SOHO MDI 2000-09-06 07:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 212 | 22 | 117 | 10.16 | 340.70 | 25.24 | 278.72 | 0.4267 | 116.1 | 25.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | 6.86 | 346.48 | 31.03 | 271.24 | 0.5140 | -553.0 | -451.7 | |
| 0 | 6 | 0 | 3 | 7.36 | 346.01 | 30.56 | 272.19 | 0.5067 | -875.0 | -770.2 | |
| 0 | 4 | 0 | 2 | 8.94 | 344.04 | 28.59 | 275.39 | 0.4768 | 604.0 | 427.1 | |
| 0 | 3 | 0 | 2 | 3.76 | 343.33 | 27.88 | 264.32 | 0.4708 | -654.0 | -586.5 | |
| 7 | 71 | 4 | 40 | 9.39 | 342.42 | 26.97 | 276.47 | 0.4521 | 1240.6 | 994.1 | |
| 8 | -5 | 4 | -5 | 10.07 | 342.17 | 26.71 | 278.02 | 0.4488 | 1322.0 | 999999 | |
| 3 | 14 | 2 | 8 | 9.26 | 341.83 | 26.38 | 276.25 | 0.4430 | 1152.9 | 877.6 | |
| 6 | -5 | 3 | -5 | 9.85 | 341.83 | 26.38 | 277.58 | 0.4435 | 1417.8 | 999999 | |
| 0 | 9 | 0 | 5 | 9.80 | 341.30 | 25.85 | 277.55 | 0.4352 | 870.0 | 661.3 | |
| 0 | 5 | 0 | 3 | 9.59 | 340.97 | 25.52 | 277.09 | 0.4299 | 671.0 | 593.5 | |
| 0 | 4 | 0 | 2 | 11.44 | 340.16 | 24.71 | 281.62 | 0.4201 | -532.0 | -436.3 | |
| 0 | 20 | 0 | 11 | 11.40 | 339.32 | 23.87 | 281.80 | 0.4070 | -792.0 | -806.4 | |
| 0 | 8 | 0 | 5 | 10.57 | 338.73 | 23.28 | 279.91 | 0.3961 | -593.0 | -634.6 | |
| 10 | 59 | 5 | 32 | 11.29 | 338.49 | 23.03 | 281.80 | 0.3937 | -1385.6 | -1045.0 | |
| 8 | -14 | 4 | -14 | 11.02 | 338.25 | 22.79 | 281.21 | 0.3894 | -1706.7 | 999999 | |
| 0 | 5 | 0 | 2 | 13.22 | 335.03 | 19.58 | 288.78 | 0.3461 | 511.0 | 506.4 | |
| 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. | |