! Unfortunately, we don’t have pictures of all the Av Systems folks that made this a success andd off course, we could ld not take everyone withh us to the h Gulf G lf off Mexico, but b the following folks were nonetheless a significant part of our team: Prof. Peter Solies, Prof. Richard Ranaudo, and Admin. Asst. Brenda Brown G d Students Grad St d t Will M Moonan, JJonathan th K Kolwyck, l k andd S Sammy Willi Williams We know that we’ve left out all of the other UTSI folks that are not in Av Systems that helped us to be successful… Thanks to all of you too! What’s Next for Airborne Mercury? The atmospheric Th t h mercury flight fl ht campaign was very successful f l with th over 17 hhours of airborne data collected. We will be busy over the next few months supporting the analysis and publication of the airborne science data. We will be returning to the Gulf of Mexico, as NOAA has already asked us to support another atmospheric mercury flight campaign in April 2011.