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Magnetogram and soft x-ray comparisons of xbp and er
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Golub, Leon Harvey, Karen L. Webb, David F. |
| Copyright Year | 1986 |
| Description | The potential importance of the smallest emerging flux regions on the sun was discussed in numerous publications. The association between the objects seen in ground-based data, such as high resolution magnetrons or H alpha and soft X-ray data has produced results which are often contradictory. In the hope of resolving the present impasse, as much simultaneous soft X-ray and magnetogram data as possible were assembled in order to clarify the situation. It was found that separation of magnetic features into chance encounters and emerging flux makes some difference in overlapp with X-ray bright points (XBPs), although the effect is not overwhelming. The difference in solar cycle dependence between XBP and ephemeral regions is not explainable in terms of the results. |
| File Size | 138865 |
| Page Count | 3 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19870011494 |
| Archival Resource Key | ark:/13960/t8hf2qk44 |
| Language | English |
| Publisher Date | 1986-12-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Magnetic Flux Solar Corona X Rays Solar Granulation Polarity Solar Cycles Data Correlation Magnetic Signatures Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
