The sun as a guide to stellar physics:
Gespeichert in:
| Weitere Verfasser: | , , |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Amsterdam ; Oxford ; Cambridge, MA
Elsevier
[2019]
|
| Schlagworte: | |
| Online-Zugang: | Inhaltsverzeichnis |
| Beschreibung: | xvii, 504 Seiten Illustrationen, Diagramme 24 cm |
| ISBN: | 9780128143346 |
Internformat
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Datensatz im Suchindex
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| adam_text | Contents List of Contributors................................................................................................. xv Preface.................................................................................................................. xvii CHAPTER 1 Discoveries and Concepts: The Sun’s Role in Astrophysics............................................................... 1 Jack B. Zirker and Oddbjørn Engvold 1. The Solar Constant.......................................................................... 2 2. The Sun’s Chemical Composition...................................................3 2.1 Spectroscopic Methods.............................................................3 2.2 Modeling of the Sun’s Atmosphere......................................... 4 2.3 Settling of Light Elements........................................................ 5 3. Internal Structure and Helioseismology.......................................... 6 3.1 Detection of Oscillatory Pattern................................................6 3.2 Interpretation of Solar Oscillations...........................................7 4. The Magnetic Sun and Its Variability..............................................8 4.1 Solar Cycle................................................................................ 9 4.2 Magnetic Fields.........................................................................9 4.3 Internal Structure and Location of the Magnetic Dynamo................................................................................... 10 5. The Solar Corona and
Wind.......................................................... 11 5.1 The Temperature of the Corona.............................................. 11 5.2 The Shape of the Corona.........................................................13 5.3 The Solar Wind....................................................................... 13 6. Earth-Sun Connection...................................................................14 6.1 Aurora and Geomagnetic Storms............................................14 6.2 The Carrington Event..............................................................15 6.3 Solar Flares, X-Rays and Energetic Particles........................ 16 6.4 Reconnection of Magnetic Fields............................................17 6.5 Coronal Mass Ejections.......................................................... 18 7. Testing Two Concepts.................................................................... 19 7.1 Neutrino Oscillations in the Sun.............................................19 7.2 Testing General Relativity...................................................... 22 8. Concluding Remarks...................................................................... 23 Acknowledgments...............................................................................24 References............................................................................................24
vi Contents CHAPTER 2 Stellar and Solar Chromospheres and Attendant Phenomena....................................................................27 Thomas R. Ayres 1. Introduction.........................................................................................27 2. Why Chromospheres Exist................................................................ 28 2.1 Stellar Convection Zones.......................................................... 28 2.2 The Solar Chromosphere............................................................29 2.3 Stellar Chromospheres................................................................31 2.4 Why Are Chromospheres So Thick?........................................32 2.5 The Wilson—Bappu Effect......................................................... 43 3. The Rotation—Age—Activity Connection.......................................45 3.1 Background................................................................................. 45 3.2 Post—Skumanich Law Insights Into the RotationAge—Activity Connection......................................................... 46 3.3 Theory Behind the Skumanich Law......................................... 50 4. Stellar Activity Cycles...................................................................... 52 References................................................................................................. 56 CHAPTER 3 The Sun’s Atmosphere............................................................. 59 Alexander I. Shapiro, Hardi Peter, and Sami K. Solanki 1.
