Ultraviolet and x-ray spectroscopy of the solar atmosphere /

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Bibliographic Details
Author / Creator:Phillips, Kenneth J. H.
Imprint:Cambridge, UK ; New York : Cambridge University Press, 2008.
Description:x, 349 p. : ill. ; 26 cm.
Language:English
Series:Cambridge astrophysics series ; 44
Subject:
Format: Print Book
URL for this record:http://pi.lib.uchicago.edu/1001/cat/bib/7302791
Hidden Bibliographic Details
Other authors / contributors:Feldman, U.
Landi, Enrico.
ISBN:9780521841603
0521841607
Notes:Includes bibliographical references (p. 336-345) and index.
Table of Contents:
  • Preface
  • 1. The solar atmosphere
  • 1.1. Introduction
  • 1.2. Chromosphere, transition region, and corona
  • 1.3. The ultraviolet and X-ray spectrum of the solar atmosphere
  • 1.4. Structure of the solar atmosphere
  • 1.5. Dynamics of the solar atmosphere
  • 1.6. The active Sun
  • 1.7. Physical conditions and energy balance
  • 1.8. Ionization and excitation conditions
  • 1.9. Chemical composition
  • 1.10. Solar-type stars
  • 2. Fundamentals of solar radiation
  • 2.1. Wavelength ranges
  • 2.2. Specific intensity and flux
  • 2.3. Radiative transfer and the source function
  • 2.4. Radiation from the solar atmosphere
  • 2.5. Radiant intensity and flux
  • 3. Fundamentals of atomic physics
  • 3.1. Introduction
  • 3.2. The one-electron atom: Bohr's theory
  • 3.3. The one-electron atom: quantum theory
  • 3.4. The multi-electron atom: quantum theory
  • 3.5. Isoelectronic sequences
  • 3.6. Interaction between atoms and electromagnetic fields
  • 3.7. Atomic codes
  • 4. Mechanisms of formation of the solar spectrum
  • 4.1. Introduction
  • 4.2. Collisional excitation and de-excitation of atomic levels
  • 4.3. Level populations
  • 4.4. Ionization and recombination
  • 4.5. Ion populations and ionization equilibrium
  • 4.6. Line radiation
  • 4.7. Continuum radiation
  • 4.8. Spectral line profiles
  • 4.9. Other excitation mechanisms of spectral lines
  • 5. Plasma diagnostic techniques
  • 5.1. Introduction
  • 5.2. Electron density diagnostics
  • 5.3. Electron temperature diagnostics
  • 5.4. Ion temperature diagnostics
  • 5.5. Emission measure diagnostics
  • 5.6. Differential emission measure diagnostics
  • 5.7. Element abundance diagnostics
  • 5.8. Ion abundances
  • 5.9. Plasma dynamics diagnostics
  • 5.10. Magnetic field diagnostics
  • 5.11. Spectral codes for solar corona research
  • 6. Ultraviolet and X-ray emission lines
  • 6.1. Introduction
  • 6.2. The 1-7 A range
  • 6.3. The 7-23 A range
  • 6.4. The 23-170 A range
  • 6.5. The 170-630 A range
  • 6.6. The 630-2000 A range (off-limb spectrum)
  • 6.7. The 630-2000 A range (disk spectrum)
  • 7. Spectrometers and imagers for observing the solar ultraviolet and X-ray spectrum
  • 7.1. Introduction
  • 7.2. Transmittance properties of materials
  • 7.3. Reflectance of VUV, EUV, and X-ray radiation from materials
  • 7.4. Ultraviolet spectrometers
  • 7.5. X-ray spectrometers
  • 7.6. Imaging instruments
  • 7.7. Instrument calibration
  • 7.8. Summary of spacecraft instruments
  • 8. Quiet Sun and coronal holes
  • 8.1. Introduction
  • 8.2. Quiet Sun corona and coronal holes: structure
  • 8.3. Quiet Sun corona and coronal holes: plasma properties
  • 8.4. Quiet Sun transition region
  • 8.5. Non-thermal broadening of ultraviolet emission lines
  • 8.6. Quiet Sun dynamic phenomena
  • 8.7. Coronal waves and oscillations
  • 9. Active regions
  • 9.1. Introduction
  • 9.2. Structure of active regions
  • 9.3. Active region loops
  • 9.4. Active region densities
  • 9.5. Active region transient phenomena
  • 10. Solar flares
  • 10.1. Introduction
  • 10.2. X-ray flare spectra
  • 10.3. Ultraviolet flare spectra
  • 10.4. Flare temperatures and emission measures
  • 10.5. Flare densities
  • 10.6. Flare morphology
  • 10.7. Mass motions in flares
  • 10.8. Non-thermal electrons
  • 10.9. X-ray fluorescence lines in flares
  • 10.10. Ionization equilibrium in flares
  • 10.11. GOES observations of flares
  • 11. Element abundances
  • 11.1. Introduction
  • 11.2. Solar wind abundances
  • 11.3. Abundances in quiet Sun and coronal hole regions
  • 11.4. FIP bias in distinct solar structures
  • 11.5. FIP bias rate of change in the solar atmosphere
  • 11.6. Is the FIP bias magnitude FIP dependent?
  • 11.7. Number of free electrons in the photosphere
  • 11.8. Summary
  • Appendix 1. Units
  • Appendix 2. Line lists
  • Glossary
  • Further reading
  • References
  • Index