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- catalog contributor b13083479.
- catalog coverage "Sun Research.".
- catalog coverage "Sun.".
- catalog created "c2004.".
- catalog date "2004".
- catalog date "c2004.".
- catalog dateCopyrighted "c2004.".
- catalog description "1 Development of the Ideas and Instruments of Modern Solar Research 1 -- 1.1 Early Telescopic Discoveries on the Sun 1 -- 1.2 The Spectroscope and Photography 5 -- 1.3 Solar-Terrestial Research and the New Astronomy 8 -- 1.4 Solar Chemical Composition and Energy Generation 14 -- 1.5 The Mt. Wilson Era of Large Telescopes 17 -- 1.6 Advances in Coronal Physics and in the Theory of Solar Activity 22 -- 1.7 Observations at Radio, Ultraviolet, and X-Ray Wavelengths 26 -- 1.8 The Solar Wind and Heliosphere 28 -- 1.9 Future Directions in Solar Instrumentation 30 -- 2 Radiative Transfer in the Sun's Atmosphere 36 -- 2.1 Photometric Principles 36 -- 2.1.1 The Radiative Intensity 36 -- 2.1.2 The Net Outward Flux and the Solar Constant 38 -- 2.2 The Radiative Transfer Equation 41 -- 2.2.1 The Optical Depth and Source Function 41 -- 2.2.2 Solution for Constant Source Function 43 -- 2.2.3".
- catalog description "179 -- 6.4 The Standard Model of Physical Conditions in the Solar Interior 180 -- 6.5 Observational Tests of the Standard Model 183 -- 6.5.1 Solar Neutrino Observations 183 -- 6.5.2 Lithium and Beryllium Abundances 186 -- 6.5.3 Stellar Structure and Evolution 187 -- 6.5.4 Geological and Climatological Evidence 189 -- 6.5.5 The Sun's Angular Momentum and Shape 190 -- 6.5.6 Solar Oscillations 191 -- 7 Rotation, Convection, and Oscillations in the Sun 195 -- 7.1 Observations of Solar Rotation 196 -- 7.1.1 Photospheric Doppler Measurements 196 -- 7.1.2 Helioseismic Measurements of Rotation in the Solar Interior 198 -- 7.1.3 Tracer Measurements 199 -- 7.2 Measurements on Convection 201 -- 7.2.1 Observations of Convection at the Photosphere 201 -- 7.2.2 Comparison with Laboratory Measurements 202 -- 7.3 Dynamics of Solar Convection and Rotation 203 -- 7.3.1".
- catalog description "A Survey of the Sun's Spectrum 65 -- 3.2 Atomic Structure 74 -- 3.3 Space Quantization and the Zeeman and Stark Effects 78 -- 3.3.1 The Zeeman Effect 79 -- 3.3.2 The Stark Effect 84 -- 3.4 Multiplet Rules for Transitions 86 -- 3.5 Atomic Transitions and their Excitation 88 -- 3.6 Rates for Radiative Transitions 90 -- 3.7 Boltzmann Equilibrium and the Saha Equation 91 -- 3.8 Rate Equations in Statistical Equilibrium 93 -- 3.9 Line Broadening 95 -- 3.9.1 Thermal and Turbulent Doppler Broadening 95 -- 3.9.2 Radiation Damping and Pressure Broadening 97 -- 3.9.3 Broadening by Self-Absorption 98 -- 3.9.4 Analysis of the Observed Profile of a Spectral Line 98 -- 3.10 Molecules on the Sun 100 -- 4 Dynamics of Solar Plasmas 103 -- 4.1 Hydrostatic Equilibrium 104 -- 4.1.1 Equilibrium in a Homogeneous Gravitational Field 104 -- 4.1.2 Self-Gravitating Atmospheres 105 -- 4.1.3".
- catalog description "Birth and Evolution of Spot Groups 240 -- 8.1.3 Photometry and Spectra of Umbrae 241 -- 8.1.4 Mass Motions and Oscillations 244 -- 8.2 Dynamics of Spots 247 -- 8.2.1 Thermal Structure of the Umbra 247 -- 8.2.2 Why Spots Are Cool 249 -- 8.2.3 Why Spots Cause Dips in the Solar Luminosity 251 -- 8.2.4 Dynamics of Sunspot Evolution 252 -- 8.3 Faculae 254 -- 8.3.1 Structure and Evolution 254 -- 8.3.2 Physical Measurements 254 -- 8.3.3 Why Faculae Are Bright 259 -- 8.4 Observations of Solar Magnetism 261 -- 8.4.1 The Sunspot Magnetic Field 261 -- 8.4.2 Photospheric Fields in Faculae and Magnetic Network 263 -- 8.4.3 Large-Scale Structure and Evolution of the Photospheric Field 266 -- 8.4.4 Global Structure of the Sun's Magnetic Field 272 -- 9 The Chromosphere and Corona 277 -- 9.1 The Chromosphere 278 -- 9.1.1 Observations of Structures and Motions at the Limb 278 -- 9.1.2".
