Results by title

The early development of life, a fundamental question for humankind, requires the presence of a suitable planetary climate. Our understanding of how habitable planets come to be begins with the worlds closest to home. Venus, Earth, and Mars differ only modestly in their mass and distance from the Sun, yet their current climates could scarcely be more divergent. Only Earth has abundant liquid water, Venus has a runaway greenhouse, and evidence for life-supporting conditions on Mars points to a bygone era. In addition, an Earth-like hydrologic cycle has been revealed in a surprising place: Saturn’s cloud-covered satellite Titan has liquid hydrocarbon rain, lakes, and river networks. 
 
Deducing the initial conditions for these diverse worlds and unraveling how and why they diverged to their current climates is a challenge at the forefront of planetary science. Through the contributions of more than sixty leading experts in the field, Comparative Climatology of Terrestrial Planets sets forth the foundations for this emerging new science and brings the reader to the forefront of our current understanding of atmospheric formation and climate evolution. Particular emphasis is given to surface-atmosphere interactions, evolving stellar flux, mantle processes, photochemistry, and interactions with the interplanetary environment, all of which influence the climatology of terrestrial planets. From this cornerstone, both current professionals and most especially new students are brought to the threshold, enabling the next generation of new advances in our own solar system and beyond.

Contents

An integrated discussion of the similarities and differences between the atmospheres of various bodies of the solar system, including the Earth.

 

This volume puts two traditions of scholarship into conversation: Euro-American work on air and atmospheres, and emergent postcolonial debates on these themes. Drawing on the strengths of the first, this collection probes its limits, while mapping an emergent field of postcolonial research on air and atmospheres.

 

Postcolonial Air and Atmospheres recontextualizes debates on atmospheres and aesthetics, exploring these themes in relation to the uneven hemispheric terrains of material decay and toxicity. It extends the narrow spatial purview of the Euro-American scholarship by taking an empire-wide perspective, considering historical questions of air and enslavement alongside South Asian histories of air conditioning and the toxic atmospheres of extractive industries. It develops a phenomenology of breathing in a range of postcolonial settings to revisit the theorizations of air and breath in Western critical theoretical scholarship. The collection comprises three sections. “Affective Atmospheres” explores the materialities of air while foregrounding atmospheres as sites of affect, politics, and power in the postcolony. “Unfree and Impure Airs” foregrounds clean and toxic air and who breathes them, along with the politics and technologies of how these unequal forms of air were and are produced. “Breathing In” centers practices of breath as a means of analyzing air and atmospheres.

This is the first of six volumes collecting significant papers of the distinguished astrophysicist and Nobel laureate S. Chandrasekhar. His work is notable for its breadth as well as for its brilliance; his practice has been to change his focus from time to time to pursue new areas of research. The result has been a prolific career full of discoveries and insights, some of which are only now being fully appreciated.

Chandrasekhar has selected papers that trace the development of his ideas and that present aspects of his work not fully covered in the books he has periodically published to summarize his research in each area.

Volume 1, Stellar Structure and Stellar Atmospheres, covers primarily the period 1930-40 and includes early papers on the theory of white dwarfs. In the Preface, Chandrasekhar explains the criteria for selection and provides historical background. Each subsequent volume will include a foreword by an authority on the topics covered.

This is the second of six volumes collecting significant papers of the distinguished astrophysicist and Nobel laureate S. Chandrasekhar. His work is notable for its breadth as well as for its brilliance; his practice has been to change his focus from time to time to pursue new areas of research. The result has been a prolific career full of discoveries and insights, some of which are only now being fully appreciated.

Chandrasekhar has selected papers that trace the development of his ideas and that present aspects of his work not fully covered in the books he has periodically published to summarize his research in each area.

Volume 2 covers primarily the period 1940-50 and includes papers on the theory of radiative transfer and on the physics and astrophysics of the negative ion of hydrogen. Of particular note are Chandrasekhar's Gibbs Lecture to the American Mathematical Society in 1946 and his "Personal Account" presented at a conference at Erevan in the U.S.S.R. in 1981. A foreword by T. W. Mullikin, a distinguished scholar in the area of radiative transfer, and an author's note provide a historical context for the papers.

An incomparable reference for astrophysicists studying pulsars and other kinds of neutron stars, Theory of Neutron Star Magnetospheres sums up two decades of astrophysical research. It provides in one volume the most important findings to date on this topic, essential to astrophysicists faced with a huge and widely scattered literature.

F. Curtis Michel, who was among the first theorists to propose a neutron star model for radio pulsars, analyzes competing models of pulsars, radio emission models, winds and jets from pulsars, pulsating X-ray sources, gamma-ray burst sources, and other neutron-star driven phenomena. Although the book places primary emphasis on theoretical essentials, it also provides a considerable introduction to the observational data and its organization. Michel emphasizes the problems and uncertainties that have arisen in the research as well as the considerable progress that has been made to date.