6,351 research outputs found

    Space cannot be cut: why self-identity naturally includes neighbourhood

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    RRS Discovery Cruise DY039, 17 Oct - 01 Dec 2015, Southampton, UK to Nassau, Bahamas. RAPID moorings cruise report

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    This cruise report covers scientific operations conducted during RRS Discovery Cruise DY039. The purpose of the cruise was the refurbishment of an array of moorings spanning the latitude of 26.5°N from the Bahamas to the Canary Islands. Cruise DY039 departed from Southampton, UK on Saturday 17 October 2015, calling at Tenerife, Spain and Nassau, Bahamas before ending in Nassau, Bahamas on 21 November 2015. The moorings are part of a purposeful Atlantic wide mooring array for monitoring the Atlantic Meridional Overturning Circulation and the associated heat transport. The array is a joint UK- US programme and is known as the RAPID-MOCHA array. During DY039 moorings were serviced at sites: EBH4, EBH4L, EBH3, EBH2, EBH1, EBH1L, EBHi, EB1, EB1L, MAR3, MAR3L, MAR2, MAR1, MAR1L, MAR0, WB6, WB4, WB4L, WBH2, WB2, WB2L, WB1, WBADCP and WBAL. Sites with suffix ‘L’ denote landers fitted with bottom pressure recorders. RAPID-AMOC continues the measurements at 26°N started with the RAPID and RAPID-WATCH programmes and through the ABC Fluxes project extends the measurements to include biological and chemical measurements in order to determine AMOC links to climate and the ocean carbon sink on interannual-to-decadal time scales. This is the first deployment of the ABC Fluxes biogeochemical samplers and sensors to the array (aside from initial oxygen sensors that were deployed in 2014). The ABC Fluxes sensors include pCO2 sensors, pH sensors, additional oxygen sensors and autonomous water samplers to collect samples for nutrient and carbonate chemistry analysis following mooring recovery. Additionally the RAPID telemetry MkIII system was deployed for the first time on the array at EBHi with 6 data pods set to release over the 18-month deployment period. 24 temperature sensors and 2 75kHz ADCPs were also added to mooring WB1 for the MerMEED project. Mooring EB1L was not able to be recovered but a replacement was deployed. A sediment trap mooring NOGST was also recovered and redeployed for the Ocean Biogeochemistry and Ecosystems Group at the NOCS. CTD stations were conducted throughout the cruise for purposes of providing pre- and post- deployment calibrations for mooring instrumentation (including oxygen and carbonate chemistry sampling) and for testing mooring releases prior to deployment. Shipboard underway measurements were systematically logged, processed and calibrated, including: surface meteorology, 5m depth sea temperatures and salinities, water depth, and navigation. Water velocity profiles from 15 m to approximately 800 m depth were obtained using the two vessel mounted Acoustic Doppler Current Profilers (one 75 kHz and one 150 kHz)

    RRS Discovery Cruise DY039, 17 Oct - 01 Dec 2015, Southampton, UK to Nassau, Bahamas. RAPID moorings cruise report