- catalog description "Condition for Onset of Convection 203 -- 7.3.2 Gravity Waves 205 -- 7.3.3 Mixing Length Theory 206 -- 7.3.4 Dynamics of Convection in a Plane Layer 208 -- 7.3.5 Models of Granulation 209 -- 7.3.6 Dynamics of Supergranulation 212 -- 7.3.7 Dynamics of the Solar Interior 212 -- 7.4 Observations of Solar Oscillations 215 -- 7.4.1 The 5-min Oscillations 215 -- 7.4.2 Oscillations of Longer and Shorter Periods 219 -- 7.5 Interpretation of Solar Oscillations 220 -- 7.5.1 Resonances in the Sun 220 -- 7.5.2 Oscillation Modes of the Solar Interior 223 -- 7.5.3 Excitation and Damping Mechanisms 225 -- 7.5.4 Comparison of the Observed and Calculated Properties of the p-Modes 226 -- 7.5.5 Oscillations as a Probe of the Solar Interior 228 -- 8 Observations of Photospheric Activity and Magnetism 233 -- 8.1 Sunspot Observations 234 -- 8.1.1 Structure of the Umbra and Penumbra 234 -- 8.1.2".
- catalog description "Dynamics of Solar Magnetic Flux Tubes 351 -- 11.1.1 Dynamical Equilibrium and Geometry 351 -- 11.1.2 Dynamical Stability 355 -- 11.1.3 Thermal Instability 357 -- 11.1.4 Steady Flows 358 -- 11.1.5 Oscillations and Waves 360 -- 11.1.6 Magnetic Field Dissipation 363 -- 11.2 Activity Behavior over the Solar Cycle 365 -- 11.2.1 The Sunspot Number and Other Activity Indices 365 -- 11.2.2 Time Behavior of the Sun's Magnetic Field 367 -- 11.1.3 Long-Term Behavior of Solar Activity 371 -- 11.3 Dynamics of the Solar Magnetic Cycle 376 -- 11.3.1 The Babcock Model of the Solar Cycle 376 -- 11.3.2 Dynamical Dynamo Models 379 -- 12 The Solar Wind and Heliosphere 387.".
- catalog description "Includes bibliographical references and index.".
- catalog description "Observations on the Disk 281 -- 9.1.3 Physical Conditions 288 -- 9.1.4 Energy Balance 293 -- 9.1.5 Chromospheric Heating 293 -- 9.1.6 Dynamics of Spicules and Fibrils 295 -- 9.2 The Corona and Transition Region 297 -- 9.2.1 Spectrum and Radiation Mechanisms 297 -- 9.2.2 Structures of the Corona and Transition Region 298 -- 9.2.3 Magnetic Fields and Plasma Motions 303 -- 9.2.4 Physical Conditions in Closed and Open Magnetic Structures 306 -- 9.2.5 Heating and Dynamics of Coronal Loops and Holes 311 -- 10 Prominences and Flares 319 -- 10.1 Prominences and Filaments 320 -- 10.1.1 Observations and Physical Conditions 320 -- 10.1.2 Dynamics 324 -- 10.2 Flares 331 -- 10.2.1 Observations and Physical Conditions 331 -- 10.2.2 Energy Release and Dynamics 344 -- 10.2.3 Acceleration of Energetic Charged Particles 348 -- 11 Dynamics of the Solar Magnetic Field 351 -- 11.1".
