Four divers were exposed successively for ten minute periods to pure tones of 5600, 1400, and 700 hertz (Hz) (in that order) in air at 100 decibels above 20 raicropascal and in water at various sound pressure levels between 125 and 150 decibels above 20 micropascal. Divers incurred moderate temporary auditory-threshold shifts (TTS) from all exposures. Equivalent amounts of TTS are produced in w...

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In this work, we outline the findings of our recent study properties $N^*(1895)$ and its consequential impacts on cross sections photoproduction $\Lambda(1405)$. Further, discuss possibility existence an isovector state, with mass similar to $\Lambda(1405)$, which refer as $\Sigma(1400)$. With idea motivating experimental investigations $\Sigma(1400)$, have studied process determined respective...

Evaluation of MM5-EMICAT2000-CMAQ performance and sensitivity in complex terrain: highresolution application to the northeastern Iberian Peninsula Pedro Jiménez, Oriol Jorba, René Parra and José M. Baldasano Barcelona Supercomputing Center – Centro Nacional de Supercomputación (BSC-CNS). Jordi Girona 29, 08034 Barcelona, Spain. Laboratory of Environmental Modeling. Universitat Politècnica de Ca...

A wide variety of agricultural chemicals with potential to affect amphibian health are released into the environment daily. Most of these chemicals are xenobiotic compounds that are highly toxic to embryos, tadpoles, and terrestrial stages. Other substances that occur in pristine environments at harmless concentrations, such as inorganic nitrogenous compounds, may reach potentially toxic levels...

The mass eigen states K1(1270) and K1(1400) are mixture of the strange members of two axial-vector SU(3) octet, P1(K A 1 ) and P1(K B 1 ). Taking into account this mixture, the forward-backward asymmetry and branching ratio of B → K1(1270, 1400) l+l− transitions are studied in the framework of different supersymmetric models. It is found that the results have considerable deviation from the sta...

Kandis Lea Jessup, Lowell Observatory, 1400 W Mars Hill Rd, Flagstaff, AZ, 86001 John R. Spencer, Lowell Observatory, 1400 W Mars Hill Rd, Flagstaff, AZ, 86001 Gilda E. Ballester, Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85271 Robert R. Howell, Dept. Geology and Geophysics, University of Wyoming, Laramie, WY 82071 Fred Roesler, Department of Physics, University of Wisco...