SOHO MDI 2000-01-27 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57 | 523 | 31 | 285 | -29.27 | 22.17 | 7.83 | 196.51 | 0.4225 | -1607.8 | -416.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 8 | 0 | 4 | -26.39 | 23.48 | 9.14 | 201.82 | 0.3846 | 791.0 | 470.1 | |
| 57 | 416 | 31 | 227 | -28.96 | 23.56 | 9.23 | 199.47 | 0.4229 | -1880.0 | -692.4 | |
| 0 | 3 | 0 | 2 | -27.39 | 22.86 | 8.52 | 199.50 | 0.3959 | -574.0 | -490.0 | |
| -2 | -2 | -2 | -2 | -29.17 | 22.92 | 8.58 | 198.03 | 0.4228 | 999999 | 999999 | |
| 0 | 4 | 0 | 2 | -29.32 | 21.33 | 7.00 | 194.79 | 0.4179 | -453.0 | -469.4 | |
| 0 | 5 | 0 | 3 | -29.50 | 20.50 | 6.17 | 193.00 | 0.4175 | 816.0 | 616.6 | |
| 0 | 12 | 0 | 6 | -30.00 | 20.31 | 5.98 | 192.31 | 0.4246 | 755.0 | 660.2 | |
| 0 | 3 | 0 | 2 | -30.05 | 19.96 | 5.62 | 191.59 | 0.4241 | 695.0 | 567.2 | |
| 0 | 4 | 0 | 2 | -29.51 | 19.31 | 4.97 | 190.55 | 0.4138 | 1005.0 | 869.1 | |
| 0 | 5 | 0 | 3 | -31.50 | 18.42 | 4.09 | 187.92 | 0.4425 | 836.0 | 711.5 | |
| 0 | 5 | 0 | 3 | -30.53 | 17.13 | 2.80 | 185.70 | 0.4250 | 1091.0 | 923.7 | |
| 0 | 4 | 0 | 2 | -30.87 | 16.96 | 2.63 | 185.27 | 0.4301 | 796.0 | 673.3 | |
| 0 | 14 | 0 | 7 | -30.11 | 16.85 | 2.52 | 185.24 | 0.4179 | 1087.0 | 898.5 | |
| 0 | 5 | 0 | 3 | -30.62 | 16.51 | 2.17 | 184.42 | 0.4255 | 842.0 | 772.3 | |
| 0 | 4 | 0 | 2 | -30.91 | 16.11 | 1.78 | 183.57 | 0.4298 | 818.0 | 758.0 | |
| 0 | 12 | 0 | 7 | -31.00 | 15.62 | 1.29 | 182.58 | 0.4307 | 1085.0 | 741.8 | |
| 0 | 3 | 0 | 1 | -27.69 | 15.37 | 1.03 | 182.43 | 0.3776 | 646.0 | 533.3 | |
| 0 | 5 | 0 | 3 | -30.96 | 15.18 | 0.84 | 181.69 | 0.4298 | 1150.0 | 930.2 | |
| 0 | 6 | 0 | 3 | -31.30 | 14.82 | 0.49 | 180.96 | 0.4350 | 804.0 | 753.7 | |
| 0 | 5 | 0 | 3 | -30.83 | 14.28 | -0.05 | 179.90 | 0.4276 | 1053.0 | 874.5 | |
| 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. | |