- catalog description "Solution for a Linear Source Function: The Eddington-Barbier Relation 44 -- 2.3 Thermodynamic Equilibrium 47 -- 2.3.1 The Planck Function 47 -- 2.3.2 Kirchhoff's Law 48 -- 2.3.3 Local Thermodynamic Equilibrium (LTE) 49 -- 2.3.4 The Brightness- and Effective Temperatures 50 -- 2.4 The Gray Atmosphere 50 -- 2.4.1 Formulation of the Problem 50 -- 2.4.2 Gray Limb Darkening in the Eddington Approximation 52 -- 2.4.3 The Photospheric Level Identified with Radiation at T[subscript eff] 53 -- 2.4.4 Radiative Diffusion 54 -- 2.5 Radiative Transfer in the Fraumhofer Lines 55 -- 2.5.1 Formation of Fraunhofer Lines 55 -- 2.5.2 The Transfer Equation for Lines 56 -- 2.5.3 The Milne-Eddington Model 57 -- 2.5.4 Comparison with Observations of Line Depth near Disk Center 58 -- 2.5.5 Comparison with Observed Center-to-Limb Behavior 60 -- 3 Solar Spectroscopy 65 -- 3.1".
- catalog description "The Photospheric Chemical Composition and the Curve of Growth 156 -- 5.5.1 The Theoretical Curve of Growth 157 -- 5.5.2 Comparison with the Empirical Curve 160 -- 5.6 The Sun's Chemical Composition 162 -- 6 The Sun's Internal Structure and Energy Generation 167 -- 6.1 Equations of Stellar Structure 168 -- 6.1.1 Mechanical Equilibrium 168 -- 6.1.2 Energy Transport 169 -- 6.1.3 Boundary Conditions 170 -- 6.2 Physical Parameters Required for the Solution 171 -- 6.2.1 Chemical Composition 171 -- 6.2.2 The Mean Molecular Weight 172 -- 6.2.3 The Ratio of Specific Heats 172 -- 6.2.4 The Radiative Opacity 173 -- 6.2.5 Energy Generation Processes 174 -- 6.3 Nuclear Reactions in the Sun's Interior 174 -- 6.3.1 Factors That Determine the Dominant Reactions 174 -- 6.3.2 The Proton-Proton Chain 175 -- 6.3.3 The Carbon-Nitrogen Cycle 177 -- 6.3.4 Nuclear Energy Generation Rates".
- catalog description "The Polytropic Approximation 105 -- 4.2 The Equations of Motion 107 -- 4.2.1 Euler's Equation 107 -- 4.2.2 Viscous Forces and the Navier-Stokes Equation 108 -- 4.2.3 The Equation of Continuity 110 -- 4.2.4 The Heat-Balance Equation 111 -- 4.2.5 Conservation of Total Energy 114 -- 4.3 The Influence of Magnetic Fields in Solar Plasma Dynamics 115 -- 4.3.1 The Lorentz Force 115 -- 4.3.2 The Importance of Self-induction 116 -- 4.3.3 The Diffusive and "Frozen-in" Approximations 117 -- 4.4 Wave Motions in the Sun 119 -- 4.4.1 Types of Waves Expected and Observed 119 -- 4.4.2 Sound Waves 119 -- 4.4.3 Simple Waves and Shock Formation 120 -- 4.4.4 Properties of Shock Waves 121 -- 4.4.5 Magnetohydrodynamic Waves 123 -- 4.4.6 Internal Gravity Waves 125 -- 4.4.7 Plasma Oscillations 125 -- 4.5 Charged Particle Dynamics 126 -- 4.5.1".
- catalog description "Validity of the Continuum Approximation and of Thermal Equilibrium 126 -- 4.5.2 Charged Particle Motions 127 -- 5 The Photosphere 133 -- 5.1 Observations of the Quiet Photosphere 135 -- 5.1.1 Limb Darkening 135 -- 5.1.2 Observed Properties of Granulation 138 -- 5.1.3 The Supergranulation and Photospheric Network 143 -- 5.2 Construction of a Photospheric Model 146 -- 5.2.1 Physical Assumptions 146 -- 5.2.2 Determination of the Temperature Profile from Continuum Limb Darkening 147 -- 5.3 Determination of the Photospheric Opacity 148 -- 5.3.1 The Empirical Technique 148 -- 5.3.2 The Sources of Photospheric Opacity 149 -- 5.4 Physical Structure and Energy Balance of the Photosphere 150 -- 5.4.1 Models of Photospheric Structure 150 -- 5.4.2 Comparison with Observations 153 -- 5.4.3 Energy Transport Mechanisms in the Photosphere 155 -- 5.5".
- catalog extent "xiv, 466 p. :".
- catalog identifier "3527403744 (hd. bd.)".
- catalog issued "2004".
- catalog issued "c2004.".
