SOHO MDI 2000-09-08 04:30:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30 | 183 | 23 | 138 | 10.38 | 341.22 | 50.27 | 277.56 | 0.7644 | -153.7 | 13.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 22 | 7 | 19 | 8.68 | 346.76 | 55.81 | 275.56 | 0.8238 | 500.6 | 395.1 | |
| 0 | 15 | 0 | 12 | 9.09 | 343.97 | 53.02 | 275.91 | 0.7953 | 698.0 | 500.1 | |
| 0 | 3 | 0 | 2 | 8.45 | 343.19 | 52.23 | 275.06 | 0.7873 | 519.0 | 463.7 | |
| 2 | 9 | 2 | 7 | 9.96 | 342.72 | 51.77 | 276.97 | 0.7817 | 688.7 | 570.1 | |
| 3 | 38 | 2 | 29 | 9.73 | 342.22 | 51.27 | 276.66 | 0.7764 | 723.7 | 620.1 | |
| 2 | 7 | 2 | 5 | 9.60 | 339.52 | 48.57 | 276.40 | 0.7463 | -276.0 | -127.3 | |
| 0 | 5 | 0 | 3 | 10.97 | 339.69 | 48.74 | 278.25 | 0.7480 | -153.0 | -209.6 | |
| 0 | 8 | 0 | 6 | 10.34 | 339.25 | 48.30 | 277.39 | 0.7430 | 277.0 | 239.6 | |
| 3 | 45 | 2 | 33 | 11.37 | 339.17 | 48.22 | 278.79 | 0.7421 | -605.5 | -666.6 | |
| 11 | -9 | 8 | -9 | 11.84 | 338.86 | 47.91 | 279.43 | 0.7385 | -982.3 | 999999 | |
| 0 | 5 | 0 | 4 | 12.43 | 338.52 | 47.57 | 280.24 | 0.7348 | -745.0 | -711.4 | |
| 0 | 5 | 0 | 3 | 11.08 | 338.04 | 47.08 | 278.41 | 0.7288 | -681.0 | -602.9 | |
| 0 | 5 | 0 | 3 | 11.74 | 337.77 | 46.82 | 279.32 | 0.7258 | -809.0 | -804.3 | |
| 0 | 4 | 0 | 3 | 11.23 | 337.25 | 46.30 | 278.63 | 0.7195 | -472.0 | -354.6 | |
| 0 | 7 | 0 | 5 | 12.20 | 337.11 | 46.16 | 279.98 | 0.7181 | -807.0 | -553.3 | |
| 0 | 5 | 0 | 4 | 11.56 | 336.68 | 45.73 | 279.10 | 0.7128 | -582.0 | -471.1 | |
| 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. | |