LDR | | 05296cmm u2200661Ii 4500 |
001 | | 000000314986 |
003 | | OCoLC |
005 | | 20230525165702 |
006 | | m d |
007 | | cr |n||||||||| |
008 | | 170811s2017 nju o 001 0 eng d |
020 | |
▼a 1400888204
▼q (electronic bk.) |
020 | |
▼a 9781400888207
▼q (electronic bk.) |
020 | |
▼z 0691162921 |
035 | |
▼a 1510362
▼b (N$T) |
035 | |
▼a (OCoLC)1000395127 |
037 | |
▼a 1025994
▼b MIL |
037 | |
▼a 22573/ctt1vwmmbf
▼b JSTOR |
040 | |
▼a IDEBK
▼b eng
▼e rda
▼c IDEBK
▼d N$T
▼d OCLCQ
▼d N$T
▼d EBLCP
▼d YDX
▼d OCLCF
▼d COO
▼d JSTOR
▼d 248032 |
049 | |
▼a MAIN |
050 | 4 |
▼a QB539.I5 |
072 | 7 |
▼a SCI
▼x 004000
▼2 bisacsh |
072 | 7 |
▼a SCI043000
▼2 bisacsh |
072 | 7 |
▼a SCI005000
▼2 bisacsh |
072 | 7 |
▼a SCI015000
▼2 bisacsh |
072 | 7 |
▼a SCI004000
▼2 bisacsh |
082 | 04 |
▼a 523.8
▼2 23 |
100 | 1 |
▼a Basu, Sarbani,
▼e author. |
245 | 10 |
▼a Asteroseismic data analysis :
▼b foundations and techniques /
▼c Sarbani Basu and William J. Chaplin.
▼h [electronic resource] |
260 | 1 |
▼a Princeton :
▼b Princeton University Press,
▼c [2017] |
300 | |
▼a 1 online resource. |
336 | |
▼a text
▼b txt
▼2 rdacontent |
337 | |
▼a computer
▼b c
▼2 rdamedia |
338 | |
▼a online resource
▼b cr
▼2 rdacarrier |
490 | 1 |
▼a Princeton series in modern observational astronomy |
500 | |
▼a Includes index. |
505 | 0 |
▼a 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 |
505 | 8 |
▼a 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 |
505 | 8 |
▼a 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 |
505 | 8 |
▼a 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 |
505 | 8 |
▼a 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 |
588 | 0 |
▼a Online resource; title from PDF title page (EBSCO, viewed August 24, 2017). |
590 | |
▼a Master record variable field(s) change: 072 |
650 | 0 |
▼a Astroseismology. |
650 | 0 |
▼a Stellar oscillations. |
650 | 7 |
▼a SCIENCE / Astronomy.
▼2 bisacsh |
650 | 7 |
▼a Astroseismology.
▼2 fast
▼0 (OCoLC)fst00819819 |
650 | 7 |
▼a Stellar oscillations.
▼2 fast
▼0 (OCoLC)fst01132957 |
650 | 7 |
▼a SCIENCE / Research & Methodology
▼2 bisacsh |
655 | 4 |
▼a Electronic books. |
700 | 1 |
▼a Chaplin, William J.,
▼e author. |
830 | 0 |
▼a Princeton series in modern observational astronomy. |
856 | 40 |
▼3 EBSCOhost
▼u http://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&db=nlabk&AN=1510362 |
938 | |
▼a YBP Library Services
▼b YANK
▼n 14643160 |
938 | |
▼a EBL - Ebook Library
▼b EBLB
▼n EBL5015553 |
938 | |
▼a ProQuest MyiLibrary Digital eBook Collection
▼b IDEB
▼n cis38414397 |
938 | |
▼a EBSCOhost
▼b EBSC
▼n 1510362 |
990 | |
▼a 관리자 |
994 | |
▼a 92
▼b N$T |