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Gammie C: Astrophyscial Fluid Mechanics

Astrophyscial Fluid Mechanics

Handbook of Radiation Belts: Physics Throughout the Solar System provides a comprehensive overview of radiation belt processes throughout the solar system in a single book, compiling all information relevant to radiation belts in one place. It features an overview of radiation belts of each applicable planet in the Solar System to assist researchers working on individual radiation belt physics, particularly of comparative or multiplanetary scope. The handbook goes on to offer a detailed guide to basics such as measurement and particle motion to more advanced topics such as radial transport and associated acceleration. It provides the respective theory behind the physics as well as detailed derivations, with worked examples and case studies, allowing readers to follow the implementation of the theory behind the science to apply in their research. The Handbook of Radiation Belts covers all relevant topics to radiation belts in our Solar System in one complete source, offering researchers, academics and students in space physics a complete guide to the topic for those performing fundamental research and teaching, as well as professionals planning and operating space missions or assets.

Physics Throughout the Solar System

Handbook of Radiation Belts

Close your eyes and imagine the last moments of a massive star, large as the Solar System. As the mass of its core approaches a fatidic value, the enormous fabric collapses. The star plasma streams like a monstrous wave inward towards the center of the star. In a fraction of a second the core of the star becomes as dense as an atomic nucleus. And then a mighty outward shock wave forms, disrupting the whole structure, the star becoming almost as bright as the whole galaxy. This explosion is a supernova!Chinese observers studied with care these events since ancient times; the observation of these explosions by Tycho Brahe and Kepler was crucial for the adoption of the Copernican system. Do you know that each drop of your blood contains iron atoms produced in these cosmic cataclysms? We are literally star dust, disseminated in the galactic medium by supernovae.This book guides the reader in the discovery of these rare events, the most spectacular that the Universe can offer. Present models reproduce the explosion only with difficulty, as if some details were wrong, or a whole aspect of physics was missing from the equations. Different aspects of these events are illustrated, as well as their historical and scientific importance and their crucial role in the evolution of the galaxy and the living organisms.

Supernova: The Last Flash Of The Disappearing Star

This book highlights the basic concepts and equations for bioengineering flow processes. Physical concepts and meanings are emphasized while rigorous derivations are simplified, making it easier for self learning on some biological and medical flow processes. The well known Bernoulli equation in hydraulics is extended for pulsating flows, peristaltic flows and cardiac pumping. The dimensional analysis, model law and dimensionless equations can be related to computational models and experimental observations. The velocity vector imaging stored in echocardiograms can be used to analyze the pumping characteristics of the ventricular contraction. New topics included oxygen transport in membrane oxygenator and micro mixing of blood flow in capillary channels.

Bioengineering Fluid Mechanics

Annals of Mathematics Studies

Quasiperiodic Solutions of the Generalized SQG Equation

Handbook of Electronic Structure Theory provides a much-needed learning resource that collects and demonstrates the various key methods involved in electronic structure theory, the feasibility and reliability of electronic structure calculations and their applications using computational chemistry, with a particular focus on the most modern and recent problems which are poorly covered in existing, largely outdated book literature. This handbook is designed with early career researcher learning in mind by aiming to provide a careful, structured, coherent, measured, and incremental presentation of the subject matter as well as appropriate problems and worked tutorial examples. Elements like summary boxes, worked examples, and downloadable data sets make this a holistic guide to the topic for learners from different backgrounds who require a deeper understanding of electronic structure theory. Part I one of the book focuses on the critical core theories, before Part II moves on to some of the most important recent developments and their potential future directions, including key topics such as the electronic excited states and the harnessing of machine learning. Finally, Part III then collects a range of key case study examples of applications such as for biomolecules, in spectroscopy, or for use in catalysis amongst others. Handbook of Electronic Structure Theory is written primarily for masters, PhD, and postdoctoral students in theoretical and computational chemistry as well as experimental researchers wishing to apply quantum chemical methods in a critical way. The book will also have significant relevance to those studying and teaching in the adjacent fields of computational physics, materials science, and astrochemistry, who are making use of electronic structure methods. It is also likely to be of interest to chemists working on designing new materials and compounds targeting industrial and environmental applications such as catalysis, energy harvesting or green chemistry.

Methods and Applications

Handbook of Electronic Structure Theory

Foundations of Biochemistry and Biophysics

The Compressible Fluid Physics of the Human Respiratory System

An expert and contemporary presentation of computational analysis and design tools for professionals studying or applying the principles of aerodynamics In Aerodynamics: A Computational Introduction, a distinguished aerospace engineer and researcher Krzysztof Fidkowski delivers an up-to-date and authoritative reference text covering the essentials of aerodynamics. The book covers key topics, including basic fluid dynamics, potential flow, airfoil theory, boundary layers, wing theory, and compressible flow. Fidkowski takes a computation-first approach to the subject matter, presenting aerodynamics in a way that is compatible with the way the subject is handled in contemporary businesses and research labs. Aerodynamics offers numerical demonstrations, codes, and theory comparisons that make important derivations and conclusions easier to understand and apply. Readers will also find: <ul> <li>A self-contained introduction to the thermodynamics, mathematics, and numerical methods central to the subject of aerodynamics</li> <li>Comprehensive explorations of kinematics, dynamics, and potential flow</li> <li>Practical discussions of panel methods and airfoil theory, including design tools</li> <li>Numerical and analytical tools for boundary-layer analysis</li> <li>Complete treatment of finite-wing theory, including horseshoe vortices, lifting-line theory, and the vortex-lattice method.</li> </ul> Perfect for engineering students who want to learn how to apply basic numerical methods to large-scale aerodynamics problems, Aerodynamics: A Computational Introduction will also benefit professionals who wish to better understand aerodynamics and computational fluid dynamics.

A Computational Introduction

Aerodynamics

Physics of the Tropical Atmosphere and Tropical Cyclones

How do you explore distant stars, buried water on Mars or the first moments after the Big Bang - without leaving your back garden? In The Radio Universe, award-winning astrophysicist Emma Chapman takes us on an electrifying voyage through the cosmos using one of the most powerful, yet overlooked, tools in science: the radio wave. With dazzling clarity and humour, Chapman reveals how these invisible messengers glide through space, bounce off planets, tunnel through clouds and slip past galactic dust - carrying secrets of the universe that no other kind of light can uncover. We follow a single radio wave as it escapes Earth and travels outward - ricocheting off the Moon, tunnelling through Venus's furnace-thick atmosphere, tracing ancient ice hidden in Mercury's shadows and diving deep into the swirling arms of the Milky Way. Along the way, we meet black holes that roar louder than stars, pulsars more precise than atomic clocks and galaxies lit by the very first starlight. We explore volcanic pancake planets, death-defying neutron stars, the eerie possibility of alien broadcasts - and the fragile question of our own future in the cosmos. A celebration of human ingenuity and cosmic curiosity, The Radio Universe reveals that the true frontier of space isn't 'out there' - it's humming quietly all around us, waiting to be heard.

How to Explore Outer Space Without Leaving Earth

The Radio Universe

Dynamics and Astrophysics of Galaxies

Astrophyscial Fluid Mechanics

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