- catalog language "eng".
- catalog publisher "Weinheim : Wiley-VCH,".
- catalog spatial "Sun Research.".
- catalog spatial "Sun.".
- catalog subject "Astrophysics.".
- catalog subject "QB521 .F68 2004".
- catalog tableOfContents "1 Development of the Ideas and Instruments of Modern Solar Research 1 -- 1.1 Early Telescopic Discoveries on the Sun 1 -- 1.2 The Spectroscope and Photography 5 -- 1.3 Solar-Terrestial Research and the New Astronomy 8 -- 1.4 Solar Chemical Composition and Energy Generation 14 -- 1.5 The Mt. Wilson Era of Large Telescopes 17 -- 1.6 Advances in Coronal Physics and in the Theory of Solar Activity 22 -- 1.7 Observations at Radio, Ultraviolet, and X-Ray Wavelengths 26 -- 1.8 The Solar Wind and Heliosphere 28 -- 1.9 Future Directions in Solar Instrumentation 30 -- 2 Radiative Transfer in the Sun's Atmosphere 36 -- 2.1 Photometric Principles 36 -- 2.1.1 The Radiative Intensity 36 -- 2.1.2 The Net Outward Flux and the Solar Constant 38 -- 2.2 The Radiative Transfer Equation 41 -- 2.2.1 The Optical Depth and Source Function 41 -- 2.2.2 Solution for Constant Source Function 43 -- 2.2.3".
- catalog tableOfContents "179 -- 6.4 The Standard Model of Physical Conditions in the Solar Interior 180 -- 6.5 Observational Tests of the Standard Model 183 -- 6.5.1 Solar Neutrino Observations 183 -- 6.5.2 Lithium and Beryllium Abundances 186 -- 6.5.3 Stellar Structure and Evolution 187 -- 6.5.4 Geological and Climatological Evidence 189 -- 6.5.5 The Sun's Angular Momentum and Shape 190 -- 6.5.6 Solar Oscillations 191 -- 7 Rotation, Convection, and Oscillations in the Sun 195 -- 7.1 Observations of Solar Rotation 196 -- 7.1.1 Photospheric Doppler Measurements 196 -- 7.1.2 Helioseismic Measurements of Rotation in the Solar Interior 198 -- 7.1.3 Tracer Measurements 199 -- 7.2 Measurements on Convection 201 -- 7.2.1 Observations of Convection at the Photosphere 201 -- 7.2.2 Comparison with Laboratory Measurements 202 -- 7.3 Dynamics of Solar Convection and Rotation 203 -- 7.3.1".
- catalog tableOfContents "A Survey of the Sun's Spectrum 65 -- 3.2 Atomic Structure 74 -- 3.3 Space Quantization and the Zeeman and Stark Effects 78 -- 3.3.1 The Zeeman Effect 79 -- 3.3.2 The Stark Effect 84 -- 3.4 Multiplet Rules for Transitions 86 -- 3.5 Atomic Transitions and their Excitation 88 -- 3.6 Rates for Radiative Transitions 90 -- 3.7 Boltzmann Equilibrium and the Saha Equation 91 -- 3.8 Rate Equations in Statistical Equilibrium 93 -- 3.9 Line Broadening 95 -- 3.9.1 Thermal and Turbulent Doppler Broadening 95 -- 3.9.2 Radiation Damping and Pressure Broadening 97 -- 3.9.3 Broadening by Self-Absorption 98 -- 3.9.4 Analysis of the Observed Profile of a Spectral Line 98 -- 3.10 Molecules on the Sun 100 -- 4 Dynamics of Solar Plasmas 103 -- 4.1 Hydrostatic Equilibrium 104 -- 4.1.1 Equilibrium in a Homogeneous Gravitational Field 104 -- 4.1.2 Self-Gravitating Atmospheres 105 -- 4.1.3".
