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Asteroseismic data analysis : foundations and techniques / [electronic resource]
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| 자료유형 | E-Book |
|---|---|
| 개인저자 | Basu, Sarbani, author. Chaplin, William J., author. |
| 서명/저자사항 | Asteroseismic data analysis :foundations and techniques /Sarbani Basu and William J. Chaplin.[electronic resource] |
| 발행사항 | Princeton : Princeton University Press, [2017] |
| 형태사항 | 1 online resource. |
| 총서사항 | Princeton series in modern observational astronomy |
| 소장본 주기 | Master record variable field(s) change: 072 |
| ISBN | 1400888204 9781400888207 |
| 일반주기 |
Includes index.
|
| 내용주기 | Cover; Title; Copyright; Contents; Preface and Acknowledgments; 1 Introduction; 1.1 The Different Types of Pulsators; 1.2 A Brief History of the Study of Solar-Type Oscillations; 1.3 Overview of the Data; 1.4 Scope of This Book; 1.5 Further Reading; 1.6 Exercises; 2 Theoretical Underpinnings: Modeling Stars; 2.1 The Equations of Stellar Structure and Evolution; 2.2 The Question of ?? 2.3 Other Physical Processes; 2.4 Boundary Conditions; 2.5 Inputs to Stellar Models; 2.6 Modeling a Star; 2.7 Constructing Solar Models; 2.8 Constructing Stellar Models of a Given Mass, Radius, and Teff 2.9 Further Reading2.10 Exercises; 3 Theoretical Underpinnings: Stellar Oscillations; 3.1 The Equations of Stellar Oscillations; 3.2 Properties of Stellar Oscillations; 3.3 Changes in Frequencies in Response to Changes in Stellar Structure; 3.4 The Effects of Acoustic Glitches; 3.5 The Effects of Rotation; 3.6 Mode Excitation; 3.7 Further Reading; 3.8 Exercises; 4 Observational Data: Overview and Fundamentals; 4.1 Spatial Response of the Observations; 4.2 Photometric and Doppler Velocity Observations; 4.3 Other Contributions to the Observed Data; 4.4 Further Reading; 4.5 Exercises 5 Observational Data: Detailed Characteristics in the Frequency Domain5.1 Power Spectrum Estimation; 5.2 Statistics of the Power Spectrum; 5.3 Solar-Like Oscillations in the Frequency Domain; 5.4 Global Properties of the Oscillation Spectrum; 5.5 Frequency Spectrum of Granulation and Active-Region Signal; 5.6 Harmonic Structure from Transits, Eclipses, and Stellar Rotation; 5.7 Super-Nyquist Asteroseismology; 5.8 Further Reading; 5.9 Exercises; 6 Observational Data: Analysis of the Frequency Spectrum; 6.1 Statistical Tests: Example of Detection of Signatures of Individual Modes 6.2 Automated Detection of Oscillation Spectra6.3 Fundamentals of Peak-Bagging: Extraction of Individual Mode Parameters; 6.4 Peak-Bagging: Practicalities and Challenges; 6.5 Challenges for Peak-Bagging Posed by Mixed Modes; 6.6 Further Reading; 6.7 Exercises; 7 Drawing Inferences from Average Seismic Parameters; 7.1 The Direct Method; 7.2 Grid-Based Modeling; 7.3 Further Reading; 7.4 Exercises; 8 Interpreting Frequencies of Individual Modes: Comparing Frequencies; 8.1 Choosing the Physics of Models; 8.2 Effects of Different Model Parameters; 8.3 A Complicating Factor: The Surface Term 8.4 Common Ways of Constructing Models to Fit Frequencies8.5 Dealing with Avoided Crossings in Subgiants; 8.6 Modeling Red Giants; 8.7 Alternative Methods for Fitting Frequencies; 8.8 Analysis of Rotation; 8.9 Further Reading; 8.10 Exercises; 9 Interpreting Frequencies of Individual Modes: Other Diagnostics; 9.1 Learning from Combinations of Frequencies; 9.2 Fitting and Interpreting the Signature of Acoustic Glitches; 9.3 Analysis of Red Giants; 9.4 Further Reading; 9.5 Exercises; 10 Inverting Mode Frequencies; 10.1 The Inversion Equation; 10.2 The Regularized Least Squares Technique |
| 일반주제명 | Astroseismology. Stellar oscillations. SCIENCE / Astronomy. Astroseismology. Stellar oscillations. SCIENCE / Research & Methodology |
| 언어 | 영어 |
| 대출바로가기 | http://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&db=nlabk&AN=1510362 |
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