The need for accurate yield prediction is increasing for estimating productivity and production costs to secure high revenues in the semiconductor industry. Corresponding to this end, we introduce new spatial modeling approaches for spatially clustered defects on an integrated circuit (IC) wafer map. We use spatial location of an IC chip on the wafer as a covariate on corresponding defects count listed in a wafer map. Analysis results indicate that yield prediction can be greatly improved by capturing spatial features of defects. Tyagi and Bayoumi's (1994) wafer map data are used to illustrate the procedure.

A series of high resolution spectra of CH Cygni obtained at the Bohyunsan Optical Astronomy Observatory (BOAO) in April 2004 has been analyzed. The emission components of the [O I] 6300 A lines are de-convoluted and fitted with Gaussian functions in order to investigate the characteristics and the structure of CH Cygni system along with the analysis for Hα and [O III] lines. A present geometrical structure of the components of CH Cygni system is suggested.

The box culvert is one of the simple and common structures employed repetitively in construction field. Although parametric computer applications have demonstrated a significant amount of time savings in designing simple and repetitive structures, circulating resultant electronic documents among project participants has not been fully integrated with these applications. This paper presents a development of Web applications to improve the process of a box culvert design and document management using XML and SVG. We developed a parametric Web application in order to facilitate not only engineering design of the box culvert but also management of resultant documents over the Web. This paper presents how XML Data Island and SVG were utilized to generate engineering drawings and display them in the Web page.

Shock waves form in the intergalactic space as an ubiquitous consequence of cosmic structure formation. Using N-body/hydrodynamic simulation data of a ACDM universe, we examined the properties of cosmological shock waves including their morphological distribution. Adopting a diffusive shock acceleration model, we then calculated the amount of cosmic ray energy as well as that of gas thermal energy dissipated at the shocks. Finally, the dynamical consequence of those cosmic rays on cluster properties is discussed.

It is commonly observed that Korean students tend to use the English conjunction so more often than any other English conjunction when expressing cause or reason in English. On the other hand, because is the conjunction of choice among native English speakers. This paper attempts to explain why Korean English learners have the tendency to use so over other conjunctions, and to analyze some of the similarities and differences in the use of Korean and English causal connectors. The findings of the study provide an empirical basis for the development of course design and teaching materials, especially for the development of courses in English writing for academic purposes.

Shocks are ubiquitous in astrophysical environments and cosmic-rays (CRs) are known to be accelerated at collisionless shocks via diffusive shock acceleration. It is believed that the CR pressure is important in the evolution of the interstellar medium of our galaxy and most of galactic CRs with energies up to ~ 1015 eV are accelerated by supernova remnant shocks. In this contribution we have studied the CR acceleration at shocks through numerical simulation of 1D, quasi-parallel shocks for a wide range of shock Mach numbers and shock speeds. We show that CR modified shocks evolve to time-asymptotic states by the time injected particles are accelerated to moderately relativistic energies, and that two shocks with the same Mach number, but with different shock speeds, evolve qualitatively similarly when the results are presented in terms of a characteristic diffusion length and diffusion time. We find that 10-4 - 10-3 of the particles passed through the shock are accelerated to form the CR population, and the injection rate is higher for shocks with higher Mach number. The time asymptotic value for the CR acceleration efficiency is controlled mainly by shock Mach number, and high Mach number shocks all evolve towards efficiencies ~ 50%, regardless of the injection rate and upstream CR pressure. We conclude that the injection rates in strong quasi-parallel shocks are sufficient to lead to significant nonlinear modifications to the shock structures, implying the importance of the CR acceleration at astrophysical shocks.

The purpose of this study is to investigate how Korean primary school L2 readers construct intertextual meaning and how they relate their conceptions or beliefs about reading to their intertextualtity. School instructions or home literacy environments in English reading might influence L2 readers' reading conceptions and their reading processes which are in turn associated with their intertextual connections among the multiple texts. Though current literature in L2 reading has focused on great interest in the reading processes of a single story or text, little interest was given to L2 readers' intertextuality among the multiple stories. The researcher first diagnoses four Korean primary school readers' reading conceptions, followed by retrospective miscue reading analyses to investigate their reading processes. Finally, their intertextual connections among the five stories of adventure are examined by conducting think-aloud procedure. The results showed that L2 readers have their own reading conceptions and behaviors, which are influenced by their home literacy environment and school instructions. In addition, Korean EFL readers' conceptions of reading and behaviors are strongly connected with their intertextuality among the multiple stories.