Skylab S-054 data have been used to examine the flux from X-ray bright points with -90 s time resolution. There is evidence of a steady heating input, similar to one reported for active region loops. Also observed are impulsive brightenings of bright points and rapid decays which are consistent with
Observation of spatial and temporal variations in X-ray bright point emergence patterns
โ Scribed by Leon Golub; Allen S. Krieger; Giuseppe S. Vaiana
- Publisher
- Springer
- Year
- 1976
- Tongue
- English
- Weight
- 820 KB
- Volume
- 50
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
Observations of X-ray bright points (XBP) over a six-month interval in 1973 show significant variations in both the number density of XBP as a function of heliographic longitude and in the full Sun average number of XBP from one rotation to the next. The observed increases in XBP emergence are estimated tO be quivalent to several large active regions emerging per day for several months. The number of XBP emerging at high latitudes also varies, in phase with the low latitude variation and reaches a maximum approximately simultaneous with a major outbreak of active regions. The quantity of magnetic flux emerging in the form of XBP at high latitudes alone is estimated to be as large as the contribution from all active regions.
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