Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere

Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere PDF Author: Kenneth J. H. Phillips
Publisher: Cambridge University Press
ISBN: 0521841607
Category : Science
Languages : en
Pages : 0

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Book Description
This book explores features of the Sun's atmosphere, for graduate students/researchers in astrophysics and solar physics.

Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere

Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere PDF Author: Kenneth J. H. Phillips
Publisher: Cambridge University Press
ISBN: 9781107407916
Category : Science
Languages : en
Pages : 360

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Book Description
The solar atmosphere, above the Sun's surface layers, reaches mega-kelvin temperatures and high levels of dynamic activity through processes involving a pervading magnetic field. This book explores one of the principal means of understanding the solar atmosphere, its ultraviolet and soft X-ray emission. The ultraviolet and X-ray spectra of the Sun's atmosphere provide valuable information about its nature - the heat and density of its various parts, its dynamics, and chemical composition. The principles governing spectral line and continuous emission, and how spectral studies lead to deductions about physical properties, are described, together with spacecraft instrumentation from Skylab, SolarMax, Yohkoh, SOHO, TRACE, and Hinode. With introductions to atomic physics and diagnostic techniques used by solar spectroscopists, a list of emission lines in ultraviolet and soft X-ray regions, and a glossary of terms, this is an ideal reference for graduate students and researchers in astrophysics and solar physics.

Soft X-ray/extreme Ultraviolet Images of the Solar Atmosphere with Normal Incidence Multilayer Optics

Soft X-ray/extreme Ultraviolet Images of the Solar Atmosphere with Normal Incidence Multilayer Optics PDF Author: Joakim Fredrik Lindblom
Publisher:
ISBN:
Category :
Languages : en
Pages : 528

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Book Description


UV and X-Ray Spectroscopy of Laboratory and Astrophysical Plasmas

UV and X-Ray Spectroscopy of Laboratory and Astrophysical Plasmas PDF Author: Eric H. Silver
Publisher: Cambridge University Press
ISBN: 9780521548168
Category : Science
Languages : en
Pages : 636

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Book Description
Up-to-date accounts of recent and future advances in short-wavelength spectroscopy of laboratory and cosmic plasmas.

Absolute Intensity Measurements in the Extreme Ultraviolet Spectrum of Solar Radiation

Absolute Intensity Measurements in the Extreme Ultraviolet Spectrum of Solar Radiation PDF Author: H. E. Hinteregger
Publisher:
ISBN:
Category : Electromagnetic waves
Languages : en
Pages : 48

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Book Description


Ultraviolet Radiation in the Solar System

Ultraviolet Radiation in the Solar System PDF Author: M. Vázquez
Publisher: Springer Science & Business Media
ISBN: 1402037309
Category : Science
Languages : en
Pages : 387

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Book Description
In 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.

The Solar UV-x-Ray Spectrum from 1.5 to 2000 A.

The Solar UV-x-Ray Spectrum from 1.5 to 2000 A. PDF Author:
Publisher:
ISBN:
Category :
Languages : en
Pages : 25

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Book Description
This review illustrates the potential of UV-x-ray spectroscopy for determining the physical conditions in the solar chromosphere, transition region and corona, and how spectroscopy can be used as a tool to understand the physical mechanisms governing the atmosphere. It also illustrates the potential for understanding transient events such as solar flares. This is a vast topic, and therefore the review is necessarily not complete, but we have tried to be as general as possible in showing in particular how solar spectra are currently being used to understand the solar upper atmosphere. The review is intended for non-solar physicists with an interest in spectroscopy as well as for solar physicists who are not specialists in spectroscopy.

Ultraviolet Spectroscopy And Uv Lasers

Ultraviolet Spectroscopy And Uv Lasers PDF Author: Prabhakar Misra
Publisher: CRC Press
ISBN: 9780203908327
Category : Science
Languages : en
Pages : 604

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Book Description
This 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

Solar Ultraviolet Radiation

Solar Ultraviolet Radiation PDF Author: Christos S. Zerefos
Publisher: Springer Science & Business Media
ISBN: 3662033755
Category : Science
Languages : en
Pages : 360

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Book Description
Following the rapid developments in the UV-B measurement techniques and the rapidly growing research in the field in the late 80's and early 90's, we organized a large gathering of distinguished experts in a NATO Advanced Study Institute, held in Halkidiki, Greece on October, 2-11. 1995. The Institute was organized so as to include state of the art lectures on most aspects of solar ultraviolet radiation and its effects. This was achieved by extended lectures and discussions given in five sessions by 27 lecturers and a demonstration of filed measurements and calibration techniques at the end of the Institute. The ASI began with the sun and fundamentals on solar radiative emissions and their variability in time and continued with the interaction of solar Ultraviolet with the atmosphere through the complex scattering processes and photochemical reactions involved. Particular emphasis was given to changes in atmospheric composition imposed by different manifestations of the solar activity cycle. as well as on the modelling of radiative transfer through the atmosphere and the ocean under variable environmental conditions. Overviews on the ozone issue. its monitoring and variability were extensively discussed with emphasis on the observed acceleration of ozone decline in the early 90's. This acceleration had as a consequence, significant increases in UV-B radiation observed at a few world-wide distributed stations.

Scientific and Technical Aerospace Reports

Scientific and Technical Aerospace Reports PDF Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 372

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Book Description


Physics of the Sun

Physics of the Sun PDF Author: P.A. Sturrock
Publisher: Springer Science & Business Media
ISBN: 9401096368
Category : Science
Languages : en
Pages : 394

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Book Description
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.