SOHO MDI 2000-09-24 12:47:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95 | 390 | 49 | 200 | -5.74 | 83.51 | 8.34 | 212.56 | 0.2678 | -87.9 | -246.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 200 | 4 | 103 | -4.53 | 86.59 | 11.43 | 225.11 | 0.2800 | -1453.3 | -812.1 | |
| 5 | -1 | 3 | -1 | -4.88 | 86.52 | 11.35 | 224.04 | 0.2834 | -1407.9 | 999999 | |
| 6 | -1 | 3 | -1 | -5.16 | 86.28 | 11.12 | 222.77 | 0.2841 | -1443.1 | 999999 | |
| 4 | -1 | 2 | -1 | -4.68 | 86.23 | 11.07 | 223.82 | 0.2776 | -1471.5 | 999999 | |
| 5 | -1 | 3 | -1 | -5.31 | 85.92 | 10.76 | 221.48 | 0.2820 | -1645.8 | 999999 | |
| 8 | -1 | 4 | -1 | -5.86 | 85.82 | 10.65 | 219.91 | 0.2879 | -1185.3 | 999999 | |
| 7 | -1 | 3 | -1 | -5.46 | 85.57 | 10.41 | 220.17 | 0.2800 | -1505.7 | 999999 | |
| 5 | -1 | 3 | -1 | -5.89 | 85.38 | 10.21 | 218.66 | 0.2836 | -1214.5 | 999999 | |
| 0 | 6 | 0 | 3 | -5.68 | 84.98 | 9.81 | 218.00 | 0.2767 | -1033.0 | -851.4 | |
| 0 | 7 | 0 | 4 | -5.64 | 84.62 | 9.45 | 217.07 | 0.2724 | -1042.0 | -823.8 | |
| 0 | 30 | 0 | 16 | -6.67 | 84.44 | 9.27 | 214.36 | 0.2849 | -823.0 | -632.6 | |
| 0 | 4 | 0 | 2 | -5.78 | 83.83 | 8.66 | 214.37 | 0.2667 | -628.0 | -540.3 | |
| 4 | 12 | 2 | 6 | -7.23 | 82.15 | 6.98 | 206.28 | 0.2737 | 631.2 | 430.3 | |
| 0 | 5 | 0 | 3 | -7.23 | 81.67 | 6.51 | 204.72 | 0.2702 | 726.0 | 556.6 | |
| 0 | 8 | 0 | 4 | -5.89 | 80.32 | 5.15 | 201.94 | 0.2403 | 834.0 | 782.4 | |
| 0 | 5 | 0 | 2 | -6.17 | 80.04 | 4.88 | 200.47 | 0.2430 | 992.0 | 912.0 | |
| 0 | 7 | 0 | 3 | -5.17 | 79.96 | 4.79 | 201.66 | 0.2266 | 835.0 | 750.1 | |
| 0 | 13 | 0 | 7 | -5.60 | 79.76 | 4.60 | 200.19 | 0.2324 | 1058.0 | 880.5 | |
| 19 | 38 | 10 | 19 | -7.20 | 79.39 | 4.22 | 196.64 | 0.2561 | 1209.4 | 639.9 | |
| 24 | 55 | 12 | 28 | -5.67 | 78.59 | 3.42 | 195.22 | 0.2274 | 1428.5 | 774.3 | |
| 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. | |