Basic Mechanisms of Solar Activity: International Astronomical Union Symposia, cartea 71
Editat de V. Bumba, J. Kleczeken Limba Engleză Paperback – 31 dec 1976
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Specificații
ISBN-13: 9789027706812
ISBN-10: 9027706816
Pagini: 500
Ilustrații: 497 p. 39 illus.
Dimensiuni: 170 x 244 x 26 mm
Greutate: 0.79 kg
Ediția:Softcover reprint of the original 1st ed. 1976
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria International Astronomical Union Symposia
Locul publicării:Dordrecht, Netherlands
ISBN-10: 9027706816
Pagini: 500
Ilustrații: 497 p. 39 illus.
Dimensiuni: 170 x 244 x 26 mm
Greutate: 0.79 kg
Ediția:Softcover reprint of the original 1st ed. 1976
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria International Astronomical Union Symposia
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
The Enigma of Solar Activity.- 1/Basic Observed Parameters of the Solar Cycle.- Differential Rotation and Global-Scale Velocity Fields.- Differential Rotation and Giant Cell Circulation of the Solar Ca+-Network.- Rotational Characteristics of Coronal Holes.- On Differences in Differential Rotation.- Large-Scale Solar Magnetic Fields.- Small-Scale Solar Magnetic Fields.- Investigation of Coronal Rotation by the Spectroscopic Method.- Fast Variations of the Solar Rotation.- About the Relation between the Limb Effect of the Redshift on the Sun and the Large-Scale Distribution of Solar Activity.- Drift of Sunspots in Latitude.- Velocities Observed in Supergranules.- Long Term Evolution of Solar Sector Structure.- Solar Cycle Evolution of the General Magnetic Field.- Coronal Bright Points.- Cyclical and Secular Variations of Solar Activity.- Some Results of the Space Distribution of the Activation Vector of the Filaments in the 11-year Cycle.- Sequences of Large Sunspot Groups.- Characteristic Features of Cyclic Change of Solar Activity after 1610.- 2/Solar Convection and Differential Rotation.- Theory of Convection in a Deep Rotating Spherical Shell, and Its Application to the Sun.- The Pattern of Convection in the Sun.- On Theories of Solar Rotation.- Equilibrium Problem in a Rotating Convection Zone.- A Boussinesq Model for the Convection Zone and the Solar Angular Velocity.- Two-Dimensional Stochastic Motions and the Problem of Differential Rotation for Unrestricted Rotational Rates.- 3/Dynamo Theory and Magnetic Dissipation.- Mean-Field Magnetohydrodynamics of the Solar Convection Zone.- Mean-Field Magnetohydrodynamics as a Basis of Solar Dynamo Theory.- Dynamo in the Presence of Differential Rotation.- On Fast Magnetic Field Reconnection.- Dynamo Theory and the Solar Cycle.- Solar Magnetic Fields and Convection. VII: A Review of the Primordial Field Theory.- A Model of the Solar Cycle Driven by the Dynamo Action of the Global Convection in the Solar Convection Zone.- On the Distribution of Angular Velocity in the Sun.- On the Dipole-like Progressive Wave in the Photosphere.- 4/Stellar Activity of the Solar Type.- Stellar Activity of the Solar Type. Observational Aspects.- Chromospheric Variations in Main Sequence Stars.- The Internal Structure of the Sun and Solar Type Stars.- The Sun as a Magnetic Star.- Chromospheric Activity in F- and G-Stars.- Absolute Fluxes of K Chromospheric Emission on the H-R Diagram.- Double-Peaked Flare Events on Red Dwarf Stars and Solar ‘Sympathetic’ Flares.- Conclusions.- Summary of the Final Discussion on August 29.