Sustav sesta salv. Gasell by Miguel Alvarez - Issuu

Katse rekonstrueerida muistsete eestlaste rivastust ja varustust E. Aastatel — kasvas OÜ Mosolem kasum 21,51 ja käive 2,96 korda. Mida tähendab riigikaitse demokraatlik juhtimine? Senised ikka piisavalt alles C2Pöörake sõela noole suunas, kuni turvaluku sulgur fikseerub mootorisse. Muistse Eesti sjaajaloo thtsaim pe- riood on muistne vabadusvitlus

It contains the great majority of the photons emitted by the universe, and THz observations of molecules and dust are able penetrate deeply into molecular clouds, thus revealing the full history of star and planet formation. Accordingly, the successful deployments of the Herschel and SOFIA observatories, and the emerging capabilities of ALMA, are both revolutionizing our understanding of THz astrophysics and placing stringent demands sustav sesta salv the generation of accurate laboratory data on the relevant gas phase and solid state materials detected.

We have investigated solid materials from room temperature to 10 K, and can examine both refractory matter such as silicates and molecular ices.

For the latter, we have demonstrated that the THz bands observed are uniquely sensitive to both the molecular structure of the ice and its thermal history, and thus that THz observations can provide novel insight into the dominant condensable materials in dense, cold regions. In the gas phase we can record doppler-limited data over at least a decade in bandwidth. While quite capable, the high vacuum cryostat can only study thick samples, especially ices, due to the fairly rapid adsorption of gases onto surfaces at low temperature under such conditions.

With such modifications Science. The computational demands of this program continue to increase rapidly as these researchers seek to perform physics-based numerical simulations of earthquake processes for larger meet the needs of this research program, a multiple-institution team coordinated by SCEC has integrated several scientific codes into a numerical modeling-based research tool we call the TeraShake computational platform TSCP.

In this chapter, we describe how we extended an existing, stand-alone, wellvalidated, finite-difference, anelastic wave propagation modeling code into the highly scalable and widely used TS-AWP and then integrated this code into the TeraShake computational platform that provides end-to-end initialization to analysis research capabilities.

We also describe the techniques used to enhance the TS-AWP parallel performance on TeraGrid supercomputers, as well as the TeraShake simulations phases including input preparation, run time, data archive management, and visualization.

In addition, the TSCP has developed into a computational system that is useful to many members of the SCEC community for sustav sesta salv large-scale earthquake simulations.