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A search for outflows from x-ray bright points in coronal holes
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Mullan, D. J. Waldron, W. L. |
| Copyright Year | 1986 |
| Description | Properties of X-ray bright points using two of the instruments on Solar Maximum Mission were investigated. The mass outflows from magnetic regions were modeled using a two dimensional MHD code. It was concluded that mass can be detected from X-ray bright points provided that the magnetic topology is favorable. |
| File Size | 2320847 |
| Page Count | 84 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19860012987 |
| Archival Resource Key | ark:/13960/t3615x83x |
| Language | English |
| Publisher Date | 1986-04-07 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Solar X-rays Solar Flares Coronal Holes Magnetic Disturbances Solar Flux Velocity Distribution Solar Maximum Mission Doppler Effect 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 |