SOHO MDI 2000-09-05 16:56:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47 | 181 | 24 | 92 | 9.81 | 340.23 | 16.50 | 280.97 | 0.2888 | -635.7 | -302.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | 6.58 | 345.78 | 22.04 | 269.59 | 0.3744 | -775.0 | -658.4 | |
| 0 | 10 | 0 | 5 | 6.92 | 344.18 | 20.45 | 270.35 | 0.3483 | -817.0 | -745.9 | |
| 0 | 4 | 0 | 2 | 4.33 | 343.38 | 19.64 | 262.57 | 0.3395 | -534.0 | -521.8 | |
| 4 | 10 | 2 | 5 | 9.32 | 343.21 | 19.47 | 277.48 | 0.3333 | 879.6 | 610.6 | |
| 0 | 8 | 0 | 4 | 3.93 | 342.49 | 18.75 | 260.92 | 0.3263 | -887.0 | -757.9 | |
| 0 | 5 | 0 | 2 | 10.78 | 341.99 | 18.26 | 282.42 | 0.3165 | 683.0 | 555.9 | |
| 0 | 1 | 0 | 1 | 10.21 | 341.62 | 17.89 | 280.78 | 0.3091 | 702.0 | 628.0 | |
| 10 | 28 | 5 | 14 | 9.51 | 341.46 | 17.72 | 278.57 | 0.3050 | 1445.3 | 917.3 | |
| 0 | 4 | 0 | 2 | 8.45 | 341.41 | 17.67 | 275.09 | 0.3028 | -414.0 | -333.0 | |
| 0 | 5 | 0 | 3 | 5.25 | 341.04 | 17.30 | 264.34 | 0.2989 | -525.0 | -438.1 | |
| 6 | 78 | 3 | 40 | 10.96 | 339.21 | 15.47 | 284.79 | 0.2721 | -1013.1 | -894.1 | |
| 0 | 3 | 0 | 2 | 11.40 | 338.98 | 15.25 | 286.57 | 0.2702 | -684.0 | -611.1 | |
| 0 | 5 | 0 | 2 | 12.43 | 338.96 | 15.22 | 290.22 | 0.2745 | -591.0 | -367.5 | |
| 27 | -11 | 14 | -11 | 11.02 | 338.67 | 14.94 | 285.43 | 0.2637 | -1608.6 | 999999 | |
| 0 | 3 | 0 | 2 | 11.54 | 337.13 | 13.40 | 288.97 | 0.2411 | 629.0 | 556.7 | |
| 0 | 6 | 0 | 3 | 12.63 | 335.95 | 12.22 | 295.05 | 0.2290 | 760.0 | 587.7 | |
| 0 | 5 | 0 | 2 | 15.38 | 334.98 | 11.24 | 307.40 | 0.2377 | 774.0 | 594.8 | |
| 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. | |