Polarization In Spectral Lines
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Author |
: M. Landi Degl'Innocenti |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 899 |
Release |
: 2006-05-17 |
ISBN-10 |
: 9781402024153 |
ISBN-13 |
: 1402024150 |
Rating |
: 4/5 (53 Downloads) |
Synopsis Polarization in Spectral Lines by : M. Landi Degl'Innocenti
The scientific research based on spectropolarimetric techniques is undergoing a phase of rapid growth. Instruments of unprecedented sensitivity are nowadays available, particularly for solar observations. To fully exploit the rich diagnostic content of such observations, it is necessary to understand the physical mechanisms involved in the generation and transfer of polarized radiation in astrophysical (or laboratory) plasmas. After an introductory part based on classical physics, this book tackles the subject by a rigorous quantum-mechanical approach. The transfer equations for polarized radiation and the statistical equilibrium equations for the atomic density matrix are derived directly from the principles of Quantum Electrodynamics. The two sets of equations are then used to present a number of applications, mainly concerning the diagnostics of solar magnetic fields. This book is primarily addressed to scientists working in the field of spectropolarimetry. It may also serve as a textbook for a course at the graduate or advanced undergraduate level.
Author |
: K.N. Nagendra |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 558 |
Release |
: 1999-07-31 |
ISBN-10 |
: 0792358147 |
ISBN-13 |
: 9780792358145 |
Rating |
: 4/5 (47 Downloads) |
Synopsis Solar Polarization by : K.N. Nagendra
Novel instruments for high-precision imaging polarimetry have opened new possibilities, including for exploring effects in radiative scattering, atomic physics, spectral line formation, and radiative transfer. This volume gives a comprehensive and up-to-date account of this rapidly evolving and interdisciplinary field of science.
Author |
: Jose Carlos del Toro Iniesta |
Publisher |
: Cambridge University Press |
Total Pages |
: 247 |
Release |
: 2003-03-06 |
ISBN-10 |
: 9781139436502 |
ISBN-13 |
: 1139436503 |
Rating |
: 4/5 (02 Downloads) |
Synopsis Introduction to Spectropolarimetry by : Jose Carlos del Toro Iniesta
Spectropolarimetry embraces the most complete and detailed measurement and analysis of light, as well as its interaction with matter. This book provides an introductory overview of the area, which plays an increasingly important role in modern solar observations. Chapters include a comprehensive description of the polarization state of polychromatic light and its measurement, an overview of astronomical (solar) polarimetry, the radiative transfer equation for polarized light, and the formation of spectral lines in the presence of a magnetic field. Most topics are dealt with within the realm of classical physics, although a small amount of quantum mechanics is introduced where necessary. This text will be a valuable reference for graduates and researchers in astrophysics, solar physics and optics.
Author |
: Takashi Fujimoto |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 384 |
Release |
: 2007-12-22 |
ISBN-10 |
: 9783540735878 |
ISBN-13 |
: 3540735879 |
Rating |
: 4/5 (78 Downloads) |
Synopsis Plasma Polarization Spectroscopy by : Takashi Fujimoto
You’ll learn all the underlying science and how to perform all the latest analytical techniques that plasma polarization spectroscopy (PPS) offers with this new book. The authors report on recent results of laboratory experiments, keeping you current with all the latest developments and applications in the field. There is also a timely discussion centered on instrumentation that is crucial to your ability to perform successful PPS experiments.
Author |
: John R. Ferraro |
Publisher |
: Academic Press |
Total Pages |
: 385 |
Release |
: 2012-12-02 |
ISBN-10 |
: 9780323137904 |
ISBN-13 |
: 0323137903 |
Rating |
: 4/5 (04 Downloads) |
Synopsis Introductory Raman Spectroscopy by : John R. Ferraro
Praise for Introductory Raman Spectroscopy - Highlights basic theory, which is treated in an introductory fashion - Presents state-of-the-art instrumentation - Discusses new applications of Raman spectroscopy in industry and research
Author |
: Achim Gandorfer |
Publisher |
: vdf Hochschulverlag AG |
Total Pages |
: 200 |
Release |
: 2005 |
ISBN-10 |
: 3728130184 |
ISBN-13 |
: 9783728130181 |
Rating |
: 4/5 (84 Downloads) |
Synopsis The Second Solar Spectrum by : Achim Gandorfer
Author |
: Sergi Kazantsev |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 218 |
Release |
: 2013-03-09 |
ISBN-10 |
: 9789401727082 |
ISBN-13 |
: 9401727082 |
Rating |
: 4/5 (82 Downloads) |
Synopsis Polarization Spectroscopy of Ionized Gases by : Sergi Kazantsev
Polarization Spectroscopy of Ionized Gases describes the physical principles of the technique and its applications to remote sensing. Transport phenomena and local anisotropies can be studied. The theoretical part of the book considers the basic phenomena of the ordering of the velocities of fast exciting charged particles. The polarization of the outer electron shells of excited atoms or molecules is described, and a variety of effects are examined in detail. An integral equation is derived which gives the intensity and polarization of emitted lines. Methods for solving the equation are analyzed. Universal spectropolarimetric remote sensing has been applied to low pressure gas discharges in the laboratory and to non-thermal processes in the solar atmosphere. For researchers interested in the remote sensing of ionized gases.
