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At least 451 records · Page 25

Measurement of Volatile Compounds for Real-Time Analysis of Soil Microbial Metabolic Response to Simulated Snowmelt

Snowmelt dynamics are a significant determinant of microbial metabolism in soil and regulate global biogeochemical cycles of carbon and nutrients by creating seasonal variations in soil redox and nutrient pools. With an increasing concern that climate change accelerates both snowmelt timing and rate, obtaining an accurate characterization of microbial response to snowmelt is important for understanding biogeochemical cycles intertwined with soil. However, observing microbial metabolism and its dynamics non-destructively remains a major challenge for systems such as soil. Microbial volatile compounds (mVCs) emitted from soil represent information-dense signatures and when assayed non-destructively using state-of-the-art instrumentation such as Proton Transfer Reaction-Time of Flight-Mass Spectrometry (PTR-TOF-MS) provide time resolved insights into the metabolism of active microbiomes. In this study, we used PTR-TOF-MS to investigate the metabolic trajectory of microbiomes from a subalpine forest soil, and their response to a simulated wet-up event akin to snowmelt. Using an information theory approach based on the partitioning of mutual information, we identified mVC metabolite pairs with robust interactions, including those that were non-linear and with time lags. The biological context for these mVC interactions was evaluated by projecting the connections onto the Kyoto Encyclopedia of Genes and Genomes (KEGG) network of known metabolic pathways. Simulated snowmelt resulted in a rapid increase in the production of trimethylamine (TMA) suggesting that anaerobic degradation of quaternary amine osmo/cryoprotectants, such as glycine betaine, may be important contributors to this resource pulse. Unique and synergistic connections between intermediates of methylotrophic pathways such as dimethylamine, formaldehyde and methanol were observed upon wet-up and indicate that the initial pulse of TMA was likely transformed into these intermediates by methylotrophs. Increases in ammonia oxidation signatures (transformation of hydroxylamine to nitrite) were observed in parallel, and while the relative role of nitrifiers or methylotrophs cannot be confirmed, the inferred connection to TMA oxidation suggests either a direct or indirect coupling between these processes. Overall, it appears that such mVC time-series from PTR-TOF-MS combined with causal inference represents an attractive approach to non-destructively observe soil microbial metabolism and its response to environmental perturbation.

59 BASIC BIOLOGICAL SCIENCES↗

Dimensional Reduction for Sampled Priors and Application to Photometric Redshift Distributions

A typical Bayesian inference on the values of some parameters of interest q from some data D involves running a Markov Chain (MC) to sample from the posterior $p$($q$,$n$|$D$) $\propto$ $\mathcal{L}$($D$|$q$,$n$)$p$(q)$p$($n$), where n are some nuisance parameters with a separable prior. In some cases, the nuisance parameters are high-dimensional, and their prior p(n) is itself defined only by a set of samples that have been drawn from some other MC. The MC for the posterior will typically require evaluation of p(n) at arbitrary values of n, i.e., one needs to provide a density estimator over the full n space from the provided samples. But the high dimensionality of n hinders both the density estimation and the efficiency of the MC for the posterior. We describe a solution to this problem: a linear compression of the n space into a much lower-dimensional space u, which projects away directions in n space that cannot appreciably alter $\mathcal{L}$. The algorithm for doing so is a slight modification to principal components analysis, and is less restrictive on p(n) than other proposed solutions to this issue. We demonstrate this “mode projection” technique using the analysis of 2-point correlation functions of weak lensing fields and galaxy density in the Dark Energy Survey, where n is a binned representation of the redshift distribution n(z) of the galaxies.

79 ASTRONOMY AND ASTROPHYSICS↗

Gauge invariants of linearized gravity with a general background metric

In linearized gravity with distributed matter, the background metric has no generic symmetries, and decomposition of the metric perturbation into global normal modes is generally impractical. This complicates the identification of the gauge-invariant part of the perturbation, which is a concern, for example, in the theory of dispersive gravitational waves (GWs) whose energy–momentum must be gauge-invariant. Here, we propose how to identify the gauge-invariant part of the metric perturbation and the six independent gauge invariants per se for an arbitrary background metric. For the Minkowski background, the operator that projects the metric perturbation on the invariant subspace is proportional to the well-known dispersion operator of linear GWs in vacuum. For a general background, this operator is expressed in terms of the Green’s operator of the vacuum wave equation. Further, if the background is smooth, it can be found asymptotically using the inverse scale of the background metric as a small parameter.

