SOHO MDI 2002-08-02 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73 | 405 | 38 | 206 | -8.23 | 145.48 | 4.26 | 196.41 | 0.2609 | -27.2 | 227.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 8 | 0 | 4 | -7.30 | 149.93 | 8.71 | 213.48 | 0.2736 | 671.0 | 646.1 | |
| 0 | 5 | 0 | 2 | -6.73 | 149.68 | 8.46 | 213.89 | 0.2632 | 708.0 | 442.9 | |
| 7 | 107 | 4 | 55 | -8.15 | 149.39 | 8.16 | 210.18 | 0.2808 | -1091.9 | -405.5 | |
| 0 | 10 | 0 | 5 | -7.33 | 149.25 | 8.03 | 211.29 | 0.2678 | 690.0 | 725.5 | |
| 4 | 13 | 2 | 7 | -7.04 | 148.88 | 7.66 | 210.67 | 0.2605 | 989.6 | 646.3 | |
| 13 | -3 | 7 | -3 | -8.10 | 148.70 | 7.48 | 208.13 | 0.2745 | -1515.8 | 999999 | |
| 0 | 5 | 0 | 3 | -6.87 | 148.36 | 7.14 | 209.24 | 0.2536 | 886.0 | 592.8 | |
| 0 | 5 | 0 | 2 | -7.56 | 148.25 | 7.03 | 207.59 | 0.2629 | -790.0 | -641.9 | |
| 0 | 5 | 0 | 3 | -7.97 | 147.89 | 6.67 | 205.71 | 0.2663 | -953.0 | -659.2 | |
| 0 | 4 | 0 | 2 | -8.72 | 146.10 | 4.87 | 198.43 | 0.2668 | -720.0 | -587.7 | |
| 15 | 40 | 8 | 20 | -8.07 | 145.93 | 4.71 | 198.63 | 0.2554 | -1428.5 | -717.5 | |
| 2 | 8 | 1 | 4 | -7.65 | 145.24 | 4.02 | 196.54 | 0.2453 | -902.9 | -639.0 | |
| 0 | 15 | 0 | 7 | -8.47 | 144.57 | 3.35 | 193.12 | 0.2557 | 644.0 | 599.0 | |
| 0 | 5 | 0 | 2 | -7.20 | 143.60 | 2.38 | 190.31 | 0.2312 | 659.0 | 443.2 | |
| 13 | 67 | 6 | 34 | -7.97 | 143.17 | 1.94 | 187.99 | 0.2430 | 1520.4 | 815.9 | |
| 0 | 3 | 0 | 2 | -9.40 | 142.49 | 1.27 | 184.74 | 0.2658 | 792.0 | 690.5 | |
| 0 | 4 | 0 | 2 | -7.84 | 142.25 | 1.03 | 184.27 | 0.2393 | -241.0 | -108.4 | |
| 14 | 97 | 7 | 50 | -9.19 | 141.93 | 0.71 | 182.69 | 0.2618 | 1467.2 | 843.5 | |
| 0 | 4 | 0 | 2 | -10.42 | 141.77 | 0.55 | 181.93 | 0.2824 | 541.0 | 424.4 | |
| 5 | -18 | 3 | -18 | -8.66 | 141.61 | 0.39 | 181.53 | 0.2525 | 1420.9 | 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. | |