SOHO MDI 2000-01-23 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26 | 221 | 20 | 170 | -29.38 | 24.69 | -46.74 | 124.40 | 0.7702 | -768.7 | -306.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15 | 157 | 11 | 118 | -29.43 | 26.34 | -45.08 | 125.05 | 0.7558 | -1346.9 | -544.7 | |
| -1 | -1 | -1 | -1 | -29.13 | 26.33 | -45.10 | 124.67 | 0.7547 | 999999 | 999999 | |
| 4 | -1 | 3 | -1 | -29.48 | 25.87 | -45.56 | 124.93 | 0.7604 | -480.0 | 999999 | |
| 4 | -1 | 3 | -1 | -29.15 | 25.94 | -45.49 | 124.54 | 0.7584 | -841.5 | 999999 | |
| 0 | 14 | 0 | 11 | -28.97 | 25.16 | -46.27 | 124.01 | 0.7651 | -464.0 | -216.8 | |
| 0 | 6 | 0 | 4 | -28.23 | 24.88 | -46.55 | 122.99 | 0.7649 | -442.0 | -369.6 | |
| 0 | 6 | 0 | 5 | -27.56 | 23.60 | -47.82 | 121.71 | 0.7746 | 488.0 | 481.5 | |
| 0 | 6 | 0 | 5 | -30.82 | 21.30 | -50.13 | 124.88 | 0.8058 | 502.0 | 488.4 | |
| 0 | 4 | 0 | 3 | -29.83 | 20.74 | -50.69 | 123.53 | 0.8075 | 558.0 | 514.1 | |
| 0 | 4 | 0 | 3 | -30.41 | 19.68 | -51.75 | 123.89 | 0.8181 | 286.0 | 309.2 | |
| 0 | 2 | 0 | 2 | -29.90 | 19.77 | -51.66 | 123.31 | 0.8159 | 534.0 | 546.8 | |
| 0 | 6 | 0 | 5 | -29.70 | 19.34 | -52.08 | 122.95 | 0.8189 | 529.0 | 568.7 | |
| 0 | 6 | 0 | 5 | -31.04 | 17.55 | -53.88 | 124.01 | 0.8371 | 552.0 | 392.2 | |
| 0 | 1 | 0 | 1 | -29.93 | 18.44 | -52.99 | 122.97 | 0.8271 | 518.0 | 491.3 | |
| 3 | 9 | 3 | 8 | -30.07 | 17.88 | -53.54 | 122.97 | 0.8319 | 419.3 | 298.8 | |
| 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. | |