SOHO MDI 2000-02-09 08:51:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 56 | 304 | 35 | 185 | 26.56 | 199.30 | -10.30 | 16.30 | 0.5702 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 5 | 0 | 3 | 25.21 | 206.22 | -3.38 | 5.80 | 0.5300 | |
| 0 | 5 | 0 | 3 | 21.67 | 206.22 | -3.37 | 6.61 | 0.4767 | |
| 10 | 22 | 6 | 12 | 24.19 | 205.40 | -4.20 | 7.46 | 0.5162 | |
| 3 | 9 | 2 | 5 | 28.04 | 203.47 | -6.13 | 9.45 | 0.5762 | |
| 0 | 6 | 0 | 4 | 28.66 | 202.64 | -6.96 | 10.48 | 0.5869 | |
| 0 | 7 | 0 | 4 | 23.91 | 202.62 | -6.97 | 12.39 | 0.5192 | |
| 0 | 3 | 0 | 2 | 26.17 | 202.28 | -7.32 | 11.98 | 0.5528 | |
| 0 | 4 | 0 | 2 | 23.69 | 202.26 | -7.34 | 13.13 | 0.5173 | |
| 0 | 6 | 0 | 4 | 30.26 | 200.68 | -8.91 | 12.63 | 0.6142 | |
| 0 | 5 | 0 | 3 | 28.08 | 200.87 | -8.72 | 13.29 | 0.5840 | |
| 9 | 34 | 6 | 21 | 27.34 | 200.76 | -8.84 | 13.80 | 0.5742 | |
| 0 | 4 | 0 | 3 | 29.46 | 200.36 | -9.24 | 13.43 | 0.6044 | |
| 6 | 14 | 4 | 9 | 30.57 | 199.80 | -9.80 | 13.70 | 0.6210 | |
| 0 | 5 | 0 | 3 | 29.95 | 199.50 | -10.10 | 14.38 | 0.6138 | |
| 2 | 8 | 2 | 5 | 30.40 | 198.77 | -10.82 | 15.14 | 0.6223 | |
| 0 | 14 | 0 | 9 | 28.92 | 198.93 | -10.66 | 15.66 | 0.6022 | |
| 0 | 10 | 0 | 6 | 29.38 | 197.81 | -11.79 | 16.96 | 0.6125 | |
| 0 | 7 | 0 | 4 | 28.01 | 197.70 | -11.90 | 17.88 | 0.5951 | |
| 0 | 7 | 0 | 5 | 29.05 | 197.53 | -12.06 | 17.52 | 0.6094 | |
| 24 | 79 | 14 | 46 | 24.32 | 197.82 | -11.78 | 20.05 | 0.5449 | |
| 2 | 14 | 1 | 9 | 27.70 | 197.15 | -12.44 | 18.83 | 0.5934 | |
| 0 | 8 | 0 | 5 | 25.11 | 196.48 | -13.12 | 21.52 | 0.5625 | |
| 0 | 3 | 0 | 2 | 25.49 | 196.04 | -13.55 | 21.88 | 0.5697 | |
| 0 | 15 | 0 | 9 | 24.96 | 195.76 | -13.84 | 22.70 | 0.5643 | |
| 0 | 4 | 0 | 3 | 24.75 | 195.21 | -14.38 | 23.65 | 0.5646 | |
| 0 | 6 | 0 | 4 | 27.62 | 188.97 | -20.63 | 29.39 | 0.6384 | |
| 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 | |