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Author: Kenneth J. H. Phillips
Publisher: Cambridge University Press
Published: 2008-06-26
Total Pages: 0
ISBN-13: 0521841607
DOWNLOAD EBOOKThis book explores features of the Sun's atmosphere, for graduate students/researchers in astrophysics and solar physics.
Author: Eric H. Silver
Publisher: Cambridge University Press
Published: 2004-01-29
Total Pages: 636
ISBN-13: 9780521548168
DOWNLOAD EBOOKUp-to-date accounts of recent and future advances in short-wavelength spectroscopy of laboratory and cosmic plasmas.
Author: Charles Philip Sonett
Publisher: University of Arizona Press
Published: 1991
Total Pages: 1040
ISBN-13: 9780816512973
DOWNLOAD EBOOKAn interdisciplinary approach to solar physics, as eighty-nine contributors trace the evolution of the Sun and provide a review of our current understanding of both its structure and its role in the origin and evolution of the solar system.
Author: Prabhakar Misra
Publisher: CRC Press
Published: 2002-02-25
Total Pages: 604
ISBN-13: 9780203908327
DOWNLOAD EBOOKThis volume presents a complete and thorough examination of advances in the instrumentation, evaluation, and implementation of UV technology for reliable and efficient data acquisition and analysis. It provides real-world applications in expanding fields such as chemical physics, plasma science, photolithography, laser spectroscopy, astronomy and a
Author: M. Vázquez
Publisher: Springer Science & Business Media
Published: 2006-06-30
Total Pages: 387
ISBN-13: 1402037309
DOWNLOAD EBOOKIn the history of science the opening up of a new observational or experimental window is always followed by an increase in knowledge of the subject concerned. This is also the case with the subject of this book, ultraviolet radiation (hereafter UV). In principle, the ultraviolet range might be just one more of these windows, of no particular importance. However, the energy per UV photon provides the main peculiarity, its magnitude being great enough to produce important ch- ical reactions in the atmospheres of planets and satellites, thereby a?ecting the transmission of this radiation to the ground. The Sun is the main natural source of UV radiation in the Solar System and our planet is the body where its in?uences can be best tested and the only one where its relation with life can be studied. However, the terrestrial atmosphere blocksmostofthephotonsinthiselectromagneticrangeandastronomershavehad to develop various techniques (balloons, planes and rockets) to cross this barrier and access the information. These tools have been used in parallel to investigate the physical properties of the terrestrial atmosphere and the interaction of its constituents with light. This book will addresses most of these topics.
Author: Janice L. Bishop
Publisher: Cambridge University Press
Published: 2019-11-28
Total Pages: 655
ISBN-13: 110718620X
DOWNLOAD EBOOKComprehensive overview of the spectroscopic, mineralogical, and geochemical techniques used in planetary remote sensing.
Author: International Astronomical Union. Colloquium
Publisher: Cambridge University Press
Published: 1990-04-26
Total Pages: 444
ISBN-13: 9780521370189
DOWNLOAD EBOOKThis book gives an account of the proceedings of the International Astronomical Union Colloquium 115: High Resolution X-Ray Spectroscopy of Cosmic Plasmas. This was the first IAU meeting dedicated to high resolution X-ray spectroscopy of objects outside the solar system. A broad range of objects and astrophysical conditions are discussed. Results from the first generation of satellites with spectroscopic capability, i.e. the Einstein Observatory, EXOSAT, and Tenma, are reviewed from a perspective of a more precise interpretation allowed by improved theoretical models and plasma diagnostics. Laboratory and solar X-ray results that model or are relevant to conditions found in cosmic X-ray sources are also presented. The colloquium presents a forum for discussion of scientific objectives of new international missions in high resolution X-ray spectroscopy.
Author: G. J. Tallents
Publisher: Cambridge University Press
Published: 2018-02-22
Total Pages: 313
ISBN-13: 1108318010
DOWNLOAD EBOOKPlasmas comprise more than 99% of the observable universe. They are important in many technologies and are key potential sources for fusion power. Atomic and radiation physics is critical for the diagnosis, observation and simulation of astrophysical and laboratory plasmas, and plasma physicists working in a range of areas from astrophysics, magnetic fusion, and inertial fusion utilise atomic and radiation physics to interpret measurements. This text develops the physics of emission, absorption and interaction of light in astrophysics and in laboratory plasmas from first principles using the physics of various fields of study including quantum mechanics, electricity and magnetism, and statistical physics. Linking undergraduate level atomic and radiation physics with the advanced material required for postgraduate study and research, this text adopts a highly pedagogical approach and includes numerous exercises within each chapter for students to reinforce their understanding of the key concepts.
Author: Markus J. Aschwanden
Publisher: Springer
Published: 2019-05-22
Total Pages: 719
ISBN-13: 3030139565
DOWNLOAD EBOOKThis is a follow-on book to the introductory textbook "Physics of the Solar Corona" previously published in 2004 by the same author, which provided a systematic introduction and covered mostly scientific results from the pre-2000 era. Using a similar structure as the previous book the second volume provides a seamless continuation of numerous novel research results in solar physics that emerged in the new millennium (after 2000) from the new solar missions of RHESSI, STEREO, Hinode, CORONAS, and the Solar Dynamics Observatory (SDO) during the era of 2000-2018. The new solar space missions are characterized by unprecedented high-resolution imaging, time resolution, spectral capabilities, stereoscopy and tomography, which reveal the intricate dynamics of magneto-hydrodynamic processes in the solar corona down to scales of 100 km. The enormous amount of data streaming down from SDO in Terabytes per day requires advanced automated data processing methods. The book focuses exclusively on new research results after 2000, which are reviewed in a comprehensive manner, documented by over 3600 literature references, covering theory, observations, and numerical modeling of basic physical processes that are observed in high-temperature plasmas of the Sun and other astrophysical objects, such as plasma instabilities, coronal heating, magnetic reconnection processes, coronal mass ejections, plasma waves and oscillations, or particle acceleration.