71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSIC↗

Response of Silicon-Based Linear Energy Transfer Spectrometers: Implication for Radiation Risk Assessment in Space Flights

There is considerable interest in developing silicon-based telescopes because of their compactness and low power requirements. Three such telescopes have been flown on board the Space Shuttle to measure the linear energy transfer spectra of trapped, galactic cosmic ray, and solar energetic particles. Dosimeters based on single silicon detectors have also been flown on the Mir orbital station. A comparison of the absorbed dose and radiation quality factors calculated from these telescopes with that estimated from measurements made with a tissue equivalent proportional counter show differences which need to be fully understood if these telescopes are to be used for astronaut radiation risk assessments. Instrument performance is complicated by a variety of factors. A Monte Carlo-based technique was developed to model the behavior of both single element detectors in a proton beam, and the performance of a two-element, wide-angle telescope, in the trapped belt proton field inside the Space Shuttle. The technique is based on: (1) radiation transport intranuclear-evaporation model that takes into account the charge and angular distribution of target fragments, (2) Landau-Vavilov distribution of energy deposition allowing for electron escape, (3) true detector geometry of the telescope, (4) coincidence and discriminator settings, (5) spacecraft shielding geometry, and (6) the external space radiation environment, including albedo protons. The value of such detailed modeling and its implications in astronaut risk assessment is addressed. c2001 Elsevier Science B.V. All rights reserved.

manned↗

Materials Data on InCuO2 by Materials Project

CuInO2 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Cu1+ is bonded in a linear geometry to two equivalent O2- atoms. Both Cu–O bond lengths are 1.85 Å. In3+ is bonded to six equivalent O2- atoms to form edge-sharing InO6 octahedra. All In–O bond lengths are 2.21 Å. O2- is bonded to one Cu1+ and three equivalent In3+ atoms to form a mixture of distorted edge and corner-sharing OIn3Cu tetrahedra.

36 MATERIALS SCIENCE↗

Materials Data on InAgO2 by Materials Project

AgInO2 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Ag1+ is bonded in a linear geometry to two equivalent O2- atoms. Both Ag–O bond lengths are 2.11 Å. In3+ is bonded to six equivalent O2- atoms to form edge-sharing InO6 octahedra. All In–O bond lengths are 2.21 Å. O2- is bonded to one Ag1+ and three equivalent In3+ atoms to form a mixture of distorted corner and edge-sharing OIn3Ag tetrahedra.

36 MATERIALS SCIENCE↗

Materials Data on MgC2 by Materials Project

MgC2 crystallizes in the tetragonal P4_2/mnm space group. The structure is three-dimensional. Mg2+ is bonded in a distorted linear geometry to six equivalent C1- atoms. There are two shorter (2.17 Å) and four longer (2.57 Å) Mg–C bond lengths. C1- is bonded in a 2-coordinate geometry to three equivalent Mg2+ and one C1- atom. The C–C bond length is 1.26 Å.

36 MATERIALS SCIENCE↗

Materials Data on Ag2HgO2 by Materials Project

Ag2HgO2 crystallizes in the tetragonal P4_32_12 space group. The structure is three-dimensional. Ag1+ is bonded in a linear geometry to two equivalent O2- atoms. There are one shorter (2.13 Å) and one longer (2.14 Å) Ag–O bond lengths. Hg2+ is bonded in a distorted rectangular see-saw-like geometry to four equivalent O2- atoms. There are two shorter (2.09 Å) and two longer (2.62 Å) Hg–O bond lengths. O2- is bonded to two equivalent Ag1+ and two equivalent Hg2+ atoms to form corner-sharing OAg2Hg2 tetrahedra.

36 MATERIALS SCIENCE↗

Materials Data on AlCuO2 by Materials Project

CuAlO2 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Cu1+ is bonded in a linear geometry to two equivalent O2- atoms. Both Cu–O bond lengths are 1.88 Å. Al3+ is bonded to six equivalent O2- atoms to form edge-sharing AlO6 octahedra. All Al–O bond lengths are 1.92 Å. O2- is bonded to one Cu1+ and three equivalent Al3+ atoms to form a mixture of distorted corner and edge-sharing OAl3Cu tetrahedra.

36 MATERIALS SCIENCE↗

Materials Data on GaCuO2 by Materials Project

CuGaO2 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Cu1+ is bonded in a linear geometry to two equivalent O2- atoms. Both Cu–O bond lengths are 1.87 Å. Ga3+ is bonded to six equivalent O2- atoms to form edge-sharing GaO6 octahedra. All Ga–O bond lengths are 2.02 Å. O2- is bonded to one Cu1+ and three equivalent Ga3+ atoms to form a mixture of distorted edge and corner-sharing OGa3Cu tetrahedra.

