SOHO MDI 2000-11-03 01:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90 | 478 | 58 | 312 | -23.10 | 305.11 | 31.19 | 226.73 | 0.6558 | -779.9 | -414.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -23.41 | 311.98 | 38.06 | 231.64 | 0.7238 | -447.0 | -376.8 | |
| 14 | 96 | 9 | 64 | -22.53 | 307.57 | 33.65 | 229.51 | 0.6753 | -1208.4 | -583.3 | |
| 13 | 216 | 9 | 143 | -23.98 | 305.98 | 32.05 | 226.48 | 0.6710 | -1154.7 | -411.3 | |
| 8 | -3 | 5 | -3 | -24.22 | 305.65 | 31.72 | 225.91 | 0.6699 | -1025.5 | 999999 | |
| 5 | -3 | 3 | -3 | -23.78 | 305.53 | 31.60 | 226.33 | 0.6653 | -1360.0 | 999999 | |
| 9 | -3 | 6 | -3 | -23.55 | 305.07 | 31.14 | 226.22 | 0.6590 | -1311.7 | 999999 | |
| 2 | 48 | 2 | 31 | -23.09 | 304.27 | 30.34 | 226.07 | 0.6475 | -911.4 | -736.7 | |
| 2 | 9 | 1 | 6 | -25.06 | 304.79 | 30.87 | 224.20 | 0.6690 | -527.4 | -442.7 | |
| 0 | 2 | 0 | 1 | -21.52 | 303.60 | 29.68 | 227.41 | 0.6280 | 116.0 | 128.6 | |
| 18 | 56 | 11 | 35 | -20.53 | 303.29 | 29.37 | 228.39 | 0.6166 | -1096.1 | -691.9 | |
| 4 | -7 | 2 | -7 | -22.76 | 303.65 | 29.73 | 225.92 | 0.6389 | -1127.4 | 999999 | |
| 3 | 17 | 2 | 11 | -25.50 | 303.43 | 29.51 | 222.49 | 0.6605 | 637.3 | 488.9 | |
| 3 | -12 | 2 | -12 | -25.53 | 303.20 | 29.27 | 222.24 | 0.6587 | 837.2 | 999999 | |
| 9 | 26 | 6 | 16 | -22.41 | 299.75 | 25.83 | 222.51 | 0.5984 | 1057.2 | 653.2 | |
| 0 | 5 | 0 | 3 | -20.87 | 293.96 | 20.03 | 217.45 | 0.5285 | 402.0 | 400.6 | |
| 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. | |