Dynamics of the sun and stars : honoring the life and work of Michael J. Thompson / / Mario J. P. F. G. Monteiro [and three others], editors |
Edizione | [1st ed. 2020.] |
Pubbl/distr/stampa | Cham, Switzerland : , : Springer, , [2020] |
Descrizione fisica | 1 online resource (XIV, 343 p. 110 illus., 23 illus. in color.) |
Disciplina | 523.7 |
Collana | Astrophysics and space science proceedings |
Soggetto topico |
Helioseismology
Astroseismology |
ISBN | 3-030-55336-1 |
Formato | Materiale a stampa |
Livello bibliografico | Monografia |
Lingua di pubblicazione | eng |
Nota di contenuto | Part I: The Life and Work of Michael J. Thompson -- Michael Thompson’s Legacy in Solar and Stellar Physics -- Michael Thompson in Sheffield -- Michael J. Thompson: A Remarkable Scientist, Leader, and Friend -- Michael -- Assessing the Threat of Major Outbreaks of Vector-Borne Diseases Under a Changing Climate -- Touching the Interior Structure and Dynamics of Our Nearest Star -- Part II: Solar Interior and Dynamics -- Uncovering the Hidden Layers of the Sun -- Solar Rotation -- On Solar and Solar-Like Stars Convection, Rotation and Magnetism -- Recent Progress in Local Helioseismology -- Time-Distance Helioseismology of Deep Meridional Circulation -- Surface Rotation and Magnetic Activity of Solar-Like Stars: Impact on Seismic Detections -- Study of Acoustic Halos in NOAA Active Region 12683 -- Helioseismic Center-to-Limb Effect and Measured Travel-Time Asymmetries Around Sunspots -- Probing the Variation with Depth of the Solar Meridional Circulation Using Legendre Function Decomposition -- New Inversion Scheme for Time-Distance Helioseismology -- On Active Region Emergence Precursors -- Solar Hemispheric Helicity Rules: A New Explanation -- Comparing Solar Activity Minima Using Acoustic Oscillation Frequencies -- Solar Cycle Variation of Large Scale Plasma Flows -- Measuring the Dispersion Relation of Acoustic-Gravity Waves in the Solar Atmosphere -- Non-adiabatic Helioseismology via 3D Convection Simulations -- Part III: From the Sun to the Stars -- Deciphering Solar Convection -- G Modes and the Solar Core -- Inverse Analysis of Asteroseismic Data: A Review -- Diagnostics from Solar and Stellar Glitches -- Dynamo States with Strikingly Different Symmetries Coexisting in Global Solar Simulations -- Influence of Turbulence on an Essentially Nonlinear Dynamo Mechanism -- Part IV: Stellar Dynamics -- The Tachocline Revisited -- Seismic Signatures of Solar and Stellar Magnetic Activity -- Confinement of Magnetic Fields Below the Solar Convection Zone -- Asteroseismic Study of KIC 11145123: Its Structure and Rotation -- The Impact of a Fossil Magnetic Field on Dipolar Mixed-Mode Frequencies in Sub- and Red-Giant Stars -- Asteroseismic Stellar Modelling: Systematics from the Treatment of the Initial Helium Abundance -- Direct Travel Time of X-ray Class Solar Storms -- On the Limits of Seismic Inversions for Radial Differential Rotation of Solar-Type Stars -- The Physical Origin of the Luminosity Maximum of the RGB-Bump -- A New Utility to Study Strong Chemical Gradients in Stellar Interiors -- 16 Cygni A: A Testbed for Stellar Core Physics -- Exploring the Origins of Intense Magnetism in Early M-Dwarf Stars -- Part V: The Future -- A Future Path for Solar Synoptic Ground-Based Observations -- Observational Asteroseismology of Solar-Like Oscillators in the 2020s and Beyond -- Oblique Pulsation: New, Challenging Observations with TESS Data -- Accounting for Asphericity -- A Comparison of Global Helioseismic-Instrument Performances: Solar-SONG, GOLF and VIRGO -- Open Discussion -- Contemplating the Future. |
Record Nr. | UNISA-996418437703316 |
Cham, Switzerland : , : Springer, , [2020] | ||
Materiale a stampa | ||
Lo trovi qui: Univ. di Salerno | ||
|
