SOHO MDI 2000-07-17 12:47:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93 | 586 | 51 | 322 | 19.22 | 289.12 | 21.72 | 306.46 | 0.4360 | 313.6 | 169.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | 25.34 | 294.18 | 26.78 | 311.58 | 0.5464 | 723.0 | 556.4 | |
| 0 | 3 | 0 | 2 | 22.03 | 292.74 | 25.34 | 307.64 | 0.5030 | 657.0 | 583.7 | |
| 22 | 351 | 12 | 194 | 19.45 | 290.81 | 23.41 | 304.94 | 0.4589 | 1451.9 | 649.0 | |
| 26 | -3 | 14 | -3 | 18.40 | 290.47 | 23.07 | 303.25 | 0.4465 | 1834.8 | 999999 | |
| -4 | -3 | -4 | -3 | 18.72 | 290.48 | 23.07 | 303.89 | 0.4490 | 999999 | 999999 | |
| 0 | 4 | 0 | 2 | 23.17 | 290.89 | 23.49 | 311.48 | 0.4910 | 355.0 | 505.8 | |
| 8 | -3 | 5 | -3 | 19.02 | 290.11 | 22.71 | 304.85 | 0.4466 | 1541.9 | 999999 | |
| 0 | 6 | 0 | 3 | 20.05 | 288.67 | 21.27 | 308.46 | 0.4370 | 570.0 | 478.8 | |
| 0 | 13 | 0 | 7 | 19.36 | 288.40 | 20.99 | 307.46 | 0.4276 | -667.0 | -432.0 | |
| 0 | 7 | 0 | 4 | 19.54 | 287.57 | 20.17 | 308.85 | 0.4190 | 47.0 | -37.7 | |
| 6 | 163 | 3 | 88 | 18.74 | 287.02 | 19.62 | 307.94 | 0.4049 | -1156.6 | -686.0 | |
| 0 | 3 | 0 | 2 | 21.33 | 286.96 | 19.56 | 313.06 | 0.4286 | -347.0 | -366.3 | |
| 31 | -11 | 17 | -11 | 18.92 | 286.51 | 19.11 | 308.99 | 0.4001 | -1798.1 | 999999 | |
| 0 | 3 | 0 | 2 | 21.05 | 286.69 | 19.29 | 312.90 | 0.4227 | -954.0 | -849.1 | |
| 0 | 13 | 0 | 7 | 21.26 | 286.36 | 18.96 | 313.76 | 0.4211 | -848.0 | -807.1 | |
| 0 | 16 | 0 | 9 | 21.86 | 285.46 | 18.05 | 316.18 | 0.4171 | -352.0 | -487.4 | |
| 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. | |