SOHO MDI 2000-11-09 19:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57 | 377 | 30 | 196 | -12.79 | 176.88 | -8.32 | 153.09 | 0.3134 | 1473.9 | 584.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 1 | -16.42 | 179.17 | -6.03 | 163.38 | 0.3541 | -744.0 | -647.3 | |
| 16 | 332 | 8 | 173 | -13.35 | 177.83 | -7.38 | 156.46 | 0.3143 | 1356.3 | 711.9 | |
| 21 | -2 | 11 | -2 | -12.35 | 177.46 | -7.75 | 154.01 | 0.3018 | 1911.4 | 999999 | |
| 11 | -2 | 6 | -2 | -12.60 | 176.90 | -8.31 | 152.77 | 0.3097 | 1668.9 | 999999 | |
| 9 | -2 | 5 | -2 | -13.04 | 176.84 | -8.36 | 153.27 | 0.3166 | 1132.0 | 999999 | |
| 0 | 4 | 0 | 2 | -13.73 | 175.34 | -9.87 | 150.38 | 0.3384 | 608.0 | 595.5 | |
| 0 | 4 | 0 | 2 | -11.74 | 174.82 | -10.39 | 145.75 | 0.3152 | 516.0 | 567.3 | |
| 0 | 4 | 0 | 2 | -10.71 | 174.69 | -10.51 | 143.46 | 0.3025 | -602.0 | -478.6 | |
| 0 | 4 | 0 | 2 | -14.96 | 174.07 | -11.14 | 149.19 | 0.3661 | -673.0 | -595.4 | |
| 0 | 5 | 0 | 3 | -17.62 | 173.34 | -11.87 | 151.20 | 0.4087 | -403.0 | -355.2 | |
| 0 | 6 | 0 | 3 | -9.31 | 172.95 | -12.25 | 136.12 | 0.3035 | -802.0 | -686.0 | |
| 0 | 11 | 0 | 6 | -11.82 | 171.64 | -13.56 | 138.56 | 0.3484 | -530.0 | -607.4 | |
| 0 | 4 | 0 | 2 | -12.62 | 171.56 | -13.65 | 139.90 | 0.3591 | -770.0 | -661.3 | |
| 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. | |