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Based on the lecture notes of a school titled ‘Tides in Astronomy and Astrophysics’ that brought together students and researchers, this book focuses on the fundamental theories of tides at different scales of the universe—from tiny satellites to whole galaxies—and on the most recent developments. It also attempts to place the study of tides in a historical perspective. Starting with a general tutorial on tides, the theme of tides is approached in 9 chapters from many directions. They allow non-experts to pick up a physical intuition and a sense of orders of magnitude in the theory of tides. These carefully prepared lecture notes by leaders in the field include many illustrative figures and drawings. Some even offer a variety of simple back-of the-envelope problems.
Taking a transdisciplinary approach to seismology, this unique book reviews the most recent developments in planetary seismology, helioseismology, and asteroseismology.
In the early seventeenth century, Galileo Galilei posited that tides were a consequence of Earths motion. Today weve achieved an accurate understanding of the ways that orbiting objects interact to create visibleand sometimes tangibleeffects on Earth. Earth, Sun, and Moon: Cyclic Patterns of Lunar Phases, Eclipses, and the Seasons explains the cycles that affect our daily lives and how the major figures in astronomy used the scientific method to prove their theories about these cycles in accordance with Next Generation Science Standards.
In Debating the Stars, Ovanes Akopyan sheds new light on the astrological controversies that arose in the late fifteenth and early sixteenth centuries after the publication of Giovanni Pico della Mirandola’s Disputationes adversus astrologiam divinatricem (1496). This treatise has often been held responsible for a contemporary reassessment of the status of astrology, a discipline that attracted widespread fascination in the Renaissance. Akopyan’s reconstruction of the development of Pico’s views demonstrates that the Disputationes was a continuation of rather than a drastic rupture with the rest of his legacy. By investigating the philosophical and humanist foundations for Pico’s attack on astrological predictions, Akopyan challenges the popular assumption that the treatise was written under Girolamo Savonarola’s spell. He shows instead how it was appropriated ideologically by pro-Savonarolan circles after Pico’s death. This book also offers a comprehensive study of the immediate reception of the Disputationes across Italy and Europe and reveals that the debates initiated by Pico’s intervention pervaded all of the European intellectual oikumene.
Based on lectures given at a CNRS summer school in France, this book covers many aspects of stellar environments (both observational and theoretical) and offers a broad overview of the field. More specifically, Part I of the book focuses on the Sun, the properties of the ejected plasma, of the solar wind and on space weather. The second part deals with tides in planetary systems and in binary stellar systems, as well as with interactions in massive binary stars as seen by interferometry. Finally the chapters of Part III discuss the environments of young or evolved stars, stellar winds, agnetic fields and disks. With its broad approach the book will provide advanced students as well as researchers with a good overview of the environments of the Sun and the stars.
The third edition of the definitive international reference book on all aspects of the medical care of older persons will provide every physician involved in the care of older patients with a comprehensive resource on all the clinical problems they are likely to encounter, as well as on related psychological, philosophical, and social issues.
This volume synthesizes the results of work carried out by several international teams of the SIROCO (Seismology for Rotation and Convection) collaboration. It provides the theoretical background required to interpret the huge quantity of high-quality observational data recently provided by space experiments such as CoRoT and Kepler. Asteroseismology allows astrophysicists to test, to model and to understand stellar structure and evolution as never before. The chapters in this book address the two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology". The book offers the reader solid theoretical background knowledge and adapted seismic diagnostic techniques.
Peripheral Nerve Disorders: Pathology and Genetics is a definitive, clinically-oriented guide to the pathology of peripheral nerve disorders. These commonly seen neurological challenges have many causes and accurate diagnosis is often necessary via pathological analysis. New techniques exploiting molecular biological knowledge have opened up new vistas to understanding the pathogenesis of these disorders, and hence their effective management. This new title takes a disease-oriented approach to understanding the pathology of these conditions. It combines classical and contemporary techniques to enable practitioners in neurology and neuropathology to better understanding of the disease processes underlying patients’ presentations and to formulate appropriate management plans. Peripheral Nerve Disorders: Pathology and Genetics is a valuable resource for neurologists, neuropathologists, pathologists, neurobiologists and geneticists.
This volume of lecture notes brings together the knowledge on pulsations of the Sun and the stars, with a particular emphasis on recent observations and modelling, and on the influence of pulsations of other physical processes. The book begins with an extensive introduction to helioseismology. The solar cycle and gravity modes are discussed before the focus is widened from helioseismology to asteroseismology which is detailed in a series of specific chapters. Based on courses given at a graduate school, these tutorial lecture notes will be of interest and useful to a rather broad audience of scientists and students.
Stellar models are the very basic building blocks with which we build up our knowledge of the Universe. New numerical experiments are heralding a new level of sophistication in our ability to model, and understand, how stars work. This volume provides an overview and the most recent advances in modeling of stellar structure and evolution. Modeling of stars relies on our understanding of the detailed physical processes happening in stars, and the most recent observations of stars made by modern large telescopes and current high technologies. IAU Symposium 252 presents the most recent developments in five key areas, including: improvements of the physical ingredients of stellar models; the evolution of low and intermediate mass stars; the evolution of massive stars; close binary evolution; and stellar physics in the era of very large telescopes. This overview of stellar research is at a level suitable for research astronomers and graduate students.