Recent experiments were carried out on the Prague Asterix Laser System (PALS) towards the demonstration of a soft x-ray laser Thomson scattering diagnostic for a laser-produced exploding foil. The Thomson probe utilized the Ne-like zinc x-ray laser which was double-passed to deliver {approx}1 mJ of focused energy at 21.2 nm wavelength and lasting {approx}100 ps. The plasma under study was heated single-sided using a Gaussian 300-ps pulse of 438-nm light (3{omega} of the PALS iodine laser) at laser irradiances of 10{sup 13}-10{sup 14} W cm{sup -2}. Electron densities of 10{sup 20}-10{sup 22} cm{sup -3} and electron temperatures from 200 to 500 eV were probed at 0.5 or 1 ns after the peak of the heating pulse during the foil plasma expansion. A flat-field 1200 line mm{sup -1} variable-spaced grating spectrometer with a cooled charge-coupled device readout viewed the plasma in the forward direction at 30{sup o} with respect to the x-ray laser probe. We show results from plasmas generated from {approx}1 {micro}m thick targets of Al and polypropylene (C{sub 3}H{sub 6}). Numerical simulations of the Thomson scattering cross-sections will be presented. These simulations show electron peaks in addition to a narrow ion feature due to collective (incoherent) Thomson scattering. The …

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Email from Christina Ocasio to the Texas Stonewall Democratic Caucus Austin chapter about meetings and bylaws.

This cleanup verification package documents completion of remedial action for the 126-F-1, 184-F Powerhouse Ash Pit. This waste site received coal ash from the 100-F Area coal-fired steam plant. Leakage of process effluent from the 116-F-14 , 107-F Retention Basins flowed south into the ash pit, contaminating the northern portion.

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Measurements of CP violating observables of the decays B{sup 0} {yields} {phi}K{sup 0}, B{sup 0} {yields} {eta}'K{sub S}, B{sup 0} {yields} {rho}K{sub S}, B{sup 0} {yields} K{sup +}K{sup -}K{sup 0} and B{sup 0} {yields} K{sub S}K{sub S}K{sub S} are presented. In addition limits on the branching functions of B{sup 0} {yields} {phi}{pi}{sup 0}, B{sup 0} {yields} {phi}{pi}{sup +}, B {yields} K{sup *}K{sub S}, B {yields} {eta}'{pi}{sup 0}, B {yields} {eta}'{eta}, and B{sup 0} {yields} K{sub S}K{sub S}K{sub L} are reported.

Testimony issued by the Government Accountability Office with an abstract that begins "In February 2007, a series of Washington Post articles disclosed troublesome deficiencies in the provision of outpatient services at Walter Reed Army Medical Center, raising concerns about the care for returning servicemembers. These deficiencies included a confusing disability evaluation system and servicemembers in outpatient status for months and sometimes years without a clear understanding about their plan of care. The reported problems at Walter Reed prompted broader questions about whether the Department of Defense (DOD) as well as the Department of Veterans Affairs (VA) are fully prepared to meet the needs of returning servicemembers. In response to the deficiencies reported at Walter Reed, the Army took a number of actions and DOD formed a joint DOD-VA Senior Oversight Committee. This statement provides information on the near-term actions being taken by the Army and the broader efforts of the Senior Oversight Committee to address longer-term systemic problems that impact health care and disability evaluations for returning servicemembers. Preliminary observations in this testimony are based largely on documents obtained from and interviews with Army officials, and DOD and VA representatives of the Senior Oversight Committee, as well as on GAO's …

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Observations with H.E.S.S. revealed a new source of very high-energy (VHE) gamma-rays above 100 GeV - HESS J1825-137 - extending mainly to the south of the energetic pulsar PSRB1823-13. A detailed spectral and morphological analysis of HESS J1825-137 reveals for the first time in VHE gamma-ray astronomy a steepening of the energy spectrum with increasing distance from the pulsar. This behavior can be understood by invoking radiative cooling of the IC-Compton gamma-ray emitting electrons during their propagation. In this scenario the vastly different sizes between the VHE gamma-ray emitting region and the X-ray PWN associated with PSRB1823-13 can be naturally explained by different cooling timescales for the radiating electron populations. If this scenario is correct, HESS J1825-137 can serve as a prototype for a whole class of asymmetric PWN in which the X-rays are extended over a much smaller angular scales than the gamma-rays and can help understanding recent detections of X-ray PWN in systems such as HESS J1640-465 and HESS J1813-178. The future GLAST satellite will probe lower electron energies shedding further light on cooling and diffusion processes in this source.

