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|a 9783642971297
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| 100 |
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|a Stix, Michael
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| 245 |
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|a The Sun
|h Elektronische Ressource
|b An Introduction
|c by Michael Stix
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| 250 |
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|a 1st ed. 1989
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| 260 |
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|a Berlin, Heidelberg
|b Springer Berlin Heidelberg
|c 1989, 1989
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| 300 |
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|a XIII, 390 p
|b online resource
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| 505 |
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|a The Sun’s Distance, Mass, Radius, Luminosity ... -- 1.1 Distance -- 1.2 Mass -- 1.3 Radius -- 1.4 Luminosity -- 1.5 Spectral Energy Distribution -- 1.6 Bibliographical Notes -- 2. Internal Structure -- 2.1 Construction of a Model -- 2.2 Age and Pre-Main-Sequence Evolution -- 2.3 Model Ingredients -- 2.4 Results for a Standard Solar Model -- 2.5 Non-Standard Models -- 2.6 Bibliographical Notes -- 3. Tools for Solar Observation -- 3.1 Limitations -- 3.2 High-Resolution Telescopes -- 3.3 Spectrographs and Spectrometers -- 3.4 Filters and Monochromators -- 3.5 Magnetic Fields and Polarimetry -- 3.6 Special-Purpose Instruments -- 3.7 Bibliographical Notes -- 4. The Atmosphere -- 4.1 Radiative Transfer — Local Thermodynamic Equilibrium -- 4.2 Radiative Transfer — Statistical Equilibrium -- 4.3 Atmospheric Models -- 4.4 The Chemical Composition of the Sun -- 4.5 Bibliographical Notes -- 5. Oscillations -- 5.1 Observations -- 5.2 Linear Adiabatic Oscillations of a Non
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| 653 |
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|a Astronomy, Observations and Techniques
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| 653 |
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|a Astrophysics and Astroparticles
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| 653 |
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|a Geophysics
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| 653 |
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|a Observations, Astronomical
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| 653 |
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|a Astronomy—Observations
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| 653 |
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|a Astrophysics
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| 653 |
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|a Geophysics/Geodesy
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| 041 |
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7 |
|a eng
|2 ISO 639-2
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| 989 |
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|b SBA
|a Springer Book Archives -2004
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| 490 |
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|a Astronomy and Astrophysics Library
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| 856 |
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|u https://doi.org/10.1007/978-3-642-97129-7?nosfx=y
|x Verlag
|3 Volltext
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| 082 |
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|a 520
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| 520 |
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|a As in all other fields of astronomy, progress in instrumentation and observational techniques has in recent years brought a wealth of new information about the sun. This introduction presents a complete overview of solar physics, of what we know and would like to know. The increasing number of observations of solar pheno- mena on neighbouring stars makes this book valuable not only for students specializing in solar physics but also for researchers interested in stellar structure and the solar-stellar connection
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