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  • 1
    Publication Date: 2009-09-04
    Description: Primary production in over half of the world's oceans is limited by fixed nitrogen availability. The main loss term from the fixed nitrogen inventory is the production of dinitrogen gas (N(2)) by heterotrophic denitrification or the more recently discovered autotrophic process, anaerobic ammonia oxidation (anammox). Oceanic oxygen minimum zones (OMZ) are responsible for about 35% of oceanic N(2) production and up to half of that occurs in the Arabian Sea. Although denitrification was long thought to be the only loss term, it has recently been argued that anammox alone is responsible for fixed nitrogen loss in the OMZs. Here we measure denitrification and anammox rates and quantify the abundance of denitrifying and anammox bacteria in the OMZ regions of the Eastern Tropical South Pacific and the Arabian Sea. We find that denitrification rather than anammox dominates the N(2) loss term in the Arabian Sea, the largest and most intense OMZ in the world ocean. In seven of eight experiments in the Arabian Sea denitrification is responsible for 87-99% of the total N(2) production. The dominance of denitrification is reproducible using two independent isotope incubation methods. In contrast, anammox is dominant in the Eastern Tropical South Pacific OMZ, as detected using one of the isotope incubation methods, as previously reported. The abundance of denitrifying bacteria always exceeded that of anammox bacteria by up to 7- and 19-fold in the Eastern Tropical South Pacific and Arabian Sea, respectively. Geographic and temporal variability in carbon supply may be responsible for the different contributions of denitrification and anammox in these two OMZs. The large contribution of denitrification to N(2) loss in the Arabian Sea indicates the global significance of denitrification to the oceanic nitrogen budget.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Ward, B B -- Devol, A H -- Rich, J J -- Chang, B X -- Bulow, S E -- Naik, Hema -- Pratihary, Anil -- Jayakumar, A -- England -- Nature. 2009 Sep 3;461(7260):78-81. doi: 10.1038/nature08276.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Geosciences, Princeton University, Princeton, New Jersey 08544, USA. bbw@princeton.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19727197" target="_blank"〉PubMed〈/a〉
    Keywords: Anaerobiosis ; Arabia ; Bacteria/genetics/metabolism ; Carbon/metabolism ; Gases/metabolism ; Nitrites/metabolism ; Nitrogen/*metabolism ; *Nitrogen Fixation ; Oceans and Seas ; Oxidation-Reduction ; Oxygen/metabolism ; Pacific Ocean ; Quaternary Ammonium Compounds/metabolism ; RNA, Ribosomal, 16S/genetics ; Seawater/*chemistry/microbiology
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2011-01-26
    Description: We explore the feasibility of using variations in the horizontal component (ΔBH) of the Earth's magnetic field as measured by DMSP satellites while crossing the dip equator to estimate the provisional Dst index and the state of the thermosphere in near real time. Equatorial crossings are identified as locations where the vertical component of the main field measured by DMSP satellites vanishes. Local differences between measured and IGRF (epoch 2005) horizontal components (δBH) were calculated for the years 2005 to 2009. Each year quiet time (0 ≥ Dst ≥ – 7 nT) subsets of δBH were identified to establish offset baselines (δBH B) as functions of longitude along the magnetic equator ($\phi$eq) for each spacecraft. Year-to-year changes in δBH B reflect variations of the Earth's main field, indicating that baseline calculations must be updated at regular intervals for each spacecraft. Running-averaged values of ΔBH(t) = δBH ($\phi$eq, t) − δBH B ($\phi$eq, t) inferred from combined DMSP F16 and F17 data streams are shown to follow variations in Dst during the test interval. The method is also shown to apply during the magnetic superstorms of late 2003. Except during the late main phase, increases in globally averaged exospheric temperatures inferred from ΔBH and provisional Dst time series are in reasonable agreement with those inferred from measurements by accelerometers on the GRACE satellites.
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 3
    Publication Date: 2016-04-23
    Description: We compare mid-infrared (IR) 3.6 and 4.5 μm Warm Spitzer observations for Cepheids in the Milky Way and the Large and Small Magellanic Clouds. Using models, we explore in detail the effect of the CO rotation–vibration band-head at 4.6 μm on the mid-IR photometry. We confirm the temperature sensitivity of the CO band-head at 4.6 μm and find no evidence for an effect at 3.6 μm. We compare the ([3.6]–[4.5]) period–colour relations in the MW, LMC and SMC. The slopes of the period–colour relations for the three galaxies are in good agreement, but there is a trend in zero-point with metallicity, with the lowest metallicity Cepheids having redder mid-IR colours. Finally, we present a colour-[Fe/H] relation based on published spectroscopic metallicities. This empirical relation, calibrated to the metallicity system of Genovali et al., demonstrates that the ([3.6]–[4.5]) colour provides a reliable metallicity indicator for Cepheids, with a precision comparable to current spectroscopic determinations.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 4
    Publication Date: 2009-09-01
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Springer Nature
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