HYDRODYNAMICS IN MANGROVE ESTUARY

Joint Research on Environmental Science and Technology for the Eart

Photocatalytic Concrete Pavements: Laboratory Investigation of NO Oxidation Rate Under Varied Environmental Conditions

Concrete pavements containing TiO2 can be used for air pollution control by oxidizing NOX under UV-bearing sunlight. This study employed a bench-scale photoreactor to estimate NO oxidation rates for varied environmental conditions. Rates correlated positively with NO inlet concentration and irradiance and negatively with relative humidity. No correlation occurred with flow rate. A decrease in slab moisture (previously unstudied) positively correlated with NO oxidation rate at 0–2% loss of saturated mass, but negatively correlated at losses greater that 2%. Although prior researchers deemed temperature insignificant, data indicated a positive correlation. Overall, rates ranged from 9.8–64 nmol∙m-2∙s-1

Retinol esterification in Sertoli cells by lecithin-retinol acyltransferase

Esterification of retinol occurs during the metabolism of vitamin A in the testis. An acyl- CoA:retinol acyltransferase (ARAT) activity has been described for microsomes isolated from testis homogenates. That activity was also observed here in microsomal preparations obtained from cultured Sertoli cells from 20-day-old (midpubertal) rats. ARAT catalyzed the synthesis of retinyl laurate when free retinol and lauroyl-CoA were provided as substrates. However, in the absence of exogenous acyl-CoA, retinol was esterified by a different activity in a manner similar to the lecithimretinol acyltransferase (LRAT) activity described recently for liver and intestine. Microsomal preparations obtained from enriched Sertoli cell fractions from the adult rat testis had 75-fold higher levels of LRAT than the preparations from midpubertal animals, but ARAT activity was the same in both these preparations. LRAT utilized an endogenous acyl donor and either unbound retinol or retinol complexed with cellular retinol-binding protein (CRBP) to catalyze the synthesis of retinyl linoleate, retinyl oleate, retinyl palmitate, and retinyl stearate. The addition of exogenous dilaurylphosphatidylcholine (DLPC) resulted in the synthesis of retinyl laurate. The esterification from both exogenous DLPC and endogenous acyl donor was inhibited by 2 mM phenylmethanesulfonyl fluoride (PMSF). ARAT activity was not affected by similar concentrations of PMSF. Furthermore, retinol bound to CRBP, a protein known to be present in Sertoli cells, was not an effective substrate for testicular ARAT. When retinol uptake and metabolism were examined in cultured Sertoli cells from 20-day-old rats, the cells synthesized the same retinyl esters that were produced by microsomal LRAT in vitro. Pretreating the cells with PMSF did not prevent specific retinol accumulation but did inhibit retinol esterification. Consequently, the LRAT-like retinyl esters produced by cultured Sertoli cells and the sensitivity of this esterification to PMSF suggest that LRAT, and not ARAT, is the physiologically important retinyl ester synthase in the Sertoli cell

Characteristics of retinol accumulation from serum retinol-binding protein by cultured Sertoli cells

