SOHO MDI 2000-10-29 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24 | 170 | 20 | 129 | -28.54 | 293.11 | -37.92 | 134.55 | 0.7596 | 717.0 | 405.2 | |
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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 | -28.93 | 302.35 | -28.67 | 142.27 | 0.6886 | -502.0 | -341.4 | |
| 0 | 4 | 0 | 3 | -26.82 | 296.52 | -34.50 | 135.13 | 0.7189 | 604.0 | 544.3 | |
| 0 | 3 | 0 | 3 | -27.34 | 296.02 | -35.01 | 135.32 | 0.7270 | 616.0 | 551.3 | |
| 0 | 3 | 0 | 2 | -28.33 | 295.33 | -35.70 | 135.87 | 0.7400 | 473.0 | 480.8 | |
| 0 | 3 | 0 | 2 | -27.47 | 295.23 | -35.80 | 134.87 | 0.7347 | 434.0 | 397.5 | |
| 0 | 2 | 0 | 2 | -28.10 | 294.50 | -36.53 | 135.01 | 0.7452 | 608.0 | 451.1 | |
| 0 | 5 | 0 | 4 | -26.77 | 294.79 | -36.24 | 133.78 | 0.7334 | 800.0 | 690.9 | |
| 14 | 85 | 11 | 65 | -29.53 | 293.29 | -37.74 | 135.69 | 0.7648 | 822.8 | 356.5 | |
| -8 | -8 | -8 | -8 | -29.32 | 292.87 | -38.15 | 135.19 | 0.7666 | 999999 | 999999 | |
| 0 | 5 | 0 | 4 | -30.23 | 292.34 | -38.68 | 135.79 | 0.7767 | -118.0 | -6.1 | |
| 3 | 18 | 3 | 14 | -28.02 | 293.32 | -37.71 | 134.11 | 0.7543 | 709.5 | 663.3 | |
| 0 | 4 | 0 | 3 | -26.60 | 293.78 | -37.25 | 132.87 | 0.7409 | 504.0 | 433.2 | |
| 0 | 2 | 0 | 2 | -28.18 | 292.86 | -38.16 | 133.97 | 0.7591 | 340.0 | 378.3 | |
| 0 | 3 | 0 | 2 | -27.20 | 292.55 | -38.48 | 132.70 | 0.7553 | 559.0 | 497.2 | |
| 0 | 5 | 0 | 3 | -27.85 | 292.16 | -38.86 | 133.15 | 0.7627 | 326.0 | 395.8 | |
| 7 | 24 | 6 | 18 | -27.05 | 290.24 | -40.79 | 131.05 | 0.7737 | 658.8 | 420.9 | |
| 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. | |