Critical current degradation in wide samples of high field strip superconductors

Anisotropy determination of critical current density in wide samples of strip semiconductors as function of magnetic field directio

Experimental investigation of advanced super- conducting magnets. superconducting strip and its use in magnets final report

Superconducting strip for superconducting magnet coil constructio

Experimental investigation of advanced superconducting magnets Annual report

Experimental investigations of advanced superconducting magnet

Prediction of Cardiac Response to Physical Stress

This paper presents a method for predicting an individual's cardiac response to a series of fixed intensity tasks. It was determined that cardiac responses to exercise at given work loads are similar for subjects of the same sex and level of physical fitness when they are expressed in terms of resting heart rate. Using this observation as a basis, a prediction model was developed by extrapolating from emperically derived heart rate patterns. The prediction error was no more than five to ten percent of the actual heart rate value in ninety percent of the predictions.Yeshttps://us.sagepub.com/en-us/nam/manuscript-submission-guideline

The Conservation of Human Resources in Energy Systems

The operation of an energy system often requires that its personnel engage in manual and technical activities that involve exposure to health and safety hazards. A typical electric utility is used as a model for studying the operation of safety and health programs for energy systems. Specific criteria regarding standards and management are presented and discussed. These criteria are general enough so that they may be applied in the management of future energy systems

Colorado's agribusiness system: its contribution to the state economy in 1997

Includes bibliographical references.This paper describes economic contribution in four ways: employment, income, value added, and gross sales. Includes Executive summary.Sponsored by the Colorado Department of Agricultur

No-Till: North Dakota Research Emphasis

Introduction of no-till into North Dakota soil management systems has raised many questions relative to performance under present cropping or climatic conditions. A number of long term cooperative research projects were established in 1977 to answer these questions and set some guidelines for no-till production systems. The areas of research emphasis at various experiment stations are discussed along with preliminary results on one year's data

The Grism Lens-Amplified Survey from Space (GLASS). IX. The dual origin of low-mass cluster galaxies as revealed by new structural analyses

Using deep Hubble Frontier Fields imaging and slitless spectroscopy from the Grism Lens-Amplified Survey from Space, we analyze 2200 cluster and 1748 field galaxies at $0.2\leq z\leq0.7$ to determine the impact of environment on galaxy size and structure at $\log M_*/M_\odot>7.8$, an unprecedented limit at these redshifts. Based on simple assumptions-$r_e=f(M_*)$-we find no significant differences in half-light radii ($r_e$) between equal-mass cluster or field systems. More complex analyses-$r_e=f(M_*,U-V,n,z,\Sigma$)-reveal local density $(\Sigma$) to induce only a $7\% \pm 3\%$ ($95\%$ confidence) reduction in $r_e$ beyond what can be accounted for by $U-V$ color, Sersic index ($n$), and redshift ($z$) effects.Almost any size difference between galaxies in high- and low-density regions is thus attributable to their different distributions in properties other than environment. Indeed, we find a clear color-$r_e$ correlation in low-mass passive cluster galaxies ($\log M_*/M_\odot<9.8$) such that bluer systems have larger radii, with the bluest having sizes consistent with equal-mass star-forming galaxies. We take this as evidence that large-$r_e$ low-mass passive cluster galaxies are recently acquired systems that have been environmentally quenched without significant structural transformation (e.g., by ram pressure stripping or starvation).Conversely, $\sim20\%$ of small-$r_e$ low-mass passive cluster galaxies appear to have been in place since $z\sim3$. Given the consistency of the small-$r_e$ galaxies' stellar surface densities (and even colors) with those of systems more than ten times as massive, our findings suggest that clusters mark places where galaxy evolution is accelerated for an ancient base population spanning most masses, with late-time additions quenched by environment-specific mechanisms are mainly restricted to the lowest masses.Comment: The accepted version. The catalog is available through the GLASS web page (http://glass.astro.ucla.edu), or https://www.astr.tohoku.ac.jp/~mtakahiro/Publication/Morishita17