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Filament eruption onset
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Sterling, Alphonse C. Moore, Ronald L. |
| Copyright Year | 2011 |
| Description | We have been investigating filament eruptions in recent years. Use filament eruptions as markers of the coronal field evolution. Data from SoHO, Yohkoh, TRACE, Hinode, and other sources. We and others have observed: (1)Filaments often show slow rise, followed by fast rise, (2) Brightenings, preflares, microflares during slow rise (3) Magnetic evolution in hours prior to eruption onset. We investigated What do Hinode and SDO show for filament eruptions? |
| File Size | 3578387 |
| Page Count | 47 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20120004175 |
| Archival Resource Key | ark:/13960/t1dk0dw1r |
| Language | English |
| Publisher Date | 2011-12-13 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Solar Corona Solar Flares Soho Mission Solar Prominences Solar Magnetic Field Sun Transition Region and Coronal Explorer Solar Observatories Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Presentation |