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Discrepancies between empirical and theoretical models of the flaring solar chromosphere and their possible resolution
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Machado, M. E. Emslie, G. A. Brown, J. C. |
| Copyright Year | 1980 |
| Description | Models of the solar chromosphere during flaring deduced theoretically or empirically are compared. Marked discrepancies are noted and various reasons are offered to explain their existence. A means is presented for testing theoretical heating models (electron heating) by analyzing the net energy loss rates in (observed) empirical atmospheres and inverting the flare energy equation to deduce the parameters of the supposed heating mechanism. |
| File Size | 1684542 |
| Page Count | 27 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19810011461 |
| Archival Resource Key | ark:/13960/t53f9k46q |
| Language | English |
| Publisher Date | 1980-08-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Chromosphere Magnetohydrodynamics Solar X-rays Solar Flares Electron Beams Integral Equations Atmospheric Models Brightness Mathematical Models Parameter Identification Sun Solar Flux Density Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |
