SOHO MDI 2000-01-25 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 121 | 603 | 68 | 349 | 5.07 | 71.39 | 28.95 | 289.69 | 0.5139 | -188.9 | 92.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 250 | 4 | 148 | 4.50 | 74.36 | 31.92 | 286.76 | 0.5526 | 1022.6 | 789.9 | |
| 18 | -1 | 10 | -1 | 4.03 | 74.29 | 31.85 | 285.98 | 0.5497 | 1523.8 | 999999 | |
| 4 | -1 | 2 | -1 | 4.29 | 73.90 | 31.45 | 286.63 | 0.5452 | 1685.6 | 999999 | |
| 7 | -1 | 4 | -1 | 3.93 | 73.84 | 31.39 | 286.04 | 0.5429 | 1836.6 | 999999 | |
| 8 | -1 | 5 | -1 | 4.67 | 73.82 | 31.38 | 287.34 | 0.5459 | 1295.1 | 999999 | |
| 5 | -1 | 3 | -1 | 4.55 | 72.97 | 30.52 | 287.61 | 0.5333 | 1523.7 | 999999 | |
| 0 | 7 | 0 | 4 | 4.55 | 72.08 | 29.63 | 288.13 | 0.5208 | 717.0 | 708.6 | |
| 0 | 9 | 0 | 5 | 3.96 | 71.96 | 29.52 | 287.11 | 0.5164 | 877.0 | 744.9 | |
| 0 | 8 | 0 | 5 | 4.71 | 71.51 | 29.07 | 288.79 | 0.5135 | 672.0 | 548.6 | |
| 0 | 4 | 0 | 3 | 4.05 | 71.39 | 28.95 | 287.62 | 0.5087 | 870.0 | 761.6 | |
| 6 | 325 | 3 | 184 | 5.69 | 69.90 | 27.45 | 291.72 | 0.4959 | -16.2 | -523.8 | |
| 24 | -11 | 13 | -11 | 5.24 | 69.40 | 26.95 | 291.24 | 0.4863 | -1472.8 | 999999 | |
| 15 | -11 | 9 | -11 | 5.67 | 69.38 | 26.93 | 292.07 | 0.4884 | -1272.9 | 999999 | |
| 7 | -11 | 4 | -11 | 6.64 | 69.39 | 26.94 | 293.90 | 0.4943 | -1196.9 | 999999 | |
| 20 | -11 | 11 | -11 | 6.23 | 68.84 | 26.40 | 293.56 | 0.4843 | -1752.5 | 999999 | |
| 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. | |