Solar flare magnetic fields and plasmas
This volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfer effects into three-dimensional magnetohydrodynamic models...
Guardat en:
| Altres autors: | , |
|---|---|
| Format: | Livre numérique |
| Idioma: | Anglais |
| Publicat: |
New York, NY :
Springer New York
2012.
Cham : Springer Nature |
| Accés en línia: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Nota: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Solar flare magnetic fields and plasmas, Yuhong Fan, George Fisher, editors, New York, Springer, 2012, 1 vol. (201 p.), 978-1-4614-3760-4 • Solar Flare Magnetic Fields and Plasmas, Texte imprimé, 9781461437628 • Solar Flare Magnetic Fields and Plasmas, Texte imprimé, 9781489999153 |
Taula de continguts:
- Efficient Techniques for Radiation Transfer in Three-Dimensional MHD Models
- Radiative Cooling in MHD Models of the Quiet Sun Convection Zone and Corona
- Understanding Flare Radiation Processes
- Global Forces and Momenta During Solar Flare Energy Release
- The Evolution of Sunspot Magnetic Fields Associated with a Solar Flare
- Global Forces in Eruptive Solar Flares
- Data Analysis and Theory for Analysis of Vector Magnetogram Data
- Modeling and Interpreting the Effects of Spatial Resolution on Solar Magnetic Field Maps
- Magnetic Connectivity Between Active Regions 10987, 10988, 10989 by Means of Nonlinear Force-Free Field Extrapolation
- Magnetic Energy Storage and Current Density Distributions for Different Force-Free Models
- Connections Between Magnetic Topology in the Solar Atmosphere and Eruptive Flares and CMEs
- Predictions of Energy and Helicity in Four Major Eruptive Solar Flares.