Introduction........................................................................................ 59 2. Observations of the Solar Atmosphere............................................ 60 3. The Solar Spectrum............................................................................61 4. Physics of the Photosphere/Chromosphere......................................65 4.1 One-Dimensional Models...........................................................65 4.2 Three-Dimensional Models........................................................ 70 5. Physics of the Chromosphere/Corona.............................................. 73 5.1 Coronal Emission and Magnetic Structure...............................74 5.2 Basic Considerations of the Energetics....................................76 5.3 Heating Processes and Modem Models....................................77 5.4 Connection to the Low Atmosphere.........................................78 Acknowledgments.....................................................................................79 References................................................................................................. 79 CHAPTER 4 Helioseismic Inferences on the Internal Structure and Dynamics of the Sun............................ 87 Sarbani Basu and William J. Chaplin 1. Introduction........................................................................................ 88 2. Theoretical Background.................................................................... 89 2.1 Equations Governing Solar Oscillations...................................90
2.2 Properties of Solar Oscillations................................................ 92 2.3 Relating Frequency Changes to Changes in Structure............94
Contents 2.4 Effects of Rotation.................................................................. 97 2.5 Inversions.................................................................................98 3. Inferences About Solar Structure................................................ 100 3.1 Basic Results.........................................................................101 3.2 Base of the Solar Convection Zone......................................102 3.3 The Question of Diffusion.................................................... 103 3.4 Convection Zone Helium Abundance.................................. 104 3.5 The Issue of Solar Composition...........................................106 4. Inferences on Solar Dynamics.....................................................107 4.1 Properties of the Tachocline.................................................. 109 5. Helioseismic Inferences on the Solar Cycle............................... 110 5.1 Changes to Global-Mode Frequencies and Mode Parameters...................................................................110 5.2 Zonal Flows........................................................................... 116 5.3 Meridional Flows...................................................................117 5.4 The 1.3-Year Periodicities Near the Tachocline...................119 5.5 Changes in Even-Order a Coefficients................................. 120 6. Seismic Studies of Other Stars.....................................................120
Acknowledgments.............................................................................. 121 References.......................................................................................... 121 ATMOSPHERIC STRUCTURE, NON-EQUILIBRIUM THERMODYNAMICS AND MAGNETISM CHAPTER 5.1 Spectroscopy and Atomic Physics.......................127 Philip G. Judge 1. Overview...................................................................................... 128 2. Regimes of Solar Plasmas............................................................ 128 3. Origin and Types of Atomic Transitions..................................... 132 4. Atomic Structure.......................................................................... 133 5. Spectrum Formation in a Nutshell...............................................138 5.1 Optically Thick Formation................................................... 140 5.2 Optically Thin Formation..................................................... 140 5.3 Non-Local Thermodynamical Equilibrium and Further Complications........................................................................143 6. Plasma Spectroscopy................................................................... 145 7. Closing Remarks.......................................................................... 152 References.........................................................................................153 CHAPTER 5.2 Models of Solar and Stellar Atmospheres........... 157 Petr Heinzel 1.
Introduction..................................................................................157 2. Radiative Transfer........................................................................ 158 vii
viii Contents 3. Two-Level Atom............................................................................. 3.1 Partially Coherent Scattering of Line Photons...................... 162 3.2 Two-Level Line Source Function............................................163 3.3 Solution of the Two-Level Atom Problem.............................165 3.4 Radiative Heating and Cooling................................................167 4. Classical Static Atmospheres.......................................................... 167 4.1 Basic Equations of Standard Model Atmospheres................ 168 4.2 Model Example........................................................................ 171 5. Semiempirical Models.................................................................... 172 6. Isolated Atmospheric Structures..................................................... 176 7. Spectral Line Synthesis...................................................................177 8. Radiation Hydrodynamics............................................................... 179 Acknowledgments.................................................................................. 181 References.............................................................................................. 181 CHAPTER 5.3 Spectropolarimetry and Magnetic Structures........................................................ 185 Kiyoshi Ichimoto Polarization of Light and Physical Diagnostics With Spectropolarimetry...........................................................................185 2.
Spectropolarimeter.......................................................................... 189 3. Sunspots and Active Regions......................................................... 190 4. Ubiquitous Magnetic Field in the Quiet Region Photosphere ... 193 5. Magnetic Fields in the Chromosphere........................................... 198 6. Prominences......................................................................................199 Acknowledgments................................................................................. 204 References.............................................................................................. 204 1. CHAPTER 6 Coronal Magnetism as a Universal Phenomenon....................................................... 207 B.C. Low 1. Introduction..................................................................................... 207 2. The Hydromagnetic Corona........................................................... 208 3. Coronal Phenomenology................................................................. 209 3.1 Photosphere, Chromosphere, Corona, and SolarWind.........209 3.2 Coronal Polarity Reversal: The Physical Problem................211 3.3 The Corona on February 26, 1998.........................................212 3.4 Coronal Polarity Reversal and Nature of Coronal Mass Ejections................................................................................... .. 4. The Rmy 1, ß 1 Turbulent Fluid........................................... 224 4.1 Parker Magnetostatic
Theorem............................................... 224 4.2 Magnetic Helicity Conservation and Accumulation............. 228
Contents 5. Outstanding Questions and Astrophysical Implications..............230 Acknowledgments...................................................................................232 References............................................................................................... 232 CHAPTER 7 Magnetohydrodynamics and Solar Dynamo Action................................................................239 E.R. Priest 1. Introduction..................................................................................... 240 2. Magnetohydrodynamics................................................................... 241 2.1 Validity of Magnetohydrodynamics........................................241 2.2 The Magnetohydrodynamics Equations...................................241 2.3 Induction Equation.................................................................... 243 2.4 Equation of Motion...................................................................244 2.5 Equilibria................................................................................... 245 2.6 Waves..........................................................................................246 2.7 Magnetic Reconnection............................................................ 247 3. Dynamo Theory................................................................................ 251 3.1 Introduction: Solar Observations and Terminology............. 251 3.2 A History of Dynamo Ideas.....................................................254 3.3 Early Turbulent
