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Theoretical motivation for high spatial resolution, hard x-ray observations during solar flares
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Emslie, A. G. |
| Copyright Year | 1986 |
| Description | The important role played by hard X-ray radiation as a diagnostic of impulsive phase energy transport mechanism is reviewed. It is argued that the sub-arc second resolution offered by an instrument such as the Pinhole/Occulter Facility (P/OF) can greatly increase our understanding of such mechanisms. |
| File Size | 470904 |
| Page Count | 7 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19860015151 |
| Archival Resource Key | ark:/13960/t08w8999c |
| Language | English |
| Publisher Date | 1986-04-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Impulses Solar X-rays Solar Flares Bremsstrahlung Pinhole Occulter Facility High Energy Interactions Spatial Resolution Electrons Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