- catalog tableOfContents "Birth and Evolution of Spot Groups 240 -- 8.1.3 Photometry and Spectra of Umbrae 241 -- 8.1.4 Mass Motions and Oscillations 244 -- 8.2 Dynamics of Spots 247 -- 8.2.1 Thermal Structure of the Umbra 247 -- 8.2.2 Why Spots Are Cool 249 -- 8.2.3 Why Spots Cause Dips in the Solar Luminosity 251 -- 8.2.4 Dynamics of Sunspot Evolution 252 -- 8.3 Faculae 254 -- 8.3.1 Structure and Evolution 254 -- 8.3.2 Physical Measurements 254 -- 8.3.3 Why Faculae Are Bright 259 -- 8.4 Observations of Solar Magnetism 261 -- 8.4.1 The Sunspot Magnetic Field 261 -- 8.4.2 Photospheric Fields in Faculae and Magnetic Network 263 -- 8.4.3 Large-Scale Structure and Evolution of the Photospheric Field 266 -- 8.4.4 Global Structure of the Sun's Magnetic Field 272 -- 9 The Chromosphere and Corona 277 -- 9.1 The Chromosphere 278 -- 9.1.1 Observations of Structures and Motions at the Limb 278 -- 9.1.2".
- catalog tableOfContents "Condition for Onset of Convection 203 -- 7.3.2 Gravity Waves 205 -- 7.3.3 Mixing Length Theory 206 -- 7.3.4 Dynamics of Convection in a Plane Layer 208 -- 7.3.5 Models of Granulation 209 -- 7.3.6 Dynamics of Supergranulation 212 -- 7.3.7 Dynamics of the Solar Interior 212 -- 7.4 Observations of Solar Oscillations 215 -- 7.4.1 The 5-min Oscillations 215 -- 7.4.2 Oscillations of Longer and Shorter Periods 219 -- 7.5 Interpretation of Solar Oscillations 220 -- 7.5.1 Resonances in the Sun 220 -- 7.5.2 Oscillation Modes of the Solar Interior 223 -- 7.5.3 Excitation and Damping Mechanisms 225 -- 7.5.4 Comparison of the Observed and Calculated Properties of the p-Modes 226 -- 7.5.5 Oscillations as a Probe of the Solar Interior 228 -- 8 Observations of Photospheric Activity and Magnetism 233 -- 8.1 Sunspot Observations 234 -- 8.1.1 Structure of the Umbra and Penumbra 234 -- 8.1.2".
- catalog tableOfContents "Dynamics of Solar Magnetic Flux Tubes 351 -- 11.1.1 Dynamical Equilibrium and Geometry 351 -- 11.1.2 Dynamical Stability 355 -- 11.1.3 Thermal Instability 357 -- 11.1.4 Steady Flows 358 -- 11.1.5 Oscillations and Waves 360 -- 11.1.6 Magnetic Field Dissipation 363 -- 11.2 Activity Behavior over the Solar Cycle 365 -- 11.2.1 The Sunspot Number and Other Activity Indices 365 -- 11.2.2 Time Behavior of the Sun's Magnetic Field 367 -- 11.1.3 Long-Term Behavior of Solar Activity 371 -- 11.3 Dynamics of the Solar Magnetic Cycle 376 -- 11.3.1 The Babcock Model of the Solar Cycle 376 -- 11.3.2 Dynamical Dynamo Models 379 -- 12 The Solar Wind and Heliosphere 387.".
- catalog tableOfContents "Observations on the Disk 281 -- 9.1.3 Physical Conditions 288 -- 9.1.4 Energy Balance 293 -- 9.1.5 Chromospheric Heating 293 -- 9.1.6 Dynamics of Spicules and Fibrils 295 -- 9.2 The Corona and Transition Region 297 -- 9.2.1 Spectrum and Radiation Mechanisms 297 -- 9.2.2 Structures of the Corona and Transition Region 298 -- 9.2.3 Magnetic Fields and Plasma Motions 303 -- 9.2.4 Physical Conditions in Closed and Open Magnetic Structures 306 -- 9.2.5 Heating and Dynamics of Coronal Loops and Holes 311 -- 10 Prominences and Flares 319 -- 10.1 Prominences and Filaments 320 -- 10.1.1 Observations and Physical Conditions 320 -- 10.1.2 Dynamics 324 -- 10.2 Flares 331 -- 10.2.1 Observations and Physical Conditions 331 -- 10.2.2 Energy Release and Dynamics 344 -- 10.2.3 Acceleration of Energetic Charged Particles 348 -- 11 Dynamics of the Solar Magnetic Field 351 -- 11.1".