Author |
: Ashok Ambastha |
Publisher |
: CRC Press |
Total Pages |
: 268 |
Release |
: 2020-03-27 |
ISBN-10 |
: 9781000760873 |
ISBN-13 |
: 1000760871 |
Rating |
: 4/5 (73 Downloads) |
Synopsis Physics of the Invisible Sun by : Ashok Ambastha
Physics of the invisible Sun: Instrumentation, Observations, and Inferences provides a new updated perspectives of the dramatic developments in solar physics mainly after the advent of the space era. It focusses on the instrumentation exploiting the invisible windows of the electromagnetic spectrum for observing the outer, fainter layers of the Sun. It emphasizes on the several technical and observational challenges and proceeds to discuss the discoveries related to energetic phenomena occurring in the transition region and corona. The book begins with giving a brief glimpse of the historical developments during the pre-, and post-telescopic periods of visible and spectroscopic techniques, ground-based optical and radio observing sites. Various types of telescopes and back-end instrumentation are presented based on photometry, spectroscopy, and polarimetry using the Zeeman and Hanle effects for measurement of magnetic fields, and Doppler effect for radial velocity measurements. The book discusses theoretical and observational inferences based on detection of solar neutrinos, and helioseismology as the probes of the hidden solar interior, and tests of solar standard models. The characteristic properties and observational signatures of global solar p- and g-oscillations modes, developments in local helioseismology and asteroseismology are discussed. The role of the solar magnetic field and differential rotation in the activity and magnetic cycles, prediction methodologies, and dynamo models are described. Observing the Sun in IR at the longer, and the UV, EUV, XUV, X-rays, and gamma-rays at the shorter wavelengths are covered in detail. Observational challenges at each of these wavelengths are presented followed by the instrumentation for detection and imaging that have resulted in enhancing the understanding of various solar transient phenomena, such as, flares and CMEs. The outer most corona is described as a dynamic, expanding component of the Sun from the theoretical and observational perspectives of the solar wind. It then discusses the topics of the Interplanetary magnetic field, slow and fast solar wind, interaction with magnetised and non-magnetised objects of the solar system, the space weather and the physics of the heliosphere. The chapter on the future directions in solar physics presents a brief overview of the new major facilities in various observing windows, and the future possibilities of observing the Sun from ground and vantage locations in space. Features: Systematic overview of the developments in instrumentation, observational challenges and inferences derived from ground-based and space-borne solar projects. Advances in the understanding about the solar interior from neutrinos and helioseismology. Recent research results and future directions from ground- and space-based observations. This book may serve as a reference book for scientific researchers interested in multi-wavelength instrumentation and observational aspects of solar physics. It may also be used as a textbook for a graduate-level course.
Author |
: John T. Jefferies |
Publisher |
: |
Total Pages |
: 328 |
Release |
: 1968 |
ISBN-10 |
: UCAL:B4264183 |
ISBN-13 |
: |
Rating |
: 4/5 (83 Downloads) |
Synopsis Spectral Line Formation by : John T. Jefferies
The purpose of this book is to discuss certain aspects of the theory of the formation and analysis of the line spectrum of a hot gas. The underlying motivation for most of the studies discussed here lies in a desire to develop a physically sound procedure for interpreting the line spectrum of a stellar atmosphere ; correspondingly, the major emphasis is given to problems encountered in astrophysics.
Author |
: Jan Olof Stenflo |
Publisher |
: Springer Science & Business Media |
Total Pages |
: 401 |
Release |
: 2013-03-09 |
ISBN-10 |
: 9789401582469 |
ISBN-13 |
: 9401582467 |
Rating |
: 4/5 (69 Downloads) |
Synopsis Solar Magnetic Fields by : Jan Olof Stenflo
Magnetic fields are responsible for much of the variability and structuring in the universe, but only on the Sun can the basic magnetic field related processes be explored in detail. While several excellent textbooks have established a diagnostic foundation for exploring the physics of unmagnetized stellar atmospheres through spectral analysis, no corresponding treatise for magnetized stellar atmospheres has been available. The present monograph fills this gap. The theoretical foundation for the diagnostics of stellar magnetism is developed from first principles in a comprehensive way, both within the frameworks of classical physics and quantum field theory, together with a presentation of the various solar applications. This textbook can serve as an introduction to solar and stellar magnetism for astronomers and physicists at the graduate or advanced undergraduate level and will also become a resource book for more senior scientists with a general interest in cosmic magnetic fields.