SOHO MDI 2000-09-06 11:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60 | 258 | 33 | 144 | 9.96 | 340.97 | 27.28 | 277.90 | 0.4578 | 66.5 | 63.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 10 | 0 | 6 | 6.75 | 346.95 | 33.26 | 271.23 | 0.5469 | -439.0 | -315.7 | |
| 0 | 9 | 0 | 5 | 7.44 | 346.02 | 32.33 | 272.45 | 0.5328 | -742.0 | -705.0 | |
| 0 | 3 | 0 | 2 | 7.14 | 344.60 | 30.91 | 271.78 | 0.5120 | -732.0 | -574.2 | |
| 9 | 96 | 5 | 54 | 9.27 | 342.58 | 28.89 | 276.07 | 0.4814 | 1160.5 | 980.9 | |
| 13 | -4 | 7 | -4 | 9.99 | 342.37 | 28.68 | 277.60 | 0.4788 | 1355.8 | 999999 | |
| 9 | -4 | 5 | -4 | 9.74 | 342.08 | 28.39 | 277.09 | 0.4741 | 1653.0 | 999999 | |
| 0 | 7 | 0 | 4 | 9.10 | 341.57 | 27.88 | 275.76 | 0.4660 | 1038.0 | 865.3 | |
| 0 | 8 | 0 | 5 | 9.70 | 341.40 | 27.71 | 277.07 | 0.4637 | 563.0 | 517.1 | |
| 0 | 13 | 0 | 7 | 9.44 | 341.06 | 27.37 | 276.55 | 0.4584 | 887.0 | 687.6 | |
| 0 | 6 | 0 | 3 | 11.19 | 340.15 | 26.46 | 280.56 | 0.4465 | -346.0 | -491.2 | |
| 9 | 26 | 5 | 14 | 11.31 | 339.27 | 25.58 | 281.07 | 0.4332 | -1049.8 | -820.4 | |
| 0 | 7 | 0 | 4 | 10.55 | 338.71 | 25.02 | 279.45 | 0.4233 | -828.0 | -632.4 | |
| 11 | 66 | 6 | 36 | 11.28 | 338.38 | 24.69 | 281.25 | 0.4195 | -1335.5 | -898.4 | |
| 0 | 3 | 0 | 2 | 3.61 | 337.88 | 24.19 | 262.67 | 0.4141 | -588.0 | -465.1 | |
| 9 | -13 | 5 | -13 | 11.10 | 338.06 | 24.37 | 280.91 | 0.4141 | -1566.3 | 999999 | |
| 0 | 4 | 0 | 2 | 11.19 | 337.15 | 23.46 | 281.40 | 0.4001 | 497.0 | 339.0 | |
| 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. | |