SOHO MDI 2001-02-01 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52 | 435 | 42 | 351 | 24.97 | 114.88 | -42.74 | 51.39 | 0.7875 | 778.3 | 168.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 15 | 0 | 12 | 26.04 | 117.97 | -39.65 | 48.37 | 0.7694 | -591.0 | -366.1 | |
| 32 | 215 | 25 | 163 | 23.77 | 117.47 | -40.15 | 51.19 | 0.7596 | 1378.6 | 559.5 | |
| 7 | 52 | 6 | 41 | 25.32 | 116.31 | -41.32 | 50.22 | 0.7789 | 821.1 | 187.3 | |
| 0 | 3 | 0 | 2 | 24.59 | 116.49 | -41.13 | 50.90 | 0.7731 | 449.0 | 414.3 | |
| 0 | 3 | 0 | 3 | 24.50 | 116.02 | -41.60 | 51.30 | 0.7765 | 216.0 | 283.1 | |
| 0 | 3 | 0 | 3 | 24.43 | 114.56 | -43.06 | 52.24 | 0.7886 | 318.0 | 266.9 | |
| 0 | 7 | 0 | 6 | 26.29 | 113.54 | -44.08 | 50.82 | 0.8069 | 369.0 | 216.1 | |
| 0 | 3 | 0 | 3 | 24.04 | 114.56 | -43.07 | 52.68 | 0.7865 | 366.0 | 387.9 | |
| 0 | 3 | 0 | 2 | 23.73 | 114.51 | -43.11 | 53.04 | 0.7853 | 392.0 | 332.3 | |
| 0 | 4 | 0 | 3 | 30.18 | 111.17 | -46.45 | 48.07 | 0.8443 | -275.0 | -206.4 | |
| 0 | 4 | 0 | 4 | 26.47 | 112.91 | -44.71 | 50.98 | 0.8129 | -287.0 | -313.6 | |
| 0 | 3 | 0 | 2 | 24.57 | 113.39 | -44.23 | 52.77 | 0.7991 | 222.0 | 199.8 | |
| 0 | 9 | 0 | 8 | 27.36 | 110.83 | -46.79 | 51.16 | 0.8332 | 258.0 | 50.5 | |
| 12 | 38 | 10 | 32 | 24.45 | 112.07 | -45.55 | 53.62 | 0.8095 | -335.3 | -132.4 | |
| 1 | 19 | 1 | 16 | 25.03 | 110.87 | -46.75 | 53.62 | 0.8220 | -880.3 | -705.5 | |
| 0 | 34 | 0 | 31 | 27.09 | 109.77 | -47.85 | 52.00 | 0.8399 | -749.0 | -598.0 | |
| 0 | 3 | 0 | 3 | 29.18 | 108.16 | -49.46 | 50.62 | 0.8606 | -414.0 | -432.8 | |
| 0 | 1 | 0 | 1 | 27.92 | 108.42 | -49.20 | 51.79 | 0.8534 | -580.0 | -490.3 | |
| 0 | 16 | 0 | 16 | 28.92 | 107.44 | -50.18 | 51.23 | 0.8644 | -368.0 | -242.3 | |
| 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. | |