Dynamos.........................................................257 3.4 Flux-Transport Dynamos..........................................................259 3.5 Tachocline Dynamos................................................................ 262 3.6 Global Computations................................................................ 264 3.7 Concluding Remarks................................................................ 264 References............................................................................................... 266 CHAPTER 8 Solar and StellarVariability....................................... 267 Marianne Faurobert 1. Introduction..................................................................................... 267 2. Magnetic Activity of the Sun and Stars.........................................269 2.1 Solar Magnetic Activity........................................................... 269 2.2 Magnetic Activity of Cool Stars............................................. 272 3. Irradiance Variations........................................................................ 283 3.1 Solar Irradiance Variability......................................................284 3.2 Solar Irradiance Reconstruction.............................................. 286 3.3 Stellar Irradiance Variability................................................... 291 4. Concluding Remarks........................................................................ 294 References............................................................................................... 295 CHAPTER 9 High-
Energy Solar Physics.......................................... 301 H.S. Hudson and A.L. MacKinnon 1. Introduction.....................................................................................301 2. Nonequilibrium Plasmas.................................................................. 305 IX
x Contents 2.1 Particle Distribution Functions.............................................305 2.2 Particle Acceleration............................................................ 307 2.3 Magnetic Reconnection.........................................................307 3. Overview of Observations............................................................308 3.1 The Lower Solar Atmosphere.............................................. 309 3.2 Coronal Hard X-Ray Sources............................................... 311 3.3 Radiophysics..........................................................................311 3.4 Gamma-Ray Observations.................................................... 317 3.5 Neutral and Relativistic Particles......................................... 320 3.6 Summary................................................................................321 4. Solar and Stellar “Superflares”................................................... 322 5. Additional Topics......................................................................... 324 5.1 Coronal Mass Ejections, Solar Energetic Particles, and Flares.................................................................................... 324 5.2 Flares, Microflares, and Nanoflares......................................325 6. Conclusions...................................................................................327 References..........................................................................................328 CHAPTER 10 Space Weather at Earth and in Qur Solar
System...................................................................... 335 Noe Lugaz 1. Space Weather: A Short Historical Perspective.......................... 335 2. Solar Eruptions and Propagation................................................. 337 2.1 Coronal Observations........................................................... 337 2.2 Observations of Coronal Mass Ejection Heliospheric Propagation...........................................................................339 2.3 Numerical Simulations.......................................................... 339 2.4 Acceleration and Transport of Energetic Particles...............340 3. Impact at Earth.............................................................................340 3.1 Geomagnetic Storms and Substorms................................... 341 3.2 Magnetopause and Radiation Belts......................................344 3.3 Effects of Solar Energetic Particles......................................345 4. Impact at Other Planets and Throughout the Solar System...... 345 4.1 Mercury.................................................................................346 4.2 Venus and Mars.....................................................................347 4.3 Jupiter and Saturn................................................................. 347 4.4 Outer Heliosphere................................................................. 347 5. Star—Planet Interaction: Space Weather in Exoplanetary Systems and Conclusions............................................................. 348
Acknowledgments..............................................................................350 References..........................................................................................350
Contents CHAPTER 11 The Solar-Stellar Connection...............................363 Gibor Basri 1. Introduction...................................................................................... 363 2. Photometry and Starspots............................................................... 364 3. Activity Cycles................................................................................. 368 4. Chromospheric and Transition RegionDiagnostics.......................369 5. Coronal Diagnostics........................................................................ 371 6. Flares and Mass Loss.......................................................................373 7. Rotation—Activity—Age Relations................................................376 8. Final Thoughts.................................................................................. 382 References...............................................................................................383 INSTRUMENTATION CHAPTER 12.1 Observations of theSun FromSpace....................387 Alan Title 1. Introduction, Brief History, andCurrent Status............................. 388 2. What Are the Critical Questions for Solar and Heliospheric Physics?......................................................................390 2.1 The Beginning of Exploring the Sun From Space: 1946 Through 1964...................................................................392 3. The Early Years of Satellite Explorations of the Sun: 1964 Through 1970......................................................................... 395 4. Enhanced
Coordination on the Ground and in Space (1970 to 1980) in the Pre-Shuttle Era........................................... 396 5. 1980 to 2010: The Era of High-Resolution Imaging...................400 6. What Is the Status of the Questions of1896 and 1962?..............415 7. Coming Soon................................................................................... 416 References...............................................................................................416 CHAPTER 12.2 High-Resolution Ground-Based Observations of the Sun.............................................................. 419 Oddbjørn Engvold and Jack B. Zirker 1. Introduction......................................................................................420 2. Strategies and Conditions...............................................................421 2.1 Preferred Types of Observatory Sites..................................... 421 2.2 Optical and Technical Solutions.............................................422 2.3 Seeing Correction Techniques.................................................423 XI
XII Contents 3. Observations With Modern Solar Facilities.................................. 427 3.1 Swedish 1-Meter Solar Telescope...........................................428 3.2 Phillip R. Goode Solar Telescope...........................................430 3.3 The German Vacuum Tower Telescope and GREGOR at Teide Observatory in the Canary Islands........................... 430 3.4 New Vacuum Solar Telescope.................................................432 3.5 French THEMIS Telescope at Teide Observatory................432 3.6 Interferometric Atacama Large-Millimeter/Submillimeter Array...........................................................................................432 4. Outlook for the Future.................................................................... 433 4.1 Daniel K. Inouye Solar Telescope...........................................434 4.2 European Solar Telescope....................................................... 436 4.3 Plans for 8-Meter Telescopes.................................................. 437 4.4 Concluding Remarks................................................................ 437 5. Summary........................................................................................... 438 Acknowledgments.................................................................................. 438 References............................................................................................... 439 CHAPTER 13 Solar Dataand Simulations...............................................443 Neal Hurlburt 1.
