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William Alexander Percy
In this evocative biography, Benjamin E. Wise presents the singular life of William Alexander Percy (1885-1942), a queer plantation owner, poet, and memoirist from Mississippi. Though Percy is best known as a conservative apologist of the southern racial order, in this telling Wise creates a complex and surprising portrait of a cultural relativist, sexual liberationist, and white supremacist. We follow Percy as he travels from Mississippi around the globe and, always, back again to the Delta. Wise's exploration brings depth and new meaning to Percy's already compelling life story--his prominent family's troubled history, his elite education and subsequent soldiering in World War I, his civic leadership during the Mississippi River flood of 1927, his mentoring of writers Walker Percy and Shelby Foote, and the writing and publication of his classic autobiography, Lanterns on the Levee. This biography sets Percy's life and search for meaning in the context of his history in the Deep South and his experiences in the gay male world of the early twentieth century. In Wise's hands, these seemingly disparate worlds become one.
The House of Percy
Although the novels of Walker Percy represent some of the most prominent work in 20th-century Southern fiction, the Percy family itself has a history that is arguably as compelling as anything he could have created. Behind Percy's prose lurks a legacy of wealth, literary accomplishment, political leadership, depression, and suicide that spans two centuries. In this compelling biography, Wyatt-Brown skilfully combines intensive research and telling insights to produce the unforgettable story of this gifted family. 48 halftones.
The Sun Shines for All
Through a blend of social and media history, the author explores America's transition from a production-oriented society to a culture of consumption. Because of Dana's strong aversion to the consumerism that accompanied industrial capitalism, the Sun became both the conscience and the advocate for New York's working class. In the words of Joseph Pulitzer, Dana transformed the Sun into "the most piquant, entertaining, and without exception, the best newspaper in the world."
The Physics of the Solar Corona and Transition Region
Solar Physics publishes up to two Topical Issues per year that focus on areas of especially vigorous and active research. The present Topical Issue contains papers of recent results on the solar corona, as well as on the transition region and low solar wind. The majority of these papers, which were all refereed in accordance with the standards of Solar Physics, were presented in August 1999 at a workshop held in Monterey, California. The authors were offered the opportunity to present relevant parts of their contributions on an accompanying CD ROM of this Topical Issue. The Sun's magnetic field is responsible for the spectacularly dynamic and intri cate phenomenon that we call the corona. Th...
Flare Observations in the IRIS Era: What Have We Learned, and What’s Next?
Since its launch in 2013, IRIS has observed more than 10 X-class, over 100 M-class and more than 600 C-class flares at unprecedented spatial and temporal resolution. Thanks to the rich diagnostics that cover the physical conditions of the solar atmosphere from the photosphere to the hottest parts of the flaring corona, IRIS observations have provided exciting new results and constraints on flare heating models, significantly expanding our knowledge of how flares are triggered, and how the non-thermal energy is released, propagates downward from the corona, and is deposited in the low atmosphere. At the same time, the new discoveries provided by IRIS have raised new unresolved questions and n...
Heliophysics: Plasma Physics of the Local Cosmos
Heliophysics is a developing scientific discipline integrating studies of the Sun's variability, the surrounding heliosphere, and climatic environments. Over the past few centuries, our understanding of how the Sun drives space weather and climate on the Earth and other planets has advanced at an ever-increasing rate. This volume, the first in this series of three heliophysics texts, integrates such diverse topics for the first time as a coherent intellectual discipline. It emphasises the physical processes coupling the Sun and Earth, allowing insights into the interaction of the solar wind and radiation with the Earth's magnetic field, atmosphere and climate system. It provides a core resource for advanced undergraduates and graduates, and also constitutes a foundational reference for researchers in heliophysics, astrophysics, plasma physics, space physics, solar physics, aeronomy, space weather, planetary science and climate science. Additional online resources, including lecture presentations and other teaching materials, are accessible at www.cambridge.org/9780521110617.
Reconnection of Magnetic Fields
The reconnection of magnetic fields is one of the most fascinating processes in plasma physics, responsible for phenomena such as solar flares and magnetospheric substorms. The concept of reconnection has developed through recent advances in exploring the magnetospheres of the Sun and Earth through theory, computer simulations and spacecraft observations. The great challenge in understanding it stems from balancing the large volumes of plasma and magnetic fields involved with the energy release with the physical mechanism which relies on the strongly localized behavior of charged particles. This book, edited by and with contributions from leading scientists in the field, provides a comprehensive overview of recent theoretical and observational findings concerning the physics of reconnection and the complex structures that may give rise to, or develop from, reconnection. It is intended for researchers and graduate students interested in the dynamics of plasmas.
Basic Maths For Dummies
Basic maths for dummies offers the content people need to improve their basic maths skills. Filled with real world examples and written by a mathematician who specialises in tutoring adults and students, the book also provides practical advice on overcoming maths anxiety and a host of tips, tricks and memory aids.
The Sun and the Heliopsphere as an Integrated System
9 MHDTurbulence in the Heliosphere: Evolution and Intermittency 253 Bruno Bavassano, Roberto Bruno and Vincenzo Carbone 1 Introduction 254 2 MHD Turbulence Evolution 255 2. 1 Ecliptic Turbulence 256 2. 2 Polar Turbulence 258 2. 3 Conclusions on Turbulence Evolution 263 3 Intermittency 264 3. 1 Probability Distribution Functions of Fluctuations and Self-similarity 269 3. 2 Radial Evolution of Intermittency 271 3. 3 Identifying Intermittent Events 273 3. 4 Conclusions on Intermittency 277 10 283 Waves and Turbulence in the Solar Corona Eckart Marsch 1 Introduction 284 2 Coronal Magnetic Field Structures 284 3 Magnetic Network Activity and Coronal Heating 287 4 Waves and Flows in Loops and Funn...
The Dynamic Sun
Our Sun is the nearest star and thus an ideal laboratory to study dynamic processes which are related to solar terrestrial physics. The topics addressed in this book cover solar MHD and generation of acoustic waves, as well as physical parameters that are suited to describing solar activity and could serve as proxies for space weather forecasting. The influence of solar activity (radiation and solar wind) on telecommunication systems, satellite missions etc. is also discussed. In short, contribution reports are given on various topics in solar physics. The book covers solar physics from the photosphere to space weather influences. The intended level of readership is aimed at students working in this or related fields, professionals, and astronomers who wish to acquire some basic knowledge in the field of solar terrestrial relations, which is provided in the review articles.