- catalog tableOfContents "Solution for a Linear Source Function: The Eddington-Barbier Relation 44 -- 2.3 Thermodynamic Equilibrium 47 -- 2.3.1 The Planck Function 47 -- 2.3.2 Kirchhoff's Law 48 -- 2.3.3 Local Thermodynamic Equilibrium (LTE) 49 -- 2.3.4 The Brightness- and Effective Temperatures 50 -- 2.4 The Gray Atmosphere 50 -- 2.4.1 Formulation of the Problem 50 -- 2.4.2 Gray Limb Darkening in the Eddington Approximation 52 -- 2.4.3 The Photospheric Level Identified with Radiation at T[subscript eff] 53 -- 2.4.4 Radiative Diffusion 54 -- 2.5 Radiative Transfer in the Fraumhofer Lines 55 -- 2.5.1 Formation of Fraunhofer Lines 55 -- 2.5.2 The Transfer Equation for Lines 56 -- 2.5.3 The Milne-Eddington Model 57 -- 2.5.4 Comparison with Observations of Line Depth near Disk Center 58 -- 2.5.5 Comparison with Observed Center-to-Limb Behavior 60 -- 3 Solar Spectroscopy 65 -- 3.1".
- catalog tableOfContents "The Photospheric Chemical Composition and the Curve of Growth 156 -- 5.5.1 The Theoretical Curve of Growth 157 -- 5.5.2 Comparison with the Empirical Curve 160 -- 5.6 The Sun's Chemical Composition 162 -- 6 The Sun's Internal Structure and Energy Generation 167 -- 6.1 Equations of Stellar Structure 168 -- 6.1.1 Mechanical Equilibrium 168 -- 6.1.2 Energy Transport 169 -- 6.1.3 Boundary Conditions 170 -- 6.2 Physical Parameters Required for the Solution 171 -- 6.2.1 Chemical Composition 171 -- 6.2.2 The Mean Molecular Weight 172 -- 6.2.3 The Ratio of Specific Heats 172 -- 6.2.4 The Radiative Opacity 173 -- 6.2.5 Energy Generation Processes 174 -- 6.3 Nuclear Reactions in the Sun's Interior 174 -- 6.3.1 Factors That Determine the Dominant Reactions 174 -- 6.3.2 The Proton-Proton Chain 175 -- 6.3.3 The Carbon-Nitrogen Cycle 177 -- 6.3.4 Nuclear Energy Generation Rates".
- catalog tableOfContents "The Polytropic Approximation 105 -- 4.2 The Equations of Motion 107 -- 4.2.1 Euler's Equation 107 -- 4.2.2 Viscous Forces and the Navier-Stokes Equation 108 -- 4.2.3 The Equation of Continuity 110 -- 4.2.4 The Heat-Balance Equation 111 -- 4.2.5 Conservation of Total Energy 114 -- 4.3 The Influence of Magnetic Fields in Solar Plasma Dynamics 115 -- 4.3.1 The Lorentz Force 115 -- 4.3.2 The Importance of Self-induction 116 -- 4.3.3 The Diffusive and "Frozen-in" Approximations 117 -- 4.4 Wave Motions in the Sun 119 -- 4.4.1 Types of Waves Expected and Observed 119 -- 4.4.2 Sound Waves 119 -- 4.4.3 Simple Waves and Shock Formation 120 -- 4.4.4 Properties of Shock Waves 121 -- 4.4.5 Magnetohydrodynamic Waves 123 -- 4.4.6 Internal Gravity Waves 125 -- 4.4.7 Plasma Oscillations 125 -- 4.5 Charged Particle Dynamics 126 -- 4.5.1".
- catalog tableOfContents "Validity of the Continuum Approximation and of Thermal Equilibrium 126 -- 4.5.2 Charged Particle Motions 127 -- 5 The Photosphere 133 -- 5.1 Observations of the Quiet Photosphere 135 -- 5.1.1 Limb Darkening 135 -- 5.1.2 Observed Properties of Granulation 138 -- 5.1.3 The Supergranulation and Photospheric Network 143 -- 5.2 Construction of a Photospheric Model 146 -- 5.2.1 Physical Assumptions 146 -- 5.2.2 Determination of the Temperature Profile from Continuum Limb Darkening 147 -- 5.3 Determination of the Photospheric Opacity 148 -- 5.3.1 The Empirical Technique 148 -- 5.3.2 The Sources of Photospheric Opacity 149 -- 5.4 Physical Structure and Energy Balance of the Photosphere 150 -- 5.4.1 Models of Photospheric Structure 150 -- 5.4.2 Comparison with Observations 153 -- 5.4.3 Energy Transport Mechanisms in the Photosphere 155 -- 5.5".
- catalog title "Solar astrophysics / Peter V. Foukal.".
- catalog type "text".