Dynamics of the sun and stars : honoring the life and work of Michael J. Thompson / / Mario J. P. F. G. Monteiro [and three others], editors |
Edizione | [1st ed. 2020.] |
Pubbl/distr/stampa | Cham, Switzerland : , : Springer, , [2020] |
Descrizione fisica | 1 online resource (XIV, 343 p. 110 illus., 23 illus. in color.) |
Disciplina | 523.7 |
Collana | Astrophysics and space science proceedings |
Soggetto topico |
Helioseismology
Astroseismology |
ISBN | 3-030-55336-1 |
Formato | Materiale a stampa |
Livello bibliografico | Monografia |
Lingua di pubblicazione | eng |
Nota di contenuto | Part I: The Life and Work of Michael J. Thompson -- Michael Thompson’s Legacy in Solar and Stellar Physics -- Michael Thompson in Sheffield -- Michael J. Thompson: A Remarkable Scientist, Leader, and Friend -- Michael -- Assessing the Threat of Major Outbreaks of Vector-Borne Diseases Under a Changing Climate -- Touching the Interior Structure and Dynamics of Our Nearest Star -- Part II: Solar Interior and Dynamics -- Uncovering the Hidden Layers of the Sun -- Solar Rotation -- On Solar and Solar-Like Stars Convection, Rotation and Magnetism -- Recent Progress in Local Helioseismology -- Time-Distance Helioseismology of Deep Meridional Circulation -- Surface Rotation and Magnetic Activity of Solar-Like Stars: Impact on Seismic Detections -- Study of Acoustic Halos in NOAA Active Region 12683 -- Helioseismic Center-to-Limb Effect and Measured Travel-Time Asymmetries Around Sunspots -- Probing the Variation with Depth of the Solar Meridional Circulation Using Legendre Function Decomposition -- New Inversion Scheme for Time-Distance Helioseismology -- On Active Region Emergence Precursors -- Solar Hemispheric Helicity Rules: A New Explanation -- Comparing Solar Activity Minima Using Acoustic Oscillation Frequencies -- Solar Cycle Variation of Large Scale Plasma Flows -- Measuring the Dispersion Relation of Acoustic-Gravity Waves in the Solar Atmosphere -- Non-adiabatic Helioseismology via 3D Convection Simulations -- Part III: From the Sun to the Stars -- Deciphering Solar Convection -- G Modes and the Solar Core -- Inverse Analysis of Asteroseismic Data: A Review -- Diagnostics from Solar and Stellar Glitches -- Dynamo States with Strikingly Different Symmetries Coexisting in Global Solar Simulations -- Influence of Turbulence on an Essentially Nonlinear Dynamo Mechanism -- Part IV: Stellar Dynamics -- The Tachocline Revisited -- Seismic Signatures of Solar and Stellar Magnetic Activity -- Confinement of Magnetic Fields Below the Solar Convection Zone -- Asteroseismic Study of KIC 11145123: Its Structure and Rotation -- The Impact of a Fossil Magnetic Field on Dipolar Mixed-Mode Frequencies in Sub- and Red-Giant Stars -- Asteroseismic Stellar Modelling: Systematics from the Treatment of the Initial Helium Abundance -- Direct Travel Time of X-ray Class Solar Storms -- On the Limits of Seismic Inversions for Radial Differential Rotation of Solar-Type Stars -- The Physical Origin of the Luminosity Maximum of the RGB-Bump -- A New Utility to Study Strong Chemical Gradients in Stellar Interiors -- 16 Cygni A: A Testbed for Stellar Core Physics -- Exploring the Origins of Intense Magnetism in Early M-Dwarf Stars -- Part V: The Future -- A Future Path for Solar Synoptic Ground-Based Observations -- Observational Asteroseismology of Solar-Like Oscillators in the 2020s and Beyond -- Oblique Pulsation: New, Challenging Observations with TESS Data -- Accounting for Asphericity -- A Comparison of Global Helioseismic-Instrument Performances: Solar-SONG, GOLF and VIRGO -- Open Discussion -- Contemplating the Future. |
Record Nr. | UNINA-9910431343203321 |
Cham, Switzerland : , : Springer, , [2020] | ||
Materiale a stampa | ||
Lo trovi qui: Univ. Federico II | ||
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