Monitoring the Earth is the first book to review the recent advances in satellite technology, computing and mass spectrometry that are opening up completely new avenues of enquiry to Earth scientists. Among the geological changes that were previously considered too slow or too extensive for direct measurements and that can now be monitored directly are continental displacements, mountain uplift, the growth and decay of icesheets and glaciers, the faulting and folding of rocks, the progress of weathering and sedimentation, and the growth of coral reefs. In addition to these developments, the book assesses progress in fields not normally considered part of physical geology, such as the shape and orbit of the gravity and the terrestrial magnetic field. The results from the new findings are already helping Earth scientists analyze and explain the underlying mechanisms, notably with regard to the storage and release of strain during earthquakes and the interaction of glacial history with the Earth's rate of rotation. The outcoe is a foretaste of the physical geology of the space age.lly illustrated with line drawings and photographs, and ith a bibliography that encompasses the scattered and disparate litarature, Monitoring the Earth is intended for undergraduates in geology, geomorphology, geomatic engineering and planetary science, but it should also be of interest to astronomers and historians of science.
There are several billion stars in the Milky Way galaxy. One of them is the middle-aged G2V yellow dwarf that rules our lives. The Sun Today discusses the Sun’s appearance and composition, its internal workings, and the various kinds of radiation it emits, and it puts forward a novel explanation for coronal heating. The book draws on the findings of telescopic observation, space missions, and technical and theoretical advances in many fields, and shows why we need to know more if we are to understand and manage our foothold in the Universe. From the reviews of other books by Claudio Vita-Finzi: The Sun – A User’s Manual (2008) ....this, jargon-free, concise, beautifully illustrated and eminently readable book... D.W. Hughes, Times Literary Supplement Solar History (2013) ....a book that is supremely informative, intensely stimulating and enjoyable to read... Ian Seymour, Astronomy Now A History of the Solar System (2016) ...there is a huge amount of useful information in this book that would benefit anyone who needed more detail than is available in a typical popular science title. Brian Clegg, Popular Science
This well illustrated book presents a compact history of the Solar System from its dusty origins 4,600,000 years ago to the present day. Its primary aim is to show how the planets and their satellites, comets, meteors, interplanetary dust, solar radiation and cosmic rays continually interact, sometimes violently, and it reflects humanity's progress in exploring and interpreting this history. The book is intended for a general readership at a time when human and robotic exploration of space is often in the news and should also appeal to students at all levels. It covers the essentials but refers to a large literature which can be accessed via the internet.
In a dynamic treatment of planets of the Solar System from a unified perspective Planetary Geology deals with the origin of planetary bodies, the forces that fashion their surfaces, the rise and fall of icecaps and oceans, and the role of life in planetary history.
This is an account of the many ways in which the Sun affects our planet, how its influence has changed over the last few centuries and millennia, and the extent to which we can predict its future impact. The book is the first to integrate astronomical, geological, climatic and social aspects of the Sun. It includes a topical treatment of solar contribution to global warming, and demonstrates how wild and variable is the so-called Solar Constant. Our nearest star is a complex machine which needs to be treated with caution, and this book will equip every reader with the knowledge that is required to understand the benefits and dangers it can bring.
Beyond the four centuries of sunspot observation and the five decades during which artificial satellites have monitored the Sun – that is to say for 99.99999% of the Sun’s existence – our knowledge of solar history depends largely on analogy with kindred main sequence stars, on the outcome of various kinds of modelling, and on indirect measures of solar activity. They include the analysis of lunar rocks and meteorites for evidence of solar flares and other components of the solar cosmic-ray (SCR) flux, and the measurement of cosmogenic isotopes in wood, stratified ice and marine sediments to evaluate changes in the galactic cosmic-ray (GCR) flux and thus infer changes in the sheltering magnetic fields of the solar wind. In addition, shifts in the global atmospheric circulation which appear to result from cyclic fluctuations in solar irradiance have left their mark in river sediments and in the isotopic composition of cave deposits. In this volume the results these sources have already produced have been summarised, paying special attention to those that reflect processes in different parts of the Sun’s interior and that display periodicities and trends which may enable us to forecast future large-scale environmental changes.
There are several billion stars in the Milky Way galaxy. One of them is the middle-aged G2V yellow dwarf that rules our lives. The Sun Today discusses the Sun’s appearance and composition, its internal workings, and the various kinds of radiation it emits, and it puts forward a novel explanation for coronal heating. The book draws on the findings of telescopic observation, space missions, and technical and theoretical advances in many fields, and shows why we need to know more if we are to understand and manage our foothold in the Universe. From the reviews of other books by Claudio Vita-Finzi: The Sun – A User’s Manual (2008) ....this, jargon-free, concise, beautifully illustrated and eminently readable book... D.W. Hughes, Times Literary Supplement Solar History (2013) ....a book that is supremely informative, intensely stimulating and enjoyable to read... Ian Seymour, Astronomy Now A History of the Solar System (2016) ...there is a huge amount of useful information in this book that would benefit anyone who needed more detail than is available in a typical popular science title. Brian Clegg, Popular Science
This is an account of the many ways in which the Sun affects our planet, how its influence has changed over the last few centuries and millennia, and the extent to which we can predict its future impact. The book is the first to integrate astronomical, geological, climatic and social aspects of the Sun. It includes a topical treatment of solar contribution to global warming, and demonstrates how wild and variable is the so-called Solar Constant. Our nearest star is a complex machine which needs to be treated with caution, and this book will equip every reader with the knowledge that is required to understand the benefits and dangers it can bring.
Beyond the four centuries of sunspot observation and the five decades during which artificial satellites have monitored the Sun – that is to say for 99.99999% of the Sun’s existence – our knowledge of solar history depends largely on analogy with kindred main sequence stars, on the outcome of various kinds of modelling, and on indirect measures of solar activity. They include the analysis of lunar rocks and meteorites for evidence of solar flares and other components of the solar cosmic-ray (SCR) flux, and the measurement of cosmogenic isotopes in wood, stratified ice and marine sediments to evaluate changes in the galactic cosmic-ray (GCR) flux and thus infer changes in the sheltering magnetic fields of the solar wind. In addition, shifts in the global atmospheric circulation which appear to result from cyclic fluctuations in solar irradiance have left their mark in river sediments and in the isotopic composition of cave deposits. In this volume the results these sources have already produced have been summarised, paying special attention to those that reflect processes in different parts of the Sun’s interior and that display periodicities and trends which may enable us to forecast future large-scale environmental changes.
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