SOHO MDI 2002-08-01 12:06:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45 | 230 | 23 | 119 | -8.52 | 145.15 | -8.80 | 149.07 | 0.2923 | 193.2 | 228.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4 | 10 | 2 | 5 | -8.82 | 150.26 | -3.69 | 165.87 | 0.2618 | -1012.9 | -759.4 | |
| 0 | 5 | 0 | 2 | -8.83 | 149.74 | -4.21 | 163.97 | 0.2641 | -990.0 | -667.2 | |
| 0 | 4 | 0 | 2 | -7.33 | 148.71 | -5.24 | 158.27 | 0.2457 | 774.0 | 706.5 | |
| 0 | 10 | 0 | 5 | -7.90 | 148.34 | -5.61 | 157.78 | 0.2570 | 829.0 | 742.0 | |
| 0 | 5 | 0 | 3 | -7.09 | 148.27 | -5.68 | 156.25 | 0.2448 | 881.0 | 810.5 | |
| 0 | 12 | 0 | 6 | -7.50 | 148.15 | -5.80 | 156.46 | 0.2520 | 1100.0 | 922.4 | |
| 11 | 50 | 6 | 26 | -8.09 | 146.57 | -7.38 | 152.05 | 0.2725 | -998.7 | -599.6 | |
| 7 | 28 | 3 | 14 | -8.59 | 145.75 | -8.19 | 150.38 | 0.2864 | -1026.1 | -600.0 | |
| 0 | 3 | 0 | 2 | -9.21 | 145.21 | -8.73 | 149.87 | 0.3000 | -361.0 | -316.3 | |
| 0 | 12 | 0 | 6 | -8.20 | 144.19 | -9.76 | 145.15 | 0.2950 | -403.0 | 56.7 | |
| 0 | 11 | 0 | 6 | -8.58 | 143.85 | -10.10 | 144.96 | 0.3033 | 595.0 | 475.0 | |
| 0 | 4 | 0 | 2 | -9.00 | 143.02 | -10.92 | 143.63 | 0.3170 | 604.0 | 571.0 | |
| 0 | 5 | 0 | 3 | -8.48 | 142.80 | -11.15 | 142.03 | 0.3124 | 929.0 | 823.9 | |
| 13 | 71 | 7 | 37 | -9.30 | 142.48 | -11.46 | 142.86 | 0.3263 | 1279.3 | 1000.6 | |
| 4 | -14 | 2 | -14 | -8.57 | 142.10 | -11.85 | 140.53 | 0.3208 | 1374.0 | 999999 | |
| 6 | -14 | 3 | -14 | -9.15 | 141.96 | -11.99 | 141.32 | 0.3297 | 1144.2 | 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. | |