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Model development for ulysses and soho
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Wu, S. T. |
| Copyright Year | 1993 |
| Description | The purpose of this research is to provide scientific expertise in solar physics and in the development and use of magnetohydrodynamic (MHD) models of coronal structures for the computation of Lyman alpha scattered radiation in these structures. The specific objectives will be to run MHD models with new boundary conditions and compute resulting scattered solar Lyman alpha intensities, guided by results from the first series of boundary conditions. |
| File Size | 2204003 |
| Page Count | 43 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19940020011 |
| Archival Resource Key | ark:/13960/t9b61h24v |
| Language | English |
| Publisher Date | 1993-11-27 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Solar Corona Ulysses Mission Magnetohydrodynamics Lyman Alpha Radiation Soho Mission Two Dimensional Models Stellar Radiation Boundary Conditions Solar Magnetic Field Stellar Models Stellar Structure 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 |