The sun and cool stars : activity, magnetism, dynamos : proceedings of Colloquium no. 130 of the International Astronomical Union, held in Helsinki, Finland, 17-20 July 1990

The contributions in this volume report recent studies on the sun and late-type stars. Particular emphasis is placed on observations that are relevant to the question of large-scale magnetic activity, and also on the theoretical (dynamo) models for such activity. Experimental papers deal with surfac...

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Hovedforfatter: Tuominen, Ilkka Vilhelmi, 1939-
Institution som forfatter: Union astronomique internationale. Colloque (Auteur)
Andre forfattere: Moss, D, 1943- (Directeur de la publication), Rüdiger, Günther (Directeur de la publication)
Format: Livre numérique
Sprog:Anglais
Udgivet: Berlin [etc.] : Springer [20..].
Cham : Springer Nature
Serier:Lecture notes in physics 380
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Edition sous un autre format:• The Sun and Cool Stars: activity, magnetism, dynamos, Texte imprimé, 9783540539551
• The Sun and Cool Stars: activity, magnetism, dynamos, Texte imprimé, 9783662138106
• The Sun and Cool Stars: activity, magnetism, dynamos, Texte imprimé, 9783662138113
Indholdsfortegnelse:
  • The confrontation of mean-field theories with numerical simulations
  • On numerical studies of solar/stellar convection
  • Turbulent Convection: A New Model
  • Large scale convection in stars : Towards a model for the action of coherent structures
  • Magnetoconvection patterns in rotating convection zones
  • Stellar convection as a low Prandtl number flow
  • Convective overshoot as a source of helicity
  • Topological pumping in the lower overshoot layer
  • Diffusion of particles, heat and magnetic fields in compressible turbulent media
  • The spatial structure of homogeneous turbulence at high Reynolds number
  • Compressible MHD in spherical geometry
  • The role of overshoot in solar activity: A direct simulation of the dynamo
  • Vector potential magnetic null points
  • Magnetic tubes in overshooting compressible convection
  • Convective cores in stellar models
  • Rotational effects on Reynolds stresses in the solar convection zone
  • Stable and unstable solutions of the nonlinear dynamo problem
  • Nonlinear nonaxisymmetric dynamos for active stars
  • Waves of Solar Activity
  • Non-steady global magnetic fields in kinematic theory
  • Asymptotic methods in the nonlinear mean-field dynamo
  • Fractal flux tubes of the solar magnetic field
  • ??-dynamos
  • Fossil magnetic fields and activity of young stars
  • The sun's internal differential rotation from helioseismology
  • ?-effect, meridional flow and the differential solar rotation
  • Differential rotation as an axisymmetric resonant mode of convection
  • The solar internal rotation and its implications
  • The toroidal magnetic field inside the Sun
  • The transfer of large-scale magnetic field by radial inhomogeneity of the material density in the rotating convection zone
  • Diagnostics of the solar dynamo using the observed pattern of surfacemagnetic fields
  • The large-scale magnetic field in the global solar cycle: observational aspects
  • Evolution of large and small scale magnetic fields in the sun
  • The solar dynamo
  • A topological model of the solar magnetic field reversals
  • Solar internal rotation, the boundary layer dynamo and latitude distribution of activity belts
  • Solar rotation over solar cycle 21
  • Sun-as-a-star: Its convective signature and the activity cycle
  • The hel ?10830 Å line as an indicator of the chromospheric and coronal activity of the sun
  • The rotational modulation of ca II K in the sun
  • The prolonged minima and maxima of solar activity
  • The longer term evolution of magnetic field and mass flow in a decaying active region
  • The main component analysis of the longitudinal distribution of solar activity
  • Fe I line asymmetries and shifts caused by pressure broadening
  • Rotation of large scale patterns on the solar surface as determined from filament and millimeter data
  • Large scale patterns on the solar surface indicated by microwave observations
  • The solar corona over the recent saros
  • The history of activity of the Sun and its rotational period on the ZAMS
  • The differential rotation and evolution of spots on UX Arietis from a sequence of Doppler images
  • The art of surface imaging
  • Surface imaging of El Eri
  • Towards magnetic images of rapidly rotating late-type stars
  • Chromospheric surface structures on El Eridani and HD 199178
  • Activity, colour anomalies and temperature determination in solar-type stars
  • Dynamo action in evolved stars
  • The boundary between the magnetic fields of ap stars and the fields of solar-type stars
  • Doppler mapping of CP-star surfaces with weak and strong magnetic fields
  • Temperature variations on the surface of the Si-star CU Virginis.-Learning about stellar dynamos from long-term photometry of starspots
  • Starspot activity on short-period RS CVn stars
  • Variations in spottedness of photosphere and chromosphere of the flare star EV Lac
  • Surface inhomogeneities on the W UMa star AC Bootis
  • Long-term starspot behavior of BY Dra and EV Lac
  • The spot activity of FK Comae Berenices
  • On the existence of solar-type activity in the secondary components of cataclysmic variables
  • Radial velocity variability of K giants
  • Recent advances in the observation and analysis of stellar magnetic fields
  • Limits on the magnetic flux of a pre-main sequence star
  • Stellar zeeman analyses: Effects of multi-component atmospheres
  • Multi-line Zeeman analysis
  • A new technique to measure magnetic field strength in active stars
  • Magnetic flux determination in late-type dwarfs
  • Linear polarization and magnetic fields in cool stars
  • Long-term polarimetric activity of the cool supergiant Cephei
  • Polarimetric observations of active cool binaries
  • Magnetic fields and filling factors in late-type stars: Predictions from dynamo theory
  • Activity of relatively close binaries
  • Two kinds of activity in late-type stars
  • Ca II H and K and H?, and Li abundances in the pleiades late K main-sequence
  • Is ? Boo AB a young or an evolved system? a model atmosphere analysis
  • Spectroscopic analysis of HR 1099
  • Recent advances in our understanding of chromospheric and coronal heating mechanisms
  • Ca II H high-resolution spectral monitoring of active late-type dwarfs
  • The onset of chromospheres in A-type stars: The altair affair
  • H? and NaD line variability in RY Tauri
  • He I 5876 å line in the study of chromospheric activity in F-type MS stars
  • The age evolution of Ca II emission in late type stars
  • Ca II H and Kspectroscopy of ER Vul
  • The variations of the H? line of HD199178
  • H? emission in the giant components of RS CVn systems
  • Spectroscopy of southern active stars
  • Full phase coverage of by Dra with the VLA
  • Coronal magnetic fields of Algol binaries from microwave spectra
  • On the coronal activity of RS CVn systems
  • Flare rate spectra as a possibility of diagnostics of convection zones in stars
  • Observations relating to stellar activity, magnetism and dynamos
  • Concluding summary: Theoretical aspects.