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    This cruise report covers scientific operations conducted during RRS Discovery Cruise DY039. The purpose of the cruise was the refurbishment of an array of moorings spanning the latitude of 26.5°N from the Bahamas to the Canary Islands. Cruise DY039 departed from Southampton, UK on Saturday 17 October 2015, calling at Tenerife, Spain and Nassau, Bahamas before ending in Nassau, Bahamas on 21 November 2015.The moorings are part of a purposeful Atlantic wide mooring array for monitoring the Atlantic Meridional Overturning Circulation and the associated heat transport. The array is a joint UK- US programme and is known as the RAPID-MOCHA array.During DY039 moorings were serviced at sites: EBH4, EBH4L, EBH3, EBH2, EBH1, EBH1L, EBHi, EB1, EB1L, MAR3, MAR3L, MAR2, MAR1, MAR1L, MAR0, WB6, WB4, WB4L, WBH2, WB2, WB2L, WB1, WBADCP and WBAL. Sites with suffix ‘L’ denote landers fitted with bottom pressure recorders. RAPID-AMOC continues the measurements at 26°N started with the RAPID and RAPID-WATCH programmes and through the ABC Fluxes project extends the measurements to include biological and chemical measurements in order to determine AMOC links to climate and the ocean carbon sink on interannual-to-decadal time scales. This is the first deployment of the ABC Fluxes biogeochemical samplers and sensors to the array (aside from initial oxygen sensors that were deployed in 2014).The ABC Fluxes sensors include pCO2 sensors, pH sensors, additional oxygen sensors and autonomous water samplers to collect samples for nutrient and carbonate chemistry analysis following mooring recovery.Additionally the RAPID telemetry MkIII system was deployed for the first time on the array at EBHi with 6 data pods set to release over the 18-month deployment period. 24 temperature sensors and 2 75kHz ADCPs were also added to mooring WB1 for the MerMEED project.Mooring EB1L was not able to be recovered but a replacement was deployed. A sediment trap mooring NOGST was also recovered and redeployed for the Ocean Biogeochemistry and Ecosystems Group at the NOCS.CTD stations were conducted throughout the cruise for purposes of providing pre- and post- deployment calibrations for mooring instrumentation (including oxygen and carbonate chemistry sampling) and for testing mooring releases prior to deployment.Shipboard underway measurements were systematically logged, processed and calibrated, including: surface meteorology, 5m depth sea temperatures and salinities, water depth, and navigation. Water velocity profiles from 15 m to approximately 800 m depth were obtained using the two vessel mounted Acoustic Doppler Current Profilers (one 75 kHz and one 150 kHz)

    A note on the CMH general association statistic and square contingency tables

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    In this expository note a simplified formula for the CMH general association statistic applicable to repeated categorical response data is given and applied to three-way square contingency tables

    FeH Absorption in the Near-Infrared Spectra of Late M and L Dwarfs

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    We present medium-resolution z-, J-, and H-band spectra of four late-type dwarfs with spectral types ranging from M8 to L7.5. In an attempt to determine the origin of numerous weak absorption features throughout their near-infrared spectra, and motivated by the recent tentative identification of the E 4\Pi- A ^4\Pi system of FeH near 1.6 microns in umbral and cool star spectra, we have compared the dwarf spectra to a laboratory FeH emission spectrum. We have identified nearly 100 FeH absorption features in the z-, J-, and H-band spectra of the dwarfs. In particular, we have identified 34 features which dominate the appearance of the H-band spectra of the dwarfs and which appear in the laboratory FeH spectrum. Finally, all of the features are either weaker or absent in the spectrum of the L7.5 dwarf which is consistent with the weakening of the known FeH bandheads in the spectra of the latest L dwarfs.Comment: accepted by Ap

    Time transfer between the Goddard Optical Research Facility and the U.S. Naval Observatory using 100 picosecond laser pulses

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    A horizontal two-way time comparison link in air between the University of Maryland laser ranging and time transfer equipment at the Goddard Optical Research Facility (GORF) 1.2 m telescope and the Time Services Division of the U.S. Naval Observatory (USNO) was established. Flat mirrors of 25 cm and 30 cm diameter respectively were placed on top of the Washington Cathedral and on a water tower at the Beltsville Agricultural Research Center. Two optical corner reflectors at the USNO reflect the laser pulses back to the GORF. Light pulses of 100 ps duration and an energy of several hundred microjoules are sent at the rate of 10 pulses per second. The detection at the USNO is by means of an RCA C30902E avalanche photodiode and the timing is accomplished by an HP 5370A computing counter and an HP 1000 computer with respect to a 10 pps pulse train from the Master Clock

    Inoculation of peritoneal dialysate fluid into blood culture bottles improves culture rates

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    The aim of the study was to determine if direct inoculation of peritoneal fluid into Bactec blood culture bottles would improve the positive bacteriological yield compared with conventional techniques in continuous ambulatory peritoneal dialysis (CAPD) patients with peritonitis. All patients presenting with suspected peritonitis had peritoneal fluid injected directly into aerobic and anaerobic Bactec blood culture bottles as well as into sterile culture tubes. Thirty-seven paired samples were analysed. Twenty conventional cultures (54%) were positive compared with 33 (89%) done according to the Bactec system (P < 0,002). In only 1 case did the former technique prove superior. Direct inoculation of peritoneal fluid into Bactec blood culture bottles is therefore superior to conventional methods and has obvious therapeutic implications
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