The uptake of retinol was examined in cultured Sertoli cells when retinol was provided as a complex with the transport protein retinol-binding protein (RBP). Sertoli cells accumulated [3H]retinol in a time- and temperature-dependent manner. At 32 °C, the rate of retinol accumulation was biphasic. Accumulation was linear for approximately 1 h, but then accumulation continued at a linear but decreased rate for 23 h. The change in rate of retinol accumulation occurred when the cells had accumulated approximately 0.53 pmol of retinol/Mg of cellular DNA. This amount of retinol was approximately equal to the cellular content of cellular retinol-binding protein (CRBP). Extraction and HPLC analysis of the cell-associated radioactivity yielded retinol and retinyl esters, indicating that a significant proportion of the accumulated retinol was esterified. Excess unlabeled retinol-RBP competed with [3H]retinol-RBP for [3H]retinol delivery to the cells, indicating that RBP delivery of retinol was a saturable and competable process. However, free [3H]retinol associated with Sertoli cells in a noncompetable manner. The transport constant for specific retinol accumulation from RBP was 3.0 μ , suggesting that any change in the normal circulating retinol-RBP level (approximately 2 μ ) would directly affect the rate of retinol accumulation. Neither iodinated nor reductively methylated RBP was accumulated by or tightly bound to Sertoli cells. In addition, energy inhibitors and lysosomal poisons had no effect on [3H] retinol accumulation, indicating that RBP delivery of retinol to Sertoli cells did not occur by endocytosis of the retinol-RBP complex. Competition studies indicated, however, that protein recognition is important in the retinol uptake process. RBP, CRBP, and CRBP(II) competed with [3H] retinol-RBP for [3H] retinol accumulation, but free retinol, retinol-bovine serum albumin, and retinol-/3-lactoglobulin did not. Transthyretin, bound to [3H] retinol-RBP in the physiological 1:1 ratio, decreased [3H]retinol accumulation by the cells by 25-30% compared to [3H]retinol accumulation from [3H]retinol-RBP. These studies indicated that Sertoli cell uptake of retinol involved recognition of the retinol-RBP complex at the cell surface with subsequent internalization of retinol, but not RBP. The fate of the internalized retinol may first have involved binding by CRBP, but eventually a significant portion of the accumulated retinol was esterified

Mobile radio interferometric geodetic systems

Operation of the Astronomical Radio Interferometric Earth Surveying (ARIES) in a proof of concept mode is discussed. Accuracy demonstrations over a short baseline, a 180 km baseline, and a 380 km baseline are documented. Use of ARIES in the Sea Slope Experiment of the National Geodetic Survey to study the apparent differences between oceanographic and geodetic leveling determinations of the sea surface along the Pacific Coast is described. Intergration of the NAVSTAR Global Positioning System and a concept called SERIES (Satellite Emission Radio Interferometric Earth Surveying) is briefly reviewed

Strongly Coupled Matter-Field and Non-Analytic Decay Rate of Dipole Molecules in a Waveguide

The decay rate \gam of an excited dipole molecule inside a waveguide is evaluated for the strongly coupled matter-field case near a cutoff frequency \ome_c without using perturbation analysis. Due to the singularity in the density of photon states at the cutoff frequency, we find that \gam depends non-analytically on the coupling constant $\ggg$ as $\ggg^{4/3}$. In contrast to the ordinary evaluation of \gam which relies on the Fermi golden rule (itself based on perturbation analysis), \gam has an upper bound and does not diverge at \ome_c even if we assume perfect conductance in the waveguide walls. As a result, again in contrast to the statement found in the literature, the speed of emitted light from the molecule does not vanish at \ome_c and is proportional to $c\ggg^{2/3}$ which is on the order of $10^3 \sim 10^4$ m/s for typical dipole molecules.Comment: 4 pages, 2 figure

Self-Consistent and Time-Dependent Solar Wind Models

We describe the first results from a self-consistent study of Alfven waves for the time-dependent, single-fluid magnetohydrodynamic (MHD) solar wind equations, using a modified version of the ZEUS MHD code. The wind models we examine are radially symmetrical and magnetized; the initial outflow is described by the standard Parker wind solution. Our study focuses on the effects of Alfven waves on the outflow and is based on solving the full set of the ideal nonlinear MHD equations. In contrast to previous studies, no assumptions regarding wave linearity, wave damping, and wave-flow interaction are made; thus, the models naturally account for the back-reaction of the wind on the waves, as well as for the nonlinear interaction between different types of MHD waves. Our results clearly demonstrate when momentum deposition by Alfven waves in the solar wind can be sufficient to explain the origin of fast streams in solar coronal holes; we discuss the range of wave amplitudes required to obtained such fast stream solutions