SOHO MDI 2002-08-01 07:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33 | 156 | 19 | 83 | -8.50 | 145.20 | -11.02 | 143.03 | 0.3128 | 306.6 | 240.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3 | 9 | 2 | 5 | -8.86 | 150.07 | -6.15 | 157.28 | 0.2753 | -1020.9 | -734.9 | |
| 0 | 2 | 0 | 1 | -8.95 | 149.66 | -6.55 | 156.08 | 0.2793 | -720.0 | -701.4 | |
| 0 | 4 | 0 | 2 | -8.78 | 149.55 | -6.67 | 155.45 | 0.2776 | -743.0 | -590.1 | |
| 0 | 9 | 0 | 5 | -7.17 | 148.61 | -7.61 | 149.58 | 0.2607 | 722.0 | 474.8 | |
| 0 | 3 | 0 | 2 | -7.62 | 148.32 | -7.90 | 149.51 | 0.2697 | 787.0 | 683.3 | |
| 0 | 6 | 0 | 3 | -7.25 | 148.25 | -7.97 | 148.57 | 0.2651 | 1052.0 | 916.0 | |
| 0 | 5 | 0 | 3 | -8.03 | 148.19 | -8.03 | 149.87 | 0.2767 | 912.0 | 669.8 | |
| 0 | 5 | 0 | 3 | -7.54 | 148.00 | -8.22 | 148.36 | 0.2714 | 1201.0 | 951.4 | |
| 0 | 6 | 0 | 3 | -8.10 | 146.37 | -9.85 | 144.68 | 0.2942 | 642.0 | 423.9 | |
| 9 | 19 | 5 | 10 | -8.35 | 146.04 | -10.18 | 144.27 | 0.3008 | -1182.0 | -809.0 | |
| 0 | 4 | 0 | 2 | -8.03 | 145.60 | -10.62 | 142.48 | 0.3009 | -491.0 | -648.0 | |
| 0 | 10 | 0 | 5 | -8.85 | 145.17 | -11.05 | 143.01 | 0.3161 | -1066.0 | -657.2 | |
| 0 | 4 | 0 | 2 | -8.43 | 143.96 | -12.26 | 139.25 | 0.3233 | -370.0 | -163.2 | |
| 0 | 4 | 0 | 2 | -8.68 | 143.70 | -12.52 | 139.17 | 0.3291 | 316.0 | 355.7 | |
| 0 | 5 | 0 | 3 | -8.52 | 143.46 | -12.76 | 138.31 | 0.3298 | 626.0 | 421.4 | |
| 0 | 4 | 0 | 2 | -8.41 | 143.01 | -13.20 | 137.10 | 0.3334 | 862.0 | 678.4 | |
| 0 | 3 | 0 | 2 | -9.77 | 142.84 | -13.38 | 139.39 | 0.3518 | 89.0 | 168.4 | |
| 5 | 37 | 3 | 19 | -9.12 | 142.62 | -13.60 | 137.67 | 0.3463 | 1115.2 | 795.7 | |
| 9 | 17 | 5 | 9 | -8.51 | 142.27 | -13.95 | 135.73 | 0.3430 | 1208.8 | 785.2 | |
| 7 | -18 | 4 | -18 | -9.21 | 142.16 | -14.06 | 136.90 | 0.3525 | 1135.7 | 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. | |