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 estim
โฆ LIBER โฆ
Short-term temporal variations of X-ray bright points
โ Scribed by J. T. Nolte; C. V. Solodyna; M. Gerassimenko
- Publisher
- Springer
- Year
- 1979
- Tongue
- English
- Weight
- 674 KB
- Volume
- 63
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
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 a sudden turn-off of the steady heating.
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