36 MATERIALS SCIENCE↗

Materials Data on Tl2CuAsO4 by Materials Project

CuTl2AsO4 crystallizes in the monoclinic P2_1/c space group. The structure is three-dimensional. Cu1+ is bonded in a distorted linear geometry to three O2- atoms. There are a spread of Cu–O bond distances ranging from 1.87–2.71 Å. There are two inequivalent Tl1+ sites. In the first Tl1+ site, Tl1+ is bonded in a 4-coordinate geometry to four O2- atoms. There are a spread of Tl–O bond distances ranging from 2.56–3.06 Å. In the second Tl1+ site, Tl1+ is bonded in a 5-coordinate geometry to three O2- atoms. There are a spread of Tl–O bond distances ranging from 2.59–2.81 Å. As5+ is bonded in a tetrahedral geometry to four O2- atoms. There are a spread of As–O bond distances ranging from 1.72–1.77 Å. There are four inequivalent O2- sites. In the first O2- site, O2- is bonded in a 4-coordinate geometry to one Cu1+, two equivalent Tl1+, and one As5+ atom. In the second O2- site, O2- is bonded in a 2-coordinate geometry to one Cu1+, two Tl1+, and one As5+ atom. In the third O2- site, O2- is bonded in a distorted water-like geometry to one Cu1+, one Tl1+, and one As5+ atom. In the fourth O2- site, O2- is bonded in a 3-coordinate geometry to two equivalent Tl1+ and one As5+ atom.

36 MATERIALS SCIENCE↗

Materials Data on HgN6 by Materials Project

HgN6 crystallizes in the orthorhombic Pca2_1 space group. The structure is three-dimensional. Hg2+ is bonded in a distorted linear geometry to five N+0.33- atoms. There are a spread of Hg–N bond distances ranging from 2.08–3.02 Å. There are six inequivalent N+0.33- sites. In the first N+0.33- site, N+0.33- is bonded in a 3-coordinate geometry to two equivalent Hg2+ and one N+0.33- atom. The N–N bond length is 1.22 Å. In the second N+0.33- site, N+0.33- is bonded in a linear geometry to two N+0.33- atoms. The N–N bond length is 1.16 Å. In the third N+0.33- site, N+0.33- is bonded in a distorted bent 150 degrees geometry to one Hg2+ and one N+0.33- atom. In the fourth N+0.33- site, N+0.33- is bonded in a 2-coordinate geometry to two equivalent Hg2+ and one N+0.33- atom. The N–N bond length is 1.22 Å. In the fifth N+0.33- site, N+0.33- is bonded in a linear geometry to two N+0.33- atoms. The N–N bond length is 1.16 Å. In the sixth N+0.33- site, N+0.33- is bonded in a distorted single-bond geometry to one N+0.33- atom.

36 MATERIALS SCIENCE↗

Materials Data on AgC2N3 by Materials Project

AgC2N3 crystallizes in the trigonal P3_121 space group. The structure is three-dimensional. Ag1+ is bonded in a distorted linear geometry to six equivalent N3- atoms. There are a spread of Ag–N bond distances ranging from 2.12–3.11 Å. C4+ is bonded in a linear geometry to two N3- atoms. There is one shorter (1.18 Å) and one longer (1.29 Å) C–N bond length. There are two inequivalent N3- sites. In the first N3- site, N3- is bonded in a 2-coordinate geometry to three equivalent Ag1+ and one C4+ atom. In the second N3- site, N3- is bonded in a bent 120 degrees geometry to two equivalent C4+ atoms.

36 MATERIALS SCIENCE↗

Materials Data on Ni3(BiS)2 by Materials Project

Ni3Bi2S2 crystallizes in the cubic I2_13 space group. The structure is three-dimensional. Ni is bonded in a distorted linear geometry to four equivalent Bi and two equivalent S atoms. There are two shorter (2.74 Å) and two longer (2.90 Å) Ni–Bi bond lengths. Both Ni–S bond lengths are 2.18 Å. Bi is bonded in a 7-coordinate geometry to six equivalent Ni and one S atom. The Bi–S bond length is 3.26 Å. S is bonded in a 3-coordinate geometry to three equivalent Ni and one Bi atom.

36 MATERIALS SCIENCE↗

Materials Data on CuAuO2 by Materials Project

AuCuO2 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Au3+ is bonded in a linear geometry to two equivalent O2- atoms. Both Au–O bond lengths are 2.04 Å. Cu1+ is bonded to six equivalent O2- atoms to form edge-sharing CuO6 octahedra. All Cu–O bond lengths are 2.03 Å. O2- is bonded to one Au3+ and three equivalent Cu1+ atoms to form a mixture of distorted edge and corner-sharing OCu3Au tetrahedra.

