SOHO MDI 2000-11-09 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60 | 353 | 30 | 183 | -12.50 | 176.85 | -5.72 | 160.32 | 0.2919 | 1478.7 | 602.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -11.59 | 178.43 | -4.15 | 164.61 | 0.2681 | 584.0 | 492.8 | |
| 14 | 304 | 7 | 157 | -13.31 | 177.80 | -4.77 | 164.22 | 0.2987 | 1375.4 | 749.9 | |
| 20 | -2 | 10 | -2 | -12.32 | 177.47 | -5.10 | 162.12 | 0.2843 | 1939.8 | 999999 | |
| 5 | -2 | 3 | -2 | -12.96 | 177.34 | -5.24 | 162.39 | 0.2952 | 1229.2 | 999999 | |
| 12 | -2 | 6 | -2 | -12.64 | 176.87 | -5.70 | 160.56 | 0.2927 | 1736.4 | 999999 | |
| 9 | -2 | 4 | -2 | -13.00 | 176.82 | -5.75 | 160.82 | 0.2986 | 1304.2 | 999999 | |
| 0 | 5 | 0 | 2 | -9.11 | 176.58 | -5.99 | 154.41 | 0.2396 | -552.0 | -400.0 | |
| 0 | 5 | 0 | 3 | -12.00 | 176.21 | -6.36 | 157.68 | 0.2867 | 648.0 | 489.6 | |
| 0 | 3 | 0 | 2 | -13.61 | 175.33 | -7.24 | 157.17 | 0.3170 | 540.0 | 502.5 | |
| 0 | 5 | 0 | 3 | -9.09 | 174.74 | -7.83 | 147.90 | 0.2543 | -803.0 | -602.7 | |
| 0 | 6 | 0 | 3 | -8.86 | 173.73 | -8.85 | 144.16 | 0.2607 | -533.0 | -512.6 | |
| 0 | 4 | 0 | 2 | -9.30 | 173.08 | -9.49 | 143.24 | 0.2731 | -714.0 | -714.7 | |
| 0 | 4 | 0 | 2 | -13.08 | 171.75 | -10.82 | 147.00 | 0.3371 | -701.0 | -560.4 | |
| 0 | 6 | 0 | 3 | -12.60 | 171.70 | -10.88 | 146.04 | 0.3311 | -785.0 | -688.0 | |
| 0 | 5 | 0 | 3 | -10.34 | 171.23 | -11.34 | 140.55 | 0.3060 | -689.0 | -507.8 | |
| 0 | 2 | 0 | 1 | -11.03 | 169.92 | -12.65 | 138.92 | 0.3286 | -660.0 | -664.8 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |