SOHO MDI 2000-11-02 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84 | 511 | 44 | 263 | -10.31 | 276.98 | 2.18 | 190.02 | 0.2636 | -953.3 | -391.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47 | 304 | 24 | 156 | -9.40 | 279.93 | 5.13 | 200.73 | 0.2503 | -1949.1 | -683.2 | |
| 14 | 59 | 7 | 30 | -9.79 | 278.18 | 3.37 | 193.60 | 0.2477 | -1386.8 | -673.6 | |
| 0 | 5 | 0 | 2 | -7.65 | 277.65 | 2.85 | 193.61 | 0.2103 | -425.0 | -350.5 | |
| 0 | 7 | 0 | 3 | -8.76 | 277.23 | 2.43 | 190.67 | 0.2272 | -751.0 | -577.6 | |
| 0 | 6 | 0 | 3 | -8.79 | 276.92 | 2.12 | 189.30 | 0.2269 | -737.0 | -668.5 | |
| 0 | 7 | 0 | 4 | -7.93 | 276.76 | 1.96 | 189.22 | 0.2118 | -775.0 | -682.1 | |
| 0 | 4 | 0 | 2 | -10.89 | 274.19 | -0.61 | 177.67 | 0.2599 | -461.0 | -590.4 | |
| 0 | 7 | 0 | 4 | -12.87 | 270.55 | -4.25 | 166.07 | 0.3016 | -734.0 | -471.8 | |
| 3 | 9 | 2 | 5 | -13.88 | 270.29 | -4.51 | 166.09 | 0.3190 | -1158.0 | -839.7 | |
| 0 | 6 | 0 | 3 | -13.15 | 269.95 | -4.85 | 164.45 | 0.3088 | 1133.0 | 804.3 | |
| 0 | 10 | 0 | 5 | -16.37 | 269.80 | -5.01 | 166.52 | 0.3607 | -1064.0 | -866.3 | |
| 13 | 46 | 7 | 24 | -11.67 | 269.51 | -5.30 | 161.56 | 0.2872 | 1523.7 | 1002.9 | |
| 0 | 5 | 0 | 3 | -13.40 | 269.47 | -5.33 | 163.23 | 0.3149 | 1081.0 | 871.8 | |
| 0 | 5 | 0 | 3 | -16.70 | 269.26 | -5.54 | 165.39 | 0.3681 | -716.0 | -543.9 | |
| 0 | 3 | 0 | 1 | -13.94 | 267.82 | -6.98 | 159.10 | 0.3321 | 556.0 | 466.8 | |
| 7 | 28 | 4 | 15 | -13.49 | 267.64 | -7.17 | 158.08 | 0.3265 | 1168.2 | 976.7 | |
| 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. | |