Introduction...................................................................................... 443 2. Solar Data.......................................................................................... 444 3. Transformation and Provenance..................................................... 446 4. Search and Discovery......................................................................447 5. Data Fusion and Analysis............................................................... 449 6. Solar Simulations............................................................................. 450 7. Early Simulations............................................................................. 451 8. Shift Toward Solar Similitude........................................................453 9. Future of Data and Simulation........................................................455 References............................................................................................... 458 CHAPTER 14 1. 2. 3. 4. 5. 6. 7. 8. Challengesand Prospectsfor the Future..................... 463 Jean-Claude Vial and Andrew Skumanich Helioseismology............................................................................. 463 Solar Dynamo................................................................................. 464 Magnetic Activity and Monomials...............................................464 Data Analysis and Modeling........................................................465 Magnetic Fields and Magnetography..........................................467 Required Spatial
Resolution.........................................................467 Nanoflare Heating and Parker’s Model....................................... 468 Magnetohydrodynamic Modeling................................................ 468
Contents 9. Flares.......................................................................................... 468 10. Long-Term Activity................................................................... 469 11. Instrumentation: What Do We Need?......................................470 12. The Issue of Data Volume and Mining.................................... 470 References.......................................................................................... 472 Author Index......................................................................................................... 475 Subject Index......................................................................................................... 493 xiii
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| spelling | The sun as a guide to stellar physics edited by Oddbjørn Engvold, Jean-Claude Vial, Andrew Skumanich Amsterdam ; Oxford ; Cambridge, MA Elsevier [2019] xvii, 504 Seiten Illustrationen, Diagramme 24 cm txt rdacontent n rdamedia nc rdacarrier Astrophysik (DE-588)4003326-0 gnd rswk-swf Stern (DE-588)4057342-4 gnd rswk-swf Sonne (DE-588)1236963652 gnd rswk-swf Stars Sun Sonne (DE-588)1236963652 g Stern (DE-588)4057342-4 s Astrophysik (DE-588)4003326-0 s DE-604 Engvold, Oddbjørn 1938- (DE-588)103407282X edt Vial, Jean-Claude 1947- (DE-588)1136930795 edt Skumanich, Andrew 1929- (DE-588)1186396377 edt Digitalisierung UB Bayreuth - ADAM Catalogue Enrichment application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=030946823&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | The sun as a guide to stellar physics Astrophysik (DE-588)4003326-0 gnd Stern (DE-588)4057342-4 gnd |
| subject_GND | (DE-588)4003326-0 (DE-588)4057342-4 (DE-588)1236963652 |
| title | The sun as a guide to stellar physics |
| title_auth | The sun as a guide to stellar physics |
| title_exact_search | The sun as a guide to stellar physics |
| title_full | The sun as a guide to stellar physics edited by Oddbjørn Engvold, Jean-Claude Vial, Andrew Skumanich |
| title_fullStr | The sun as a guide to stellar physics edited by Oddbjørn Engvold, Jean-Claude Vial, Andrew Skumanich |
| title_full_unstemmed | The sun as a guide to stellar physics edited by Oddbjørn Engvold, Jean-Claude Vial, Andrew Skumanich |
| title_short | The sun as a guide to stellar physics |
| title_sort | the sun as a guide to stellar physics |
| topic | Astrophysik (DE-588)4003326-0 gnd Stern (DE-588)4057342-4 gnd |
| topic_facet | Astrophysik Stern Sonne |
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