Advances in solar physics : proceedings of the Seventh European Meeting on Solar Physics Held in Catania, Italy, 11 15 May 1993
This book begins with a very readable survey "The Sun Today" by J.-C. Pecker. It is followed by thorough reviews from leading experts covering theory and observations. The focus shifts from the solar core, studied via neutrino emissions and helioseismology, through the interface regions wh...
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| מחברים אחרים: | , , |
| פורמט: | Livre numérique |
| שפה: | Anglais |
| יצא לאור: |
Berlin ; Paris [etc.] :
Springer-Verlag : Springer e-books
[20..].
Cham : Springer Nature |
| סדרה: | Lecture notes in physics
432 |
| נושאים: | |
| גישה מקוונת: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| הערה: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Advances in solar physics, proceedings of the Seventh European Meeting on Solar Physics, held at Catania, Italy, 11-15 May 1993, G. Belvedere, M. Rodonò, G.M. Simnett, (eds.), Berlin, Springer-Verlag, 1994, 1 vol. (335 p.), Lecture notes in physics, 3-540-58041-7 • Advances in Solar Physics, Texte imprimé, 9783662139837 • Advances in Solar Physics, Texte imprimé, 9783662139844 |
תוכן הענינים:
- The Sun today
- Recent results from helioseismology
- The structure of the solar core
- New sub-barrier nuclear fusion cross sections as a possible solution to the solar neutrino problem
- Helioseismic evidence for mixing in the radiative interior
- Microscopic settling and turbulent diffusion induced by rotation in the sun
- Mean-field theory of the solar dynamo
- Hydrodynamical simulations of the solar dynamo
- The asymmetric behaviour of solar activity
- On the possibility of supergiant stable flows in the convection zone of the sun
- Stellar dynamos
- On magnetic fields, rossby numbers and dynamo action in late-type stars
- The magnetic field of the solar corona
- The control of the corona by the convective zone magnetic fields
- Line-tying in a gravitationally stratified atmosphere
- Magnetic fields surrounding coronal holes
- Coronal heating mechanisms
- Coronal heating via nanoflares
- Magnetic structures of the intermediate corona
- Oscillations in quiescent prominences
- Pressure diagnostics of coronal loops observed by NIXT
- Quiet sun from multifrequency radio observations on RATAN-600
- Frequency spectra of solar microwave bursts associated with coronal mass ejections
- Observations of high-energy (E?10 MeV) gamma-rays with the PHEBUS instrument
- Observational characteristics of explosive events
- Plasma physics of explosive phenomena
- A search for small solar flares with BATSE
- Solar flares and laboratory experiments
- Particle acceleration and radiation generation by nonlinear mode-mode coupling processes in the solar corona
- A fast mechanism for the acceleration of solar energetic particles in solar flares
- Acceleration and storage of energetic particles in the solar corona
- Electromagnetic signatures of particle acceleration and propagation.-Proton acceleration in long duration flares
- Signatures of proton beams in the Ly? profile: Sensitivity of the diagnostics
- Ground based instrumentation
- Space instrumentation
- The Yohkoh mission: Instruments and recent results
- High resolution solar observations: Spectropolarimetry with THEMIS
- Conference summary.