Chemical changes during transport from cloud to disk

Chemical abundances from Magellanic cloud B stars

In recent years, B stars have been established as reliable tracers of present day abundance patterns. They yield an independent set of abundances from He to Fe which can be cross-checked against other sources such as H ii regions and cool supergiants. In this paper, we present purely spectroscopic analyses of 9 non-supergiant B stars (13 < mV < 15), 5 of which located in the young populous clus...

The process of kidney gradual changes in, Tenualosa ilisha during migration from sea to the river

Abstract In order to study kidney changes in, Tenualosa ilisha during migration from sea to the river, twenty mature T. ilisha specimens were collected from the Persian Gulf (42.7ppt salinity and 29.27°C temperature) and twenty specimens from Arvand River (2.3ppt salinity and 21.16°C temperature). Macroscopic observation indicated that the kidney was located retroperitoneal and attached to...

Chemical changes in skeletal muscle during development.

Comparisons of Cloud Microphysical Properties Retrieved from Different Algorithms during Aerosol Transport Events

Multi-spectral data from the MODerate resolution Imaging Spectroradiometer (MODIS) onboard the Terra spacecraft are used to derive cloud optical thickness and effective particle radius using the algorithm of Nakajima and Nakajima (1995). Microphysical cloud properties are retrieved during strong aerosol events from biomass burning to better understand the actual effects of cloud-aerosol interac...

Distributed Virtual Private Disk for Cloud Computing

In recent years a new technological paradigm has emerged in the computer science research community. This paradigm is referred to as Cloud Computing, a new computing paradigm whose aims are to allow users to utilize computing infrastructure over the network, supplied as an on-demand service. There are already many commercial solutions based on this approach, as well as many academic research pr...