SOHO MDI 2000-07-04 15:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76 | 357 | 56 | 264 | 18.97 | 31.14 | -46.61 | 67.30 | 0.7467 | 361.3 | -25.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25 | 115 | 18 | 81 | 19.50 | 34.48 | -43.27 | 65.59 | 0.7118 | 1183.8 | 343.3 | |
| -1 | -1 | -1 | -1 | 19.25 | 34.45 | -43.30 | 65.94 | 0.7114 | 999999 | 999999 | |
| 6 | -1 | 4 | -1 | 19.94 | 33.98 | -43.77 | 65.17 | 0.7188 | 688.9 | 999999 | |
| 4 | -1 | 3 | -1 | 20.05 | 33.59 | -44.16 | 65.16 | 0.7235 | 618.5 | 999999 | |
| 0 | 4 | 0 | 3 | 19.37 | 33.24 | -44.51 | 66.19 | 0.7252 | 244.0 | 209.0 | |
| 8 | 21 | 6 | 15 | 20.45 | 32.01 | -45.75 | 65.17 | 0.7418 | 559.2 | 74.1 | |
| 2 | 7 | 1 | 5 | 19.36 | 31.99 | -45.76 | 66.60 | 0.7389 | 111.0 | 93.0 | |
| 0 | 3 | 0 | 2 | 17.91 | 31.77 | -45.98 | 68.59 | 0.7373 | -470.0 | -508.8 | |
| 2 | 9 | 2 | 6 | 18.26 | 31.41 | -46.34 | 68.22 | 0.7422 | -771.8 | -669.1 | |
| 5 | 179 | 4 | 137 | 18.79 | 30.11 | -47.64 | 67.88 | 0.7574 | -953.6 | -192.9 | |
| 13 | -10 | 10 | -10 | 18.37 | 30.02 | -47.73 | 68.45 | 0.7574 | -1006.1 | 999999 | |
| 0 | 2 | 0 | 2 | 19.22 | 29.51 | -48.24 | 67.49 | 0.7648 | 337.0 | 206.8 | |
| 11 | -10 | 8 | -10 | 18.88 | 28.43 | -49.33 | 68.20 | 0.7752 | 827.9 | 999999 | |
| 0 | 17 | 0 | 13 | 17.48 | 27.48 | -50.27 | 70.19 | 0.7819 | -445.0 | -431.1 | |
| 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. | |