SOHO MDI 2000-03-01 12:36:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 13 | 120 | 7 | 64 | 6.47 | 272.04 | -18.77 | 54.11 | 0.3968 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 11 | 0 | 6 | 6.50 | 277.68 | -13.12 | 43.98 | 0.3263 | |
| 0 | 9 | 0 | 4 | 6.17 | 276.85 | -13.95 | 46.47 | 0.3320 | |
| 0 | 5 | 0 | 3 | 5.68 | 276.23 | -14.58 | 48.84 | 0.3341 | |
| 0 | 7 | 0 | 4 | 7.54 | 274.11 | -16.69 | 48.81 | 0.3801 | |
| 0 | 5 | 0 | 2 | 6.19 | 274.04 | -16.77 | 51.72 | 0.3669 | |
| 2 | 16 | 1 | 8 | 5.24 | 272.03 | -18.77 | 56.91 | 0.3842 | |
| 0 | 7 | 0 | 4 | 5.32 | 271.05 | -19.76 | 58.10 | 0.3982 | |
| 0 | 2 | 0 | 1 | 9.79 | 270.79 | -20.02 | 49.81 | 0.4434 | |
| 11 | 20 | 6 | 11 | 4.32 | 270.50 | -20.30 | 60.97 | 0.3974 | |
| 0 | 2 | 0 | 1 | 9.87 | 270.07 | -20.73 | 50.69 | 0.4527 | |
| 0 | 6 | 0 | 3 | 5.09 | 270.11 | -20.70 | 59.81 | 0.4091 | |
| 0 | 6 | 0 | 4 | 11.42 | 269.71 | -21.10 | 48.59 | 0.4724 | |
| 0 | 4 | 0 | 2 | 5.49 | 269.80 | -21.00 | 59.34 | 0.4166 | |
| 0 | 5 | 0 | 3 | 4.21 | 269.51 | -21.29 | 62.40 | 0.4104 | |
| 0 | 5 | 0 | 3 | 10.07 | 269.22 | -21.58 | 51.48 | 0.4649 | |
| 0 | 4 | 0 | 2 | 3.58 | 269.49 | -21.32 | 63.80 | 0.4062 | |
| 0 | 2 | 0 | 1 | 12.86 | 267.92 | -22.88 | 48.67 | 0.5069 | |
| 0 | 4 | 0 | 2 | 12.80 | 267.46 | -23.35 | 49.33 | 0.5116 | |
| 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 | |