SOHO MDI 2000-01-27 01:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65 | 483 | 35 | 260 | -29.05 | 23.09 | -1.79 | 176.24 | 0.4023 | -1565.1 | -437.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 2 | -27.71 | 25.92 | 1.04 | 182.44 | 0.3788 | 610.0 | 414.7 | |
| 61 | 408 | 33 | 220 | -28.87 | 23.92 | -0.96 | 177.87 | 0.3975 | -1904.0 | -622.9 | |
| 0 | 4 | 0 | 2 | -27.54 | 22.59 | -2.29 | 174.59 | 0.3774 | -407.0 | -393.8 | |
| 0 | 5 | 0 | 3 | -29.86 | 21.08 | -3.80 | 172.05 | 0.4174 | 345.0 | 440.4 | |
| 0 | 4 | 0 | 2 | -29.07 | 20.76 | -4.12 | 171.05 | 0.4056 | 870.0 | 630.8 | |
| 0 | 7 | 0 | 4 | -29.77 | 19.80 | -5.08 | 169.39 | 0.4192 | 924.0 | 703.6 | |
| 0 | 8 | 0 | 4 | -29.60 | 19.23 | -5.65 | 168.15 | 0.4183 | 1044.0 | 789.1 | |
| 4 | 9 | 2 | 5 | -31.58 | 18.52 | -6.35 | 167.88 | 0.4509 | 918.0 | 611.1 | |
| 0 | 4 | 0 | 2 | -31.83 | 17.69 | -7.19 | 166.51 | 0.4576 | 379.0 | 352.9 | |
| 0 | 6 | 0 | 3 | -30.76 | 17.10 | -7.78 | 164.74 | 0.4438 | 788.0 | 679.1 | |
| 0 | 3 | 0 | 2 | -29.78 | 16.64 | -8.24 | 163.17 | 0.4312 | 881.0 | 845.5 | |
| 0 | 3 | 0 | 1 | -30.03 | 16.35 | -8.52 | 162.81 | 0.4362 | 743.0 | 707.8 | |
| 0 | 3 | 0 | 2 | -28.06 | 16.29 | -8.58 | 161.05 | 0.4072 | 814.0 | 735.6 | |
| 0 | 5 | 0 | 3 | -30.49 | 15.77 | -9.10 | 162.10 | 0.4457 | 339.0 | 449.0 | |
| 0 | 4 | 0 | 2 | -30.69 | 15.53 | -9.35 | 161.83 | 0.4499 | 874.0 | 728.1 | |
| 0 | 5 | 0 | 3 | -30.98 | 14.73 | -10.15 | 160.66 | 0.4580 | 970.0 | 739.4 | |
| 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. | |