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MHD Waves in the Solar Atmosphere

MHD Waves in the Solar Atmosphere
Author: Bernard Roberts
Publisher: Cambridge University Press
Total Pages: 529
Release: 2019-07-18
Genre: Mathematics
ISBN: 1108427669

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Develops a fresh mathematical approach to coronal seismology, explaining oscillatory phenomena by drawing upon original research and complex modelling techniques.


Coupling of the Solar Atmosphere Through MHD Waves

Coupling of the Solar Atmosphere Through MHD Waves
Author: Aishawnnya Sharma
Publisher: A.K. Publications
Total Pages: 0
Release: 2022-12-22
Genre:
ISBN: 9786371085846

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From the dawn of human civilisations, Sun has played a crucial role in the wonderland of the human mind. It has been perceived as a powerful deity in the mythology of many civilisations because of its role in providing the life on Earth. Today, we know that it is an ordinary star, which is centred at our solar system. It bears more than 99% mass of the solar system and holds all the planets in the solar system together by its gravity. The Sun has formed 4.5 billion years ago from the collapse of a giant, rotating cloud of gas and dust, called the solar nebula. It is a Population I star that is rich in heavy elements, and formed from the remnants of the supernova explosion of a previous giant star. It is primarily composed of hydrogen (73%) and helium (25%) with a negligible amount of heavier elements such as oxygen, carbon, neon, silicon, magnesium and iron. The Sun is a main-sequence star with a spectral class of G2V. It is located at a distance of 1.496× 108 km (1 AU) from the Earth and has a radius of 696,342 ± 65 km, which is about 109 times the radius of the Earth. The mass of Sun is 1.9885 × 1030 kg, and its luminosity is 3.86 × 1026 W. The solar spectrum can be approximated by blackbody radiation with a temperature of 5785 K, that corresponds to the effective surface temperature of the Sun . The study of the Sun can be divided into two parts. The solar interior that is composed of the core, the radiative zone and the convective zone, and the solar atmosphere that includes the photosphere, the chromosphere, the transition region and the corona. Solar interior is primarily divided into three main regions based on energy generation and transfer processes. They are - the core, the radiative & the convective zone.


Magnetohydrodynamics of the Sun

Magnetohydrodynamics of the Sun
Author: Eric Priest
Publisher: Cambridge University Press
Total Pages: 581
Release: 2014-04-07
Genre: Science
ISBN: 0521854717

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This advanced textbook reviews the complex interaction between the Sun's plasma atmosphere and its magnetic field.


Physics Of The Sun And Its Atmosphere - Proceedings Of The National Workshop (India) On "Recent Advances In Solar Physics"

Physics Of The Sun And Its Atmosphere - Proceedings Of The National Workshop (India) On
Author: Udit Narain
Publisher: World Scientific
Total Pages: 294
Release: 2008-10-24
Genre: Science
ISBN: 9814470473

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This book presents a pedagogical, updated and modern view of the Sun from its interior to its exterior as well as the Sun-Earth system. Written by eminent scientists in solar physics, the chapters deal with recent advances in solar physics, seismic Sun, solar magnetic field, waves and oscillations, spectroscopic diagnostics of solar plasmas, partially ionized lower atmosphere, coronal heating, coronal mass ejections, radio Sun, solar wind, and the Sun-Earth system. Each chapter is fully illustrated and has a comprehensive reference list. The book covers all major topics in solar physics, and presents a rich menu to motivate graduate students who wish to pursue a solar physics research career.


Advances in Solar System Magnetohydrodynamics

Advances in Solar System Magnetohydrodynamics
Author: Eric Ronald Priest
Publisher: Cambridge University Press
Total Pages: 460
Release: 1991-06-28
Genre: Mathematics
ISBN: 9780521403252

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Most of the solar system is in the plasma state and its subtle non-linear interaction with the magnetic field is described for many purposes by the equations of magnetohydrodynamics (MHD). Over the past few years this important and complex field has become one of the most actively pursued areas of research, with increasingly diverse applications in geophysics, space physics and astrophysics. This book examines the basic MHD topics, such as equilibria, waves, instabilities and reconnection and examines each in the context of different areas that utilize MHD. Many of the world's leading experts have contributed to this volume, which has been edited by two of the key enthusiasts. It is hoped that it can help the reader to appreciate and understand the common threads between the different branches of magnetohydrodynamics. This book will be a timely exposition of recent advances made in the field.


Physics of the Sun

Physics of the Sun
Author: P.A. Sturrock
Publisher: Springer Science & Business Media
Total Pages: 394
Release: 2013-12-01
Genre: Science
ISBN: 9401096368

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This volume, together with its two companion volumes, originated in a study commis sioned by the United States National Academy of Sciences on behalf of the National Aeronautics and Space Administration. A committee composed of Tom Holzer, Dimitri Mihalas, Roger Ulrich and myself was asked to prepare a comprehensive review of current knowledge concerning the physics of the sun. We were fortunate in being able to persuade many distinguished scientists to gather their forces for the preparation of 21 separate chapters covering not only. solar physics but also relevant areas of astrophysics and solar-terrestrial relations. In proved necessary to divide the chapters into three separate volumes that cover three different aspects of solar physics. Volumes I and III are concerned with "The Solar Interior" and with "Astrophysics and Solar-Terrestrial Relations." This volume, devoted to "The Solar Atmosphere," covers not only the chromosphere and corona but also the principal phenomena usually referred to as "solar activity." The emphasis is on identifying and analyzing the relevant physical processes, but each chapter also contains a great deal of descriptive material.