Table 3
X-ray surface fluxes for magnetic structures (BKC, AR, and CO) in the corona of the Sun obtained from Yohkoh data collected in July 1996 (during a minimum in the solar cycle) within the Sun as an X-ray star framework.
| Region | Minimum | Maximum | Median | Average |
|---|---|---|---|---|
| CH | 3.00 | 3.78 | … | … |
| BKC | 3.37 | 4.30 | 4.14 | 4.10 |
| AR | 4.97 | 5.36 | 5.10 | 5.10 |
| CO | 5.89 | 6.86 | 6.19 | 6.23 |
Notes. Values are logarithmic and given in units of erg cm−2 s−1. The fluxes of solar CHs for a range of plasma temperatures between 1 MK (maximum) and 2 MK (minimum) are from (Schmitt 2012). All values refer to the ROSAT energy band.
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