A letter report issued by the Government Accountability Office with an abstract that begins "Household energy use accounts for nearly one-fourth of all energy consumed in the United States, amounting to more than $200 billion per year spent by consumers. Recent increases in energy prices have heightened consumers' interest in making their households more energy efficient. To this end, the federal government manages two key efforts--EnergyGuide and Energy Star--to inform consumers about the energy consumed by certain household products. EnergyGuide is a mandatory labeling program created under the Energy Policy and Conservation Act of 1975 (EPCA) and administered by the Federal Trade Commission (FTC) with assistance from the Department of Energy (DOE). It requires manufacturers to label and prominently display information about the energy consumption and annual energy costs of 11 categories of household products. In recent years, manufacturers have used adhesive backed labels adhered to appliances and so-called "hang tags" loosely attached to the interior or exterior of appliances. In its August 2007 revisions to the rule, FTC, among other things, prohibited the use of hang tags on the exterior of appliances, but continues to allow them on the inside. The law requires retailers to provide this information in …

Concert presented at the UNT College of Music Winspear Hall.

Daily newspaper from Chickasha, Oklahoma that includes local, state, and national news along with advertising.

We have added the capability to look at in-cylinder fuel distributions using a previously developed ignition model within a fluid mechanics code (KIVA3V) that uses an artificial neural network (ANN) to predict ignition (The combined code: KIVA3V-ANN). KIVA3V-ANN was originally developed and validated for analysis of Homogeneous Charge Compression Ignition (HCCI) combustion, but it is also applicable to the more difficult problem of Premixed Charge Compression Ignition (PCCI) combustion. PCCI combustion refers to cases where combustion occurs as a nonmixing controlled, chemical kinetics dominated, autoignition process, where the fuel, air, and residual gas mixtures are not necessarily as homogeneous as in HCCI combustion. This paper analyzes the effects of introducing charge non-uniformity into a KIVA3V-ANN simulation. The results are compared to experimental results, as well as simulation results using a more physically representative and computationally intensive code (KIVA3V-MPI-MZ), which links a fluid mechanics code to a multi-zone detailed chemical kinetics solver. The results indicate that KIVA3V-ANN produces reasonable approximations to the more accurate KIVA3V-MPI-MZ at a much reduced computational cost.

This work is part of a larger project to develop a modeling capability for magnetron sputter deposition. The process is divided into four steps: plasma transport, target sputter, neutral gas and sputtered atom transport, and film growth, shown schematically in Fig. 1. Each of these is simulated separately in this Part 1 of the project, which is jointly funded between CMLS and Engineering. The Engineering portion is the plasma modeling, in step 1. The plasma modeling was performed using the Object-Oriented Particle-In-Cell code (OOPIC) from UC Berkeley [1]. Figure 2 shows the electron density in the simulated region, using magnetic field strength input from experiments by Bohlmark [2], where a scale of 1% is used. Figures 3 and 4 depict the magnetic field components that were generated using two-dimensional linear interpolation of Bohlmark's experimental data. The goal of the overall modeling tool is to understand, and later predict, relationships between parameters of film deposition we can change (such as gas pressure, gun voltage, and target-substrate distance) and key properties of the results (such as film stress, density, and stoichiometry.) The simulation must use existing codes, either open-source or low-cost, not develop new codes. In part 1 (FY07) we identified and …

Shell-type Supernova remnants (SNRs) have long been known to harbour a population of ultra-relativistic particles, accelerated in the Supernova shock wave by the mechanism of diffusive shock acceleration. Experimental evidence for the existence of electrons up to energies of 100 TeV was first provided by the detection of hard X-ray synchrotron emission as e.g. in the shell of the young SNR SN1006. Furthermore using theoretical arguments shell-type Supernova remnants have long been considered as the main accelerator of protons - Cosmic rays - in the Galaxy; definite proof of this process is however still missing. Pulsar Wind Nebulae (PWN) - diffuse structures surrounding young pulsars - are another class of objects known to be a site of particle acceleration in the Galaxy, again through the detection of hard synchrotron X-rays such as in the Crab Nebula. Gamma-rays above 100 MeV provide a direct access to acceleration processes. The GLAST Large Area telescope (LAT) will be operating in the energy range between 30 MeV and 300 GeV and will provide excellent sensitivity, angular and energy resolution in a previously rather poorly explored energy band. We will describe prospects for the investigation of these Galactic particle accelerators with GLAST.

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Free weekly newspaper that includes business and classified advertising.