1,028 research outputs found

    Climatically driven loss of calcium in steppe soil as a sink for atmospheric carbon

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    During the last several thousand years the semi‐arid, cold climate of the Russian steppe formed highly fertile soils rich in organic carbon and calcium (classified as Chernozems in the Russian system). Analysis of archived soil samples collected in Kemannaya Steppe Preserve in 1920, 1947, 1970, and fresh samples collected in 1998 indicated that the native steppe Chernozems, however, lost 17–28 kg m−2 of calcium in the form of carbonates in 1970–1998. Here we demonstrate that the loss of calcium was caused by fundamental shift in the steppe hydrologic balance. Previously unleached soils where precipitation was less than potential evapotranspiration are now being leached due to increased precipitation and, possibly, due to decreased actual evapotranspiration. Because this region receives low levels of acidic deposition, the dissolution of carbonates involves the consumption of atmospheric CO2. Our estimates indicate that this climatically driven terrestrial sink of atmospheric CO2 is ∼2.1–7.4 g C m−2 a−1. In addition to the net sink of atmospheric carbon, leaching of pedogenic carbonates significantly amplified seasonal amplitude of CO2 exchange between atmosphere and steppe soil

    Beam Energy Dependence of the Third Harmonic of Azimuthal Correlations in Au+Au Collisions at RHIC

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    We present results from a harmonic decomposition of two-particle azimuthal correlations measured with the STAR detector in Au+Au collisions for energies ranging from sNN=7.7\sqrt{s_{NN}}=7.7 GeV to 200 GeV. The third harmonic v32{2}=cos3(ϕ1ϕ2)v_3^2\{2\}=\langle \cos3(\phi_1-\phi_2)\rangle, where ϕ1ϕ2\phi_1-\phi_2 is the angular difference in azimuth, is studied as a function of the pseudorapidity difference between particle pairs Δη=η1η2\Delta\eta = \eta_1-\eta_2. Non-zero {\vthree} is directly related to the previously observed large-Δη\Delta\eta narrow-Δϕ\Delta\phi ridge correlations and has been shown in models to be sensitive to the existence of a low viscosity Quark Gluon Plasma (QGP) phase. For sufficiently central collisions, v32{2}v_3^2\{2\} persist down to an energy of 7.7 GeV suggesting that QGP may be created even in these low energy collisions. In peripheral collisions at these low energies however, v32{2}v_3^2\{2\} is consistent with zero. When scaled by pseudorapidity density of charged particle multiplicity per participating nucleon pair, v32{2}v_3^2\{2\} for central collisions shows a minimum near {\snn}=20=20 GeV.Comment: 7 pages, 4 figures, for submission to Phys. Rev. Let

    Observation of D0D^0 meson nuclear modifications in Au+Au collisions at sNN\sqrt{s_{_{\mathrm{NN}}}} = 200 GeV

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    We report the first measurement of charmed-hadron (D0D^0) production via the hadronic decay channel (D0K+π+D^0\rightarrow K^- + \pi^+) in Au+Au collisions at sNN\sqrt{s_{_{\mathrm{NN}}}} = 200\,GeV with the STAR experiment. The charm production cross-section per nucleon-nucleon collision at mid-rapidity scales with the number of binary collisions, NbinN_{bin}, from pp+pp to central Au+Au collisions. The D0D^0 meson yields in central Au+Au collisions are strongly suppressed compared to those in pp+pp scaled by NbinN_{bin}, for transverse momenta pT>3p_{T}>3 GeV/cc, demonstrating significant energy loss of charm quarks in the hot and dense medium. An enhancement at intermediate pTp_{T} is also observed. Model calculations including strong charm-medium interactions and coalescence hadronization describe our measurements.Comment: 7 pages including author list, 4 figures, submit to PRL with revised versio
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