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How do you predict the parameters of future solar cycles? What is the role of dynamo theory in the cyclic activity of the Sun and similar stars? And what are the implications of chaos theory for stellar cycles? This book answers these questions and offers a timely review of studies in the cyclic activity of the Sun and other stars. This authoritative reference shows the importance of reliable predictions of the parameters of future solar cycles, and carefully explains the methods currently used to determine these (with special reference to the maximum of cycle 22). Some of the latest research into solar cycles is clearly presented; this includes helioseismology, observations of the extended activity cycle and the polar fields reversal, and contributions from dynamo theory and chaos theory. For graduate students and researchers, this monograph provides a much-needed synthesis of our understanding of activity cycles in the Sun and other stars.
Solar cycle. --- Stars. --- Astrophysics.
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Solar physics --- Astrophysics. --- Solar cycle. --- Stars.
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Solar cycle --- Cycle, Sunspot --- Sun-spot cycle --- Sun-spot period --- Sunspot cycle --- Sunspot period --- Cycles --- Solar activity
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Celebrating the centenary of George Ellery Hale's discovery of magnetic fields in sunspots, IAU Symposium 273 reviews the recent advances made in the fields of solar and stellar magnetism. Sunspots are responsible for the time-varying properties of the Sun, including the solar irradiance. Combined study of the spots on the Sun and on other stars provides a greater understanding of sunspot formation and behaviour on a long-term basis. On the other hand, stellar observations can be best understood by using detailed properties of the Sun as a reference point. This volume contains reviews and research articles from solar and stellar astronomers on the recent findings of solar and stellar magnetism using observational, theoretical and simulation studies of the Sun and the stars to approach the subject in a unified manner. Its findings are useful to advanced students and researchers in solar and stellar astronomy. -- Back cover.
Sunspots --- Starspots --- Solar magnetic fields --- Stars --- Solar activity --- Stellar activity --- Solar cycle --- Magnetic fields --- Sun --- Active regions
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This book offers an overview of solar physics with a focus on solar activity, particularly the activity cycle. It is known that solar activity varies periodically, but there are also phases of intermittency, such as the Maunder minimum, during which solar activity is very low or high over several decades. The book provides a brief introduction to chaos theory and investigates solar activity in terms of its chaotic behavior. It also discusses how intermittent phases of solar activity have affected and can affect Earth’s climate and long-term space weather, and reviews the underlying theories relating to the solar dynamo mechanism. Furthermore, each chapter includes references to scientific literature (review articles and papers) so that readers can delve deeper into the subjects covered. This richly illustrated book will appeal to a wide readership, and is also useful as a textbook for courses in solar physics and astrophysics.
Solar system. --- Geophysics. --- Solar and Heliospheric Physics . --- Geophysics/Geodesy. --- Geological physics --- Terrestrial physics --- Earth sciences --- Physics --- Solar cycle. --- Cycle, Sunspot --- Sun-spot cycle --- Sun-spot period --- Sunspot cycle --- Sunspot period --- Cycles --- Solar activity
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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.
Meteorology. --- Solar cycle. --- Sun -- Evolution. --- Solar cycle --- Helioseismology --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astronomy - General --- Astrophysics --- Solar activity --- History. --- Solar system --- Physics. --- Planetology. --- Atmospheric sciences. --- Astronomy. --- Astrophysics. --- Cosmology. --- Geophysics. --- Astronomy, Astrophysics and Cosmology. --- Atmospheric Sciences. --- Geophysics and Environmental Physics. --- Milky Way --- Solar radiation --- Stellar activity --- Planetary sciences --- Planetology --- Geological physics --- Terrestrial physics --- Earth sciences --- Physics --- Atmospheric sciences --- Atmosphere --- Astronomical physics --- Astronomy --- Cosmic physics --- Sun --- Evolution.
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A collection of papers edited by four experts in the field, this book sets out to describe the way solar activity is manifested in observations of the solar interior, the photosphere, the chromosphere, the corona and the heliosphere. The 11-year solar activity cycle, more generally known as the sunspot cycle, is a fundamental property of the Sun. This phenomenon is the generation and evolution of magnetic fields in the Sun’s convection zone, the photosphere. It is only by the careful enumeration and description of the phenomena and their variations that one can clarify their interdependences. The sunspot cycle has been tracked back about four centuries, and it has been recognized that to make this data set a really useful tool in understanding how the activity cycle works and how it can be predicted, a very careful and detailed effort is needed to generate sunspot numbers. This book deals with this topic, together with several others that present related phenomena that all indicate the physical processes that take place in the Sun and its exterior environment. The reviews in the book also present the latest theoretical and modelling studies that attempt to explain the activity cycle. It remains true, as has been shown in the unexpected characteristics of the first two solar cycles in the 21st century, that predictability remains a serious challenge. Nevertheless, the highly expert and detailed reviews in this book, using the very best solar observations from both ground- and space based telescopes, provide the best possible report on what is known and what is yet to be discovered. Originally published in Space Science Reviews, Vol 186, Issues 1-4, 2014.
Physics. --- Extraterrestrial Physics, Space Sciences. --- Astrophysics and Astroparticles. --- Astrophysics. --- Physique --- Astrophysique --- Science. --- Solar activity. --- Solar cycle. --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astrophysics --- Space sciences. --- Solar radiation --- Stellar activity --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Science and space --- Space research --- Cosmology --- Science
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