Nursing informatics where caring and technology meet pdf

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Nursing informatics where caring and technology meet pdf

Nursing Informatics: Where Caring and Technology Meet

Publisher : Springer
Release Date :

ISBN : 0387989234
Author :
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Since publication of the first edition in 1988, this book has established itself as the premier reference
text for nurses, nursing administrators, nursing students, and other health care professionals who
seek a state-of-the-art review of the role of IT in the nursing profession. The third edition of this
seminal work keeps readers at the forefront of the rapidly evolving field of nursing informatics,
examining new trends and thoroughly updating and revising all content. New chapters include:
Selecting a Nursing Informatics Consultant; Project Management; Consumer Informatics; Data
Mining; Education (CME, Patient); Electronic Medical Imaging; Nursing Informatics Competencies;
Telehealth and Implications; Business Process Reengineering; Nursing's Role in Telehealth.
Download Here
http://eap-books.club/readonline/?item=0387989234&lan=en

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books.club/readonline/?item=0387989234&lan=en
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We explore different scenarios to explain the chemical difference found in the remarkable giant-giant binary system HD138202+CD−3012303. For the first time, we suggest how to distinguish these scenarios by taking advantage of the extensive convective envelopes of giant stars. Methods. We carried out a high-precision determination of stellar parameters and abundances by applying a full line-by-line differential analysis on GHOST high-resolution spectra. We used the FUNDPAR program with ATLAS12 model atmospheres and specific opacities calculated for an arbitrary composition through a doubly iterated method. Physical parameters were estimated with the isochrones package and evolutionary tracks were calculated via MIST models. Results. We found a significant chemical difference between the two stars (∆[Fe/H]∼0.08dex), which is largely unexpected considering the insensitivity of giant stars to planetary ingestion and diffusion effects. We tested the possibility of engulfment events by using several different combinations of stellar mass, ingested mass, metallicity of the engulfed object and different convective envelopes. However, the planetary ingestion scenario does not seem to explain the observed differences. For the first time, we distinguished the source of chemical differences using a giant-giant binary system. By ruling out other possible scenarios such as planet formation and evolutionary effects between the two stars, we suggest that primordial inhomogeneities might explain the observed differences. This remarkable result implies that the metallicity differences that were observed in at least some main-sequence binary systems might be related to primordial inhomogeneities rather than engulfment events. We also discuss the important implications of finding primordial inhomogeneities, which affect chemical tagging and other fields such as planet formation. We strongly encourage the use of giantgiant pairs. They are a relevant complement to main-sequence pairs for determining the origin of the observed chemical differences in multiple systems.

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HotJupiters are amongthebest-studied exoplanets, but it is still poorly understood how their chemical composition and cloud properties vary with longitude. Theoretical models predict that clouds may condense on the nightside and that molecular abundances can be driven out of equilibrium by zonal winds. Here we report a phase-resolved emission spectrum of the hot Jupiter WASP-43b measured from 5–12µ 5–12µ 5–12µm with JWST’s Mid-Infrared Instrument (MIRI). 1524 ±35 1524 ±35 and 863±23 The spectra reveal a large day–night temperature contrast (with average brightness temperatures of 1524 ± 35 863 ±23 863 ±23Kelvin, respectively) and evidence for water absorption at all orbital phases. Comparisons with three-dimensional atmospheric models show that both the phase curve shape and emission spectra strongly suggest the presence of nightside clouds which become optically thick to thermal emission at pressures greater than ∼100mbar. The dayside is consistent with a cloudless atmosphere above the mid-infrared photosphere. Con3trary to expectations from equilibrium chemistry but consistent with disequilibrium kinetics models, methane is not detected on the nightside (2σ upper limit of 1–6 parts per million, depending on model assumptions).

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Past civilisations have nurtured small populations of those trying to understand and manipulate nature to some advantage in materials, tools, weapons, food, and wealth. However, they never formed communities and lacked the means of recording, communicating, and sharing successes and failures. They also lacked a common framework/philosophy to qualify them as scientists, but that all began to change in the 16th Century. In this lecture we consider the progression to a philosophy of science, and the underlying principles and assumptions that now guide scientific inquiry.We also examines the nature of scientific knowledge, the methods of acquisition, evolution, and significance over past centuries, and reflect on the value to society. In the struggle to solve problems, deliver understanding, and reveal the truth about our universe, science had to suffer and survive: ignorance, bigotry, established superstitions, and the ‘diktats’ of religions and politics, and latterly, falling education standards mired by social media. We chart that ‘scientific’ journey emphasising the importance of observation, experimentation, and the search for universal laws. Ultimately, this essentially Aristotelian perspective was challenged and overtaken by the rise of empiricism, which emphasised the importance of sensory experience and the limitations of human knowledge. Science continues to evolve and provide us with the best truths attainable with our leading edge technologies of observation and experimentation. Today, it stands as the greatest and richest contributor to human knowledge, understanding, progress, and wellbeing. In turn, debates and controversies are ongoing, shaping the field and philosophy which remains essential for understanding the nature of scientific knowledge and the models it creates. But unlike any belief system, the answers and models furnishers by science are not certain and invariant, they tend to be stochastic and incomplete - ‘the best we can do’ at a given time.

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1. Nursing Informatics: Where Caring and Technology Meet

2. Publisher : Springer Release Date :

3. ISBN : 0387989234 Author : Download Here http://eap-books.club/readonline/?item=0387989234&lan=en

4. Since publication of the first edition in 1988, this book has established itself as the premier reference text for nurses, nursing administrators, nursing students, and other health care professionals who seek a state-of-the-art review of the role of IT in the nursing profession. The third edition of this seminal work keeps readers at the forefront of the rapidly evolving field of nursing informatics, examining new trends and thoroughly updating and revising all content. New chapters include: Selecting a Nursing Informatics Consultant; Project Management; Consumer Informatics; Data Mining; Education (CME, Patient); Electronic Medical Imaging; Nursing Informatics Competencies; Telehealth and Implications; Business Process Reengineering; Nursing's Role in Telehealth. Download Here http://eap-books.club/readonline/?item=0387989234&lan=en

5. Download Here http://eap- books.club/readonline/?item=0387989234&lan=en Powered by TCPDF (www.tcpdf.org)