Beschreibung
InhaltsangabeForeword.- Dedication to George Gloeckler.- Section I: What are the Three-Dimensional Shape and Structure of the Dynamic Heliosphere?.- The Solar Wind in the Outer Heliosphere.- Constraints on the Structure of the Heliosphere Interface Based on Lyman-Alpha Absorption Spectra.- Influence of the Interstellar Magnetic Field and Neutrals on the Shape of the Outer Heliosphere.- Role of the Interstellar Magnetic Field in Voyager 1 and 2 Asymmetries.- The Dynamic Heliosphere Splinter Group.- Section II: What are the Dominant Physical Processes in the Termination Shock and Inner Heliosheath?.- The Heliospheric Magnetic Field and its Extension to the Inner Heliosheath.- Pickup Ion Acceleration and Evolution in the Heliosheath and Termination Shock.- Energetic Neutral Atom (ENA) Imaging of the Inner Heliosheath.- Section III: How are the ISM Inside and Outside of the Heliosphere Related?.- Inferences of the Local Interstellar Parameters from Observations Inside the Heliosphere.- Backscattered Lyman-Alpha Observations From SOHO/SWAN and Voyagers.- Composition of Interstellar Neutrals in the Inner Heliosheath at 100 AU.- Neutral H Density at the Termination Shock.- How are the ISM Inside and Outside of the Heliosphere Related.- Section IV: What are the Energy and Pressure Balances in the Local Bubble?.- Pressure, Ionization, and Energy Balance in the Local Bubble.- Charge Transfer in the Inner Heliosphere and Local Bubble.- Revising the Local Bubble Model Due to Solar Wind Charge Exchange X-Ray Emission.- Warm and Hot Gas in the Local ISM.- What Can be Learned from X-Ray Spectroscopy Concerning Hot Gas in the Local Bubble and Charge Exchange Processes?.- Section V: What Physical Processes Drive the Multiphase Interstellar Medium in the Local Bubble?.- What Physical Processes Drive the Interstellar Medium in the Local Bubble: Introduction.- Turbulence in the Local ISM and Local Bubble.- Exotic Clouds in the Local Interstellar Medium.- The Local Bubble Debate.- Section VI: What are the Origin and Physical Properties of the Clump of Very Local ISM?.- The Origins and Physical Properties of the Complex of Local Interstellar Clouds.- Physical Properties of the Local ISM.- Perspectives on Interstellar Dust Inside and Outside of the Heliosphere.- Dust Inside and Outside of the Heliosphere.- Section VII: What are the Roles that Magnetic Fields Play in the Local Bubble and Its Constituents?.- Obtaining Spectra of Turbulent Velocity from Observations.- Properties and Selected Implications of Magnetic Turbulence for Interstellar Medium, Local Bubble, and Solar Wind.- Section VIII: The Emerging Broad Picture.- The Heliosphere in Time.- Origin and Evolution of the Local Bubble and Local ISM.- Origin of the Local Bubble.- Kinetic Fluid Perspective in Modeling in the Heliosphere-Interstellar Medium Interface.- Section IX: Summary.- What Have We Learned?.
Inhaltsverzeichnis
Foreword.- Dedication to George Gloeckler.- Section I: What are the Three-Dimensional Shape and Structure of the Dynamic Heliosphere?.- The Solar Wind in the Outer Heliosphere.- Constraints on the Structure of the Heliosphere Interface Based on Lyman-Alpha Absorption Spectra.- Influence of the Interstellar Magnetic Field and Neutrals on the Shape of the Outer Heliosphere.- Role of the Interstellar Magnetic Field in Voyager 1 and 2 Asymmetries.- The Dynamic Heliosphere Splinter Group.- Section II: What are the Dominant Physical Processes in the Termination Shock and Inner Heliosheath?.- The Heliospheric Magnetic Field and its Extension to the Inner Heliosheath.- Pickup Ion Acceleration and Evolution in the Heliosheath and Termination Shock.- Energetic Neutral Atom (ENA) Imaging of the Inner Heliosheath.- Section III: How are the ISM Inside and Outside of the Heliosphere Related?.- Inferences of the Local Interstellar Parameters from Observations Inside the Heliosphere.- Backscattered Lyman-Alpha Observations From SOHO/SWAN and Voyagers.- Composition of Interstellar Neutrals in the Inner Heliosheath at 100 AU.- Neutral H Density at the Termination Shock.- How are the ISM Inside and Outside of the Heliosphere Related.- Section IV: What are the Energy and Pressure Balances in the Local Bubble?.- Pressure, Ionization, and Energy Balance in the Local Bubble.- Charge Transfer in the Inner Heliosphere and Local Bubble.- Revising the Local Bubble Model Due to Solar Wind Charge Exchange X-Ray Emission.- Warm and Hot Gas in the Local ISM.- What Can be Learned from X-Ray Spectroscopy Concerning Hot Gas in the Local Bubble and Charge Exchange Processes?.- Section V: What Physical Processes Drive the Multiphase Interstellar Medium in the Local Bubble?.- What Physical Processes Drive the Interstellar Medium in the Local Bubble: Introduction.- Turbulence in the Local ISM and Local Bubble.- Exotic Clouds in the Local Interstellar Medium.- The Local Bubble Debate.- Section VI: What are the Origin and Physical Properties of the Clump of Very Local ISM?.- The Origins and Physical Properties of the Complex of Local Interstellar Clouds.- Physical Properties of the Local ISM.- Perspectives on Interstellar Dust Inside and Outside of the Heliosphere.- Dust Inside and Outside of the Heliosphere.- Section VII: What are the Roles that Magnetic Fields Play in the Local Bubble and Its Constituents?.- Obtaining Spectra of Turbulent Velocity from Observations.- Properties and Selected Implications of Magnetic Turbulence for Interstellar Medium, Local Bubble, and Solar Wind.- Section VIII: The Emerging Broad Picture.- The Heliosphere in Time.- Origin and Evolution of the Local Bubble and Local ISM.- Origin of the Local Bubble.- Kinetic Fluid Perspective in Modeling in the Heliosphere-Interstellar Medium Interface.- Section IX: Summary.- What Have We Learned?.
