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Magnetic probing of the solar interior
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Estes, R. H. Benton, E. R. |
| Copyright Year | 1985 |
| Description | The magnetic field patterns in the region beneath the solar photosphere is determined. An approximate method for downward extrapolation of line of sight magnetic field measurements taken at the solar photosphere was developed. It utilizes the mean field theory of electromagnetism in a form thought to be appropriate for the solar convection zone. A way to test that theory is proposed. The straightforward application of the lowest order theory with the complete model fit to these data does not indicate the existence of any reasonable depth at which flux conservation is achieved. |
| File Size | 5053931 |
| Page Count | 75 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850022685 |
| Archival Resource Key | ark:/13960/t4xh4gp4n |
| Language | English |
| Publisher Date | 1985-07-31 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Helioseismology Photosphere Coronas Magnetic Probes Magnetometers Magnetohydrodynamic Turbulence Mathematical Models Magnetic Field Configurations Solar Interior Sunspots Solar Oscillations Solar Magnetic Field Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |