Space Physics and Aeronomy, Volume 1, Solar Physics and Solar Wind

Name: Space Physics and Aeronomy, Volume 1, Solar Physics and Solar Wind
Brand: Capstone
Price: 174.99 EUR
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Nour E. Raouafi Angelos Vourlidas Yongliang Zhang Larry J. Paxton(Herausgeber*in)

Capstone (Verlag)

1. Auflage

Erschienen am 14. April 2021

320 Seiten

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Inhalt

Cover
Title Page
Copyright Page
Contents
List of Contributors
Preface
Chapter 1 The Solar Wind
1.1. Introduction
1.2. Observations of the Nascent Solar Wind
1.2.1. Remote-Sensing Observations of Coronal Heating and the Solar Wind
1.2.2. Transient Coronal Outflows in the Nascent Solar Wind
1.3. Measurements of the Solar Wind in the Inner Heliosphere
1.3.1. Bulk Properties and Large-Scale Structures
1.3.2. Composition of the Solar Winds
1.3.3. Solar Wind Interaction Regions
1.3.4. Mesoscale Structures
1.3.5. Magnetic Reconnection in the Solar Wind
1.4. Waves and Turbulence
1.4.1. Spectra of Solar Wind Fluctuations at All Scales
1.4.2. Alfvén Waves in the Fast and Slow Winds
1.4.3. Solar Wind Fluctuations at Kinetic Scales
1.5. Kinetic Processes and Heating in the Solar Wind
1.5.1. Evolution of Anisotropies of the Solar Wind Distribution Function
1.5.2. Wave-Particle Interactions, Kinetic Instabilities, and Collisions
1.5.3. Suprathermal Particles
1.6. The Evolution of the Solar Wind from the Inner to Outer Heliosphere
1.7. Outstanding Questions and Future Prospects
Acknowledgments
References
Chapter 2 The Heating of the Solar Corona
2.1. Historical Viewpoint on the Coronal Heating Problem
2.2. Observational Constraints on Chromospheric and Coronal Heating
2.2.1. Observations of Chromospheric Heating
2.2.2. Observations of Coronal Heating
2.3. Modeling of the Solar Atmosphere
2.3.1. Approach One: Local MHD Models
2.3.2. Approach Two: Field-Aligned Hydrodynamic Modeling
2.3.3. Approach Three: Global Models of the Solar Atmosphere
2.4. Future Prospects for Modeling and Observations
Acknowledgments
References
Chapter 3 Solar Magnetism and Radiation
3.1. Introduction
3.2. The Solar Magnetic Field
3.2.1. Measurement of Solar Magnetic Field
3.2.2. Cyclical Behavior of the Global Solar Field
3.2.3. Magnetic Helicity
3.3. Solar Magnetic Features with Radiative Signatures
3.3.1. Features of the Photosphere in Visible Light
3.3.2. Chromospheric Filaments
3.3.3. Coronal Loops
3.3.4. Coronal Holes and Solar Wind Structure
3.3.5. Flares and CMEs
3.4. The Sun as a Star: Solar Irradiance Variability
3.4.1. Irradiance Variability and Surface Magnetism
3.4.2. Models for Solar Irradiance
3.4.3. Uncertainties in Irradiance Reconstructions
3.4.4. Other Physical Mechanisms for Solar Irradiance Variability
3.4.5. Effects of Solar and Stellar Irradiance on Planet and Exoplanet Atmospheres
3.5. Calcium II K Observations
3.5.1. Calcium II K Spectroheliograms
3.5.2. Mount Wilson Calcium II K Spectroheliograms
3.5.3. Kodaikanal Calcium II K Spectroheliograms
3.5.4. The Meudon Archive
3.5.5. The Arcetri Archive
3.5.6. The Coimbra Archive
3.5.7. Other Ca K Line Image Archives
3.5.8. Calcium II K Sun-as-a-Star Measurements
Acknowledgments
Note
References
Chapter 4 Solar Energetic Particles
