Listing 1 - 10 of 24 | << page >> |
Sort by
|
Choose an application
Choose an application
Helioseismology --- Astroseismology --- Stars --- Sun
Choose an application
Choose an application
Helioseismology --- Astroseismology --- Conferences - Meetings --- Helioseismology - Congresses --- Astroseismology - Congresses
Choose an application
Helioseismology has enabled us to probe the internal structure and dynamics of the Sun, including how its rotation varies in the solar interior. The unexpected discovery of an abrupt transition - the tachocline - between the differentially rotating convection zone and the uniformly rotating radiative interior has generated considerable interest and raised many fundamental issues. This volume contains invited reviews from distinguished speakers at the first meeting devoted to the tachocline, held at the Isaac Newton Institute. It provides a comprehensive account of the understanding of the properties and dynamics of the tachocline, including both observational results and major theoretical issues, involving both hydrodynamic and magnetohydrodynamic behaviour. The Solar Tachocline is a valuable reference for researchers and graduate students in astrophysics, heliospheric physics and geophysics, and the dynamics of fluids and plasmas.
Helioseismology. --- Solar dynamics --- Solar seismology --- Astroseismology --- Sun. --- Solar system
Choose an application
Astroseismology --- Helioseismology --- Stars --- Congresses --- Congresses --- Structure --- Congresses --- Delache, Philippe.
Choose an application
Choose an application
This volume presents a full mathematical exposition of the growing field of coronal seismology which will prove invaluable for graduate students and researchers alike. Roberts' detailed and original research draws upon the principles of fluid mechanics and electromagnetism, as well as observations from the TRACE and SDO spacecraft and key results in solar wave theory. The unique challenges posed by the extreme conditions of the Sun's atmosphere, which often frustrate attempts to develop a comprehensive theory, are tackled with rigour and precision; complex models of sunspots, coronal loops and prominences are presented, based on a magnetohydrodynamic (MHD) view of the solar atmosphere, and making use of Faraday's concept of magnetic flux tubes to analyse oscillatory phenomena. The rapid rate of progress in coronal seismology makes this essential reading for those hoping to gain a deeper understanding of the field.
Helioseismology. --- Magnetohydrodynamic waves. --- Fluid dynamics. --- Solar atmosphere. --- Electromagnetism.
Choose an application
Astroseismology --- Helioseismology --- Solar dynamics --- Solar seismology --- Astero-seismology --- Asteroseismology --- Extraterrestrial seismology --- Stellar oscillations --- Helioseismology - Congresses. --- Astroseismology - Congresses.
Choose an application
Sun --- Soleil --- Corona. --- Couronne --- Solar atmosphere --- Helioseismology --- Magnetohydrodynamics --- Solar oscillations --- Solar dynamics --- Solar seismology --- Astroseismology --- Corona
Listing 1 - 10 of 24 | << page >> |
Sort by
|