SOHO MDI 2000-07-15 17:37:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58 | 327 | 31 | 174 | 3.05 | 270.29 | -20.93 | 93.24 | 0.3585 | -916.6 | -393.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 21 | 4 | 11 | 2.64 | 276.98 | -14.24 | 96.87 | 0.2486 | 1212.6 | 743.2 | |
| 0 | 5 | 0 | 3 | 3.74 | 276.22 | -14.99 | 92.28 | 0.2595 | 825.0 | 721.9 | |
| 0 | 7 | 0 | 4 | 3.40 | 275.24 | -15.97 | 93.30 | 0.2764 | 1047.0 | 1032.9 | |
| 3 | 25 | 2 | 13 | 3.08 | 274.92 | -16.30 | 94.36 | 0.2823 | 1152.0 | 1027.7 | |
| 0 | 3 | 0 | 2 | 3.84 | 272.24 | -18.97 | 91.21 | 0.3259 | -791.0 | -789.2 | |
| 0 | 8 | 0 | 4 | 3.86 | 271.53 | -19.69 | 91.05 | 0.3377 | -1063.0 | -794.0 | |
| 0 | 4 | 0 | 2 | 3.50 | 271.28 | -19.93 | 92.08 | 0.3420 | -711.0 | -580.5 | |
| 9 | 217 | 5 | 116 | 3.01 | 269.17 | -22.05 | 93.05 | 0.3770 | -1825.9 | -659.6 | |
| 0 | 6 | 0 | 3 | 1.78 | 269.19 | -22.03 | 96.30 | 0.3787 | -772.0 | -708.3 | |
| 7 | -8 | 4 | -8 | 3.44 | 269.12 | -22.10 | 91.89 | 0.3773 | -1725.7 | 999999 | |
| 6 | -8 | 3 | -8 | 3.71 | 268.94 | -22.28 | 91.14 | 0.3800 | -1320.2 | 999999 | |
| 14 | -8 | 7 | -8 | 3.08 | 268.82 | -22.39 | 92.80 | 0.3824 | -1387.8 | 999999 | |
| 11 | 30 | 6 | 16 | 1.68 | 268.55 | -22.67 | 96.33 | 0.3892 | -1135.0 | -738.8 | |
| 0 | 1 | 0 | 0 | 1.47 | 268.16 | -23.05 | 96.73 | 0.3958 | -215.0 | -216.7 | |
| 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. | |