SOHO MDI 2000-01-26 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 133 | 751 | 93 | 518 | 4.79 | 71.95 | 42.68 | 282.96 | 0.6948 | -345.0 | -59.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 278 | 5 | 203 | 3.87 | 75.92 | 46.65 | 280.42 | 0.7401 | 741.5 | 422.7 | |
| 19 | -1 | 14 | -1 | 3.31 | 75.66 | 46.39 | 279.74 | 0.7358 | 1371.2 | 999999 | |
| -2 | -1 | -2 | -1 | 3.62 | 75.68 | 46.41 | 280.15 | 0.7367 | 999999 | 999999 | |
| 8 | -1 | 6 | -1 | 4.27 | 75.45 | 46.18 | 281.07 | 0.7355 | 1373.1 | 999999 | |
| 5 | 11 | 4 | 8 | 4.64 | 74.10 | 44.83 | 281.96 | 0.7207 | 896.8 | 742.6 | |
| 3 | 15 | 2 | 11 | 4.73 | 73.19 | 43.92 | 282.36 | 0.7101 | 914.0 | 663.7 | |
| 8 | 19 | 6 | 13 | 3.54 | 72.84 | 43.57 | 280.81 | 0.7028 | 1011.2 | 784.6 | |
| 0 | 5 | 0 | 3 | 5.00 | 72.62 | 43.36 | 282.91 | 0.7041 | 693.0 | 679.7 | |
| 2 | 9 | 1 | 6 | 5.09 | 72.10 | 42.83 | 283.20 | 0.6980 | 856.3 | 691.9 | |
| 0 | 3 | 0 | 2 | 3.17 | 71.24 | 41.98 | 280.74 | 0.6821 | -259.0 | -160.3 | |
| 0 | 4 | 0 | 3 | 5.19 | 70.76 | 41.49 | 283.81 | 0.6818 | 559.0 | 453.3 | |
| 6 | 398 | 4 | 262 | 4.04 | 70.32 | 41.05 | 282.29 | 0.6728 | -626.4 | -554.6 | |
| 0 | 4 | 0 | 3 | 7.03 | 70.16 | 40.89 | 286.65 | 0.6805 | -354.0 | -267.4 | |
| 4 | -12 | 3 | -12 | 4.39 | 69.83 | 40.56 | 282.98 | 0.6677 | -493.1 | 999999 | |
| 0 | 5 | 0 | 4 | 7.04 | 69.70 | 40.43 | 286.85 | 0.6749 | -480.0 | -353.7 | |
| 5 | -12 | 3 | -12 | 4.48 | 69.33 | 40.06 | 283.28 | 0.6616 | -861.8 | 999999 | |
| 6 | -12 | 4 | -12 | 4.65 | 69.04 | 39.77 | 283.64 | 0.6585 | -1363.3 | 999999 | |
| 33 | -12 | 22 | -12 | 5.16 | 69.03 | 39.76 | 284.39 | 0.6600 | -1545.4 | 999999 | |
| -18 | -12 | -18 | -12 | 5.70 | 68.97 | 39.70 | 285.21 | 0.6611 | 999999 | 999999 | |
| 28 | -12 | 19 | -12 | 6.72 | 68.46 | 39.19 | 286.92 | 0.6583 | -1574.8 | 999999 | |
| 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. | |