4.1. Introduction
4.2. History
4.3. Solar Energetic Ion Variability in Shock-Accelerated Sep Events
4.3.1. Temporal Variations
4.3.2. Spectral Variations
4.3.3. Compositional Variations
4.3.4. Spatial Variability
4.4. 3He-Rich Sep Events
4.4.1. Source and Injection Properties
4.4.2. Properties of 3He-Rich SEP Event-Averaged Electron and Ion Spectra
4.4.3. Theoretical Models for 3He-Rich Events
4.5. Sep Electrons
4.5.1. Occurrence Frequency of Solar Energetic Electron Events
4.5.2. Association with Other Solar Phenomena
4.5.3. Solar Electron Injections
4.5.4. Electron Energy Spectra
4.5.5. Electron Pitch Angle Distributions
4.6. Understanding SEPs Via Energetic Neutral Atoms (ENAs)
4.6.1. Observation of Solar ENAs
4.6.2. Solar ENA Predictions
4.6.3. Future Solar ENA Observations
4.7. Theory of Sep Acceleration and Transport
4.7.1. Particle Acceleration Associated with Magnetic Reconnection
4.7.2. Stochastic Acceleration (SA)
4.7.3. Diffusive Shock Acceleration (DSA)
4.7.4. Propagation of Energetic Particles in the Solar Wind
4.8. Concluding Remarks
Acknowledgments
References
Chapter 5 Solar Flares and Coronal Mass Ejections
5.1. Introduction
5.2. History
5.2.1. Early History
5.2.2. The "Carrington Event"
5.2.3. Improved Observations Lead to the Modern Era
5.3. Observational Signatures and Detection Properties
5.3.1. Flares
5.3.2. Coronal Mass Ejections
5.4. Theoretical Interpretations and Key Problems
5.4.1. Magnetic Reconnection
5.4.2. Global Configuration and Topology
5.4.3. Energy Deposition in Flares
5.4.4. CME Mass and Energetics
5.5. Space Weather and Beyond
5.5.1. Space Weather
5.5.2. Exoplanet Impacts
5.5.3. Enabling Predictions Using Machine Learning
Acknowledgments
References
Chapter 6 Fine-Scale Features of the Sun's Atmosphere: Spicules and Jets
6.1. Introduction
6.2. Solar Spicules
6.2.1. Earlier Spicule Observations
6.2.2. Earlier Spicule Models
6.2.3. More Recent Spicule Observations
6.2.4. More Recent Spicule Models
6.3. Coronal Jets
6.3.1. Earlier Jet Studies: Observations
6.3.2. Earlier Jet Studies: Theories
6.3.3. Later Jet Studies: Observations
6.3.4. Later Jet Studies: Theories
the Cause of Jets Revisited
6.3.5. The Magnetic Cause of Jets
6.3.6. AR Jets
6.3.7. Jet Numerical Models: Recent Progress
6.4. Jet-Like Phenomena on Differing Size Scales
6.4.1. Coronal Jets and Large-Scale Eruptions
6.4.2. Smaller-Scale Jets: Jetlets and Spicules(?)
6.5. Coronal Jets and Other Phenomena
6.5.1. Jets and Plumes
6.5.2. Jets and Macrospicules
6.5.3. Jets and Coronal Heating
6.6. The Future
Acknowledgments
Note
References
Chapter 7 Solar Interior
7.1 Solar Dynamo
7.1.1 Solar Dynamo Models: Overall Context
7.1.2 Small-Scale Turbulent Dynamos and Their Observational Signatures
7.1.3 Global Dynamo Models and Solar Cycle
7.1.4 Solar Cycle Observations to Be Modeled by a Cyclic Dynamo
7.1.5 Recent Models and Results
7.1.6 Outstanding Challenges to Be Explored
7.2 Helioseismology
7.2.1 Basic Principles
7.2.2 Observations
7.2.3 Inversions
7.2.4 Solar Cycle Variations
7.2.5 Rotation
7.2.6 Meridional Flow
7.3 Flux Emergence
7.3.1 Observations of Emerging Flux
7.3.2 Theory and Modeling of Flux Emergence
Acknowledgments
References
Index
EULA

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