36 MATERIALS SCIENCE↗

Materials Data on LiNb10O18 by Materials Project

LiNb10O18 crystallizes in the monoclinic P2_1/c space group. The structure is three-dimensional. Li1+ is bonded in a distorted linear geometry to two equivalent O2- atoms. Both Li–O bond lengths are 2.75 Å. There are five inequivalent Nb+3.50+ sites. In the first Nb+3.50+ site, Nb+3.50+ is bonded to five O2- atoms to form NbO5 square pyramids that share corners with four NbO6 octahedra and corners with six NbO5 square pyramids. The corner-sharing octahedra tilt angles range from 3–45°. There are a spread of Nb–O bond distances ranging from 2.08–2.20 Å. In the second Nb+3.50+ site, Nb+3.50+ is bonded to five O2- atoms to form NbO5 square pyramids that share corners with three NbO6 octahedra, corners with five NbO5 square pyramids, and an edgeedge with one NbO6 octahedra. The corner-sharing octahedra tilt angles range from 5–55°. There are a spread of Nb–O bond distances ranging from 2.07–2.28 Å. In the third Nb+3.50+ site, Nb+3.50+ is bonded to five O2- atoms to form NbO5 square pyramids that share a cornercorner with one NbO6 octahedra, corners with five NbO5 square pyramids, and edges with two NbO6 octahedra. The corner-sharing octahedral tilt angles are 48°. There are a spread of Nb–O bond distances ranging from 2.05–2.20 Å. In the fourth Nb+3.50+ site, Nb+3.50+ is bonded to six O2- atoms to form NbO6 octahedra that share corners with two equivalent NbO6 octahedra, corners with four NbO5 square pyramids, edges with two NbO6 octahedra, and an edgeedge with one NbO5 square pyramid. The corner-sharing octahedra tilt angles range from 9–42°. There are a spread of Nb–O bond distances ranging from 2.01–2.16 Å. In the fifth Nb+3.50+ site, Nb+3.50+ is bonded to six O2- atoms to form NbO6 octahedra that share corners with two equivalent NbO6 octahedra, corners with four NbO5 square pyramids, an edgeedge with one NbO6 octahedra, and edges with two NbO5 square pyramids. The corner-sharing octahedra tilt angles range from 9–42°. There are a spread of Nb–O bond distances ranging from 1.97–2.10 Å. There are nine inequivalent O2- sites. In the first O2- site, O2- is bonded in a T-shaped geometry to three Nb+3.50+ atoms. In the second O2- site, O2- is bonded in a T-shaped geometry to three Nb+3.50+ atoms. In the third O2- site, O2- is bonded in a 4-coordinate geometry to one Li1+ and three Nb+3.50+ atoms. In the fourth O2- site, O2- is bonded in a 3-coordinate geometry to three Nb+3.50+ atoms. In the fifth O2- site, O2- is bonded in a T-shaped geometry to three Nb+3.50+ atoms. In the sixth O2- site, O2- is bonded in a T-shaped geometry to three Nb+3.50+ atoms. In the seventh O2- site, O2- is bonded in a 3-coordinate geometry to three Nb+3.50+ atoms. In the eighth O2- site, O2- is bonded in a 3-coordinate geometry to three Nb+3.50+ atoms. In the ninth O2- site, O2- is bonded in a 3-coordinate geometry to three Nb+3.50+ atoms.

36 MATERIALS SCIENCE↗

Materials Data on CuPO3 by Materials Project

CuPO3 crystallizes in the trigonal R-3 space group. The structure is three-dimensional. Cu1+ is bonded in a distorted linear geometry to two O2- atoms. There is one shorter (1.86 Å) and one longer (1.87 Å) Cu–O bond length. P5+ is bonded to four O2- atoms to form corner-sharing PO4 tetrahedra. There are a spread of P–O bond distances ranging from 1.50–1.61 Å. There are three inequivalent O2- sites. In the first O2- site, O2- is bonded in a bent 150 degrees geometry to two equivalent P5+ atoms. In the second O2- site, O2- is bonded in a distorted bent 150 degrees geometry to one Cu1+ and one P5+ atom. In the third O2- site, O2- is bonded in a 2-coordinate geometry to one Cu1+ and one P5+ atom.

36 MATERIALS SCIENCE↗

Materials Data on TlCuO2 by Materials Project

CuTlO2 crystallizes in the trigonal R-3m space group. The structure is three-dimensional. Cu1+ is bonded in a linear geometry to two equivalent O2- atoms. Both Cu–O bond lengths are 1.83 Å. Tl3+ is bonded to six equivalent O2- atoms to form edge-sharing TlO6 octahedra. All Tl–O bond lengths are 2.33 Å. O2- is bonded to one Cu1+ and three equivalent Tl3+ atoms to form a mixture of distorted edge and corner-sharing OTl3Cu tetrahedra.

36 MATERIALS SCIENCE↗