SOHO MDI 2002-08-02 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75 | 425 | 37 | 221 | -8.17 | 145.46 | 3.36 | 193.22 | 0.2556 | 148.8 | 203.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 153 | 4 | 79 | -8.02 | 149.22 | 7.12 | 207.11 | 0.2704 | -876.1 | -123.7 | |
| 3 | -1 | 2 | -1 | -7.04 | 148.76 | 6.66 | 207.29 | 0.2521 | 1051.9 | 999999 | |
| 15 | -1 | 7 | -1 | -8.05 | 148.50 | 6.39 | 204.65 | 0.2656 | -1556.5 | 999999 | |
| 0 | 10 | 0 | 5 | -6.87 | 148.32 | 6.22 | 206.01 | 0.2462 | 693.0 | 544.9 | |
| 0 | 5 | 0 | 3 | -8.00 | 147.69 | 5.59 | 201.93 | 0.2594 | -936.0 | -695.1 | |
| 11 | 54 | 6 | 28 | -8.06 | 145.81 | 3.71 | 194.88 | 0.2504 | -1405.3 | -630.7 | |
| 0 | 13 | 0 | 7 | -7.69 | 145.05 | 2.94 | 192.23 | 0.2413 | -1030.0 | -436.5 | |
| 0 | 13 | 0 | 7 | -8.46 | 144.41 | 2.31 | 189.14 | 0.2522 | 698.0 | 618.1 | |
| 0 | 3 | 0 | 2 | -7.69 | 143.89 | 1.79 | 187.50 | 0.2378 | 591.0 | 454.7 | |
| 0 | 3 | 0 | 2 | -8.38 | 143.85 | 1.75 | 186.99 | 0.2494 | 456.0 | 414.6 | |
| 0 | 9 | 0 | 5 | -7.28 | 143.57 | 1.47 | 186.35 | 0.2303 | 396.0 | 373.5 | |
| 13 | 49 | 6 | 25 | -8.01 | 143.25 | 1.15 | 184.72 | 0.2422 | 1381.2 | 913.4 | |
| 0 | 5 | 0 | 3 | -8.91 | 142.33 | 0.23 | 180.89 | 0.2566 | 539.0 | 503.3 | |
| 14 | 108 | 7 | 55 | -9.20 | 141.97 | -0.13 | 179.51 | 0.2615 | 1546.3 | 774.3 | |
| 6 | -14 | 3 | -14 | -8.70 | 141.69 | -0.41 | 178.39 | 0.2532 | 1513.8 | 999999 | |
| 5 | -14 | 2 | -14 | -8.30 | 141.50 | -0.61 | 177.54 | 0.2464 | 1269.2 | 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. | |