Loading...
Please wait, while we are loading the content...
Similar Documents
Filament formation due to photospheric shear
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Wu, S. T. Xiao, Y. C. |
| Copyright Year | 1986 |
| Description | Recently, Wu et al. (1983, 1986) developed a three-dimensional, time-dependent axisymmetric ideal magnetohydrodynamic (MHD) model which has been used to study lower solar atmospheric response due to photospheric motion. They have shown that various observed solar features can be formed from these numerical simulation experiments. Some work currently in progress which has resulted from a specific numerical simulation experiment is reported. These results may elucidate the possible physical mechanism of formation of filament. |
| File Size | 149722 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19870011445 |
| Archival Resource Key | ark:/13960/t7mp9xc16 |
| Language | English |
| Publisher Date | 1986-12-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Magnetohydrodynamics Plasmas Physics Solar Prominences Evolution Development Plasma Density Sun Photosphere Solar Temperature Simulation Isotherms Topography Solar Atmosphere Mathematical Models Magnetic Field Configurations Line Spectra Solar Magnetic Field Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
