SOHO MDI 2000-07-07 14:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 90 | 5 | 50 | -16.88 | 34.09 | -4.83 | 168.27 | 0.3681 | 681.1 | 24.1 | |
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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 | -13.05 | 41.56 | 2.64 | 188.87 | 0.2923 | -734.0 | -434.7 | |
| 0 | 5 | 0 | 3 | -12.35 | 40.82 | 1.90 | 186.70 | 0.2789 | -865.0 | -801.0 | |
| 0 | 7 | 0 | 4 | -16.86 | 40.20 | 1.28 | 183.49 | 0.3526 | 375.0 | 265.5 | |
| 0 | 5 | 0 | 3 | -15.89 | 39.61 | 0.70 | 182.00 | 0.3362 | -844.0 | -599.7 | |
| 0 | 4 | 0 | 2 | -15.26 | 39.36 | 0.45 | 181.33 | 0.3257 | -765.0 | -681.6 | |
| 0 | 5 | 0 | 3 | -17.24 | 38.33 | -0.58 | 178.44 | 0.3584 | -736.0 | -617.7 | |
| 0 | 3 | 0 | 2 | -16.86 | 36.51 | -2.40 | 173.47 | 0.3543 | -717.0 | -579.6 | |
| 0 | 6 | 0 | 3 | -16.19 | 35.41 | -3.51 | 170.17 | 0.3460 | -1107.0 | -856.9 | |
| 0 | 4 | 0 | 2 | -18.24 | 32.90 | -6.02 | 165.04 | 0.3873 | -853.0 | -510.5 | |
| 0 | 4 | 0 | 2 | -18.33 | 31.63 | -7.28 | 162.17 | 0.3945 | -747.0 | -674.5 | |
| 0 | 4 | 0 | 2 | -18.81 | 31.19 | -7.72 | 161.56 | 0.4040 | -866.0 | -603.1 | |
| 0 | 5 | 0 | 3 | -18.98 | 30.76 | -8.16 | 160.76 | 0.4088 | -382.0 | -472.0 | |
| 0 | 3 | 0 | 2 | -17.32 | 30.29 | -8.62 | 158.18 | 0.3866 | 397.0 | 411.0 | |
| 9 | 31 | 5 | 17 | -17.59 | 29.52 | -9.39 | 156.72 | 0.3953 | 1349.0 | 960.7 | |
| 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. | |