Table 1
Summary of magnetic properties at the base of the photosphere derived from the MISMA inversion.
| Portion of photosphere | Field Strength  [G] |
Flux Density ⟨ B ⟩ [G] | Filling Factor α | |||||||||||
| major | minor | major | minor | both | major | minor | both | |||||||
|
|
||||||||||||||
| internetwork (IN) | 1258 | 1521 | 20 | (5.8) | 12 | (3.5) | 32 | (9.3) | 1.6 | (0.5) | 0.7 | (0.2) | 2.3 | (0.7) |
| mixed polarity regions | 1036 | 1041 | 5 | (1.6) | 1 | (0.3) | 6 | (1.9) | 0.5 | (0.1) | 0.1 | (0.0) | 0.6 | (0.1) |
| network | 1513 | 1644 | 23 | (6.7) | 11 | (3.2) | 34 | (9.9) | 1.5 | (0.4) | 0.7 | (0.2) | 2.2 | (0.6) |
| full subfield | 1380 | 1578 | 43 | (12.5) | 23 | (6.7) | 66 | (19.2) | 3.1 | (0.9) | 1.4 | (0.4) | 4.5 | (1.3) |
Notes. The four rows are defined from the four distributions in Fig. 7, which are normalized to the analyzed portion of the photosphere, i.e., 29% of the 29.52″ × 31.70″ subfield. The values normalized to the whole subfield area are reported within parentheses.
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