SOHO MDI 2000-09-29 19:44:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 104 | 599 | 203 | 1147 | 9.29 | 81.20 | 75.83 | 277.86 | 0.9664 | 303.2 | 211.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 546 | 31 | 1071 | 9.29 | 84.97 | 79.60 | 278.17 | 0.9815 | -261.9 | 228.3 | |
| 12 | -1 | 25 | -1 | 7.75 | 82.81 | 77.43 | 276.41 | 0.9742 | 426.0 | 999999 | |
| 15 | -1 | 30 | -1 | 9.82 | 82.42 | 77.04 | 278.49 | 0.9720 | -28.5 | 999999 | |
| 7 | -1 | 13 | -1 | 7.71 | 80.74 | 75.36 | 276.18 | 0.9656 | 356.0 | 999999 | |
| 12 | -1 | 23 | -1 | 8.73 | 80.51 | 75.14 | 277.21 | 0.9642 | 409.4 | 999999 | |
| 4 | -1 | 7 | -1 | 9.28 | 80.53 | 75.16 | 277.78 | 0.9641 | 313.3 | 999999 | |
| 15 | -1 | 26 | -1 | 8.64 | 79.55 | 74.18 | 277.04 | 0.9597 | 807.9 | 999999 | |
| 13 | -1 | 23 | -1 | 9.65 | 80.00 | 74.63 | 278.13 | 0.9615 | 506.6 | 999999 | |
| 14 | -1 | 25 | -1 | 10.39 | 80.17 | 74.80 | 278.91 | 0.9620 | 453.4 | 999999 | |
| 0 | 6 | 0 | 9 | 11.20 | 78.25 | 72.88 | 279.63 | 0.9522 | 394.0 | 384.2 | |
| 0 | 4 | 0 | 7 | 10.91 | 77.66 | 72.29 | 279.28 | 0.9492 | 156.0 | 184.3 | |
| 0 | 22 | 0 | 31 | 11.03 | 76.21 | 70.83 | 279.32 | 0.9410 | -58.0 | 20.8 | |
| 0 | 9 | 0 | 12 | 13.78 | 75.87 | 70.50 | 282.23 | 0.9383 | -444.0 | -269.9 | |
| 0 | 12 | 0 | 17 | 12.82 | 75.12 | 69.75 | 281.18 | 0.9341 | -290.0 | -263.3 | |
| 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. | |