SOHO MDI 2000-01-24 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46 | 372 | 32 | 253 | -29.12 | 24.99 | -38.54 | 127.80 | 0.6899 | -1090.9 | -320.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40 | 298 | 27 | 200 | -28.91 | 26.51 | -37.02 | 128.32 | 0.6741 | -1362.0 | -487.0 | |
| -1 | -1 | -1 | -1 | -28.97 | 25.99 | -37.54 | 128.09 | 0.6796 | 999999 | 999999 | |
| 0 | 2 | 0 | 1 | -28.43 | 24.60 | -38.92 | 126.61 | 0.6906 | -298.0 | -216.5 | |
| 0 | 6 | 0 | 4 | -27.48 | 24.95 | -38.57 | 125.54 | 0.6821 | 14.0 | 115.6 | |
| 0 | 5 | 0 | 3 | -27.76 | 24.67 | -38.85 | 125.76 | 0.6865 | -454.0 | -246.2 | |
| 0 | 7 | 0 | 5 | -28.09 | 23.06 | -40.47 | 125.37 | 0.7046 | 783.0 | 586.7 | |
| 0 | 4 | 0 | 3 | -30.80 | 20.68 | -42.84 | 127.70 | 0.7405 | 397.0 | 438.3 | |
| 1 | 8 | 1 | 6 | -30.57 | 20.33 | -43.20 | 127.24 | 0.7427 | 735.4 | 633.0 | |
| 0 | 4 | 0 | 3 | -29.69 | 20.07 | -43.45 | 126.04 | 0.7412 | 913.0 | 678.8 | |
| 0 | 8 | 0 | 6 | -30.55 | 19.41 | -44.12 | 126.82 | 0.7512 | 418.0 | 427.3 | |
| 5 | 10 | 4 | 7 | -31.05 | 19.05 | -44.47 | 127.27 | 0.7566 | -477.8 | -246.3 | |
| 0 | 7 | 0 | 5 | -29.61 | 18.70 | -44.82 | 125.35 | 0.7537 | 707.0 | 601.4 | |
| 0 | 4 | 0 | 3 | -31.51 | 16.77 | -46.75 | 126.90 | 0.7788 | 222.0 | 210.0 | |
| 0 | 6 | 0 | 5 | -29.96 | 17.42 | -46.10 | 125.26 | 0.7669 | 202.0 | 299.2 | |
| 0 | 3 | 0 | 2 | -29.43 | 17.17 | -46.36 | 124.51 | 0.7673 | 298.0 | 400.4 | |
| 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. | |