SOHO MDI 2001-01-24 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 53 | 364 | 27 | 192 | -15.04 | 252.34 | -16.84 | 121.63 | 0.3298 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 8 | 0 | 4 | -13.11 | 253.91 | -15.27 | 118.16 | 0.2923 | |
| 8 | 282 | 4 | 147 | -14.54 | 253.73 | -15.45 | 122.14 | 0.3060 | |
| 23 | -2 | 12 | -2 | -14.91 | 253.25 | -15.93 | 122.46 | 0.3158 | |
| 14 | -2 | 7 | -2 | -15.21 | 252.77 | -16.41 | 122.56 | 0.3249 | |
| 0 | 7 | 0 | 4 | -19.03 | 251.83 | -17.36 | 130.35 | 0.3717 | |
| 0 | 3 | 0 | 2 | -16.87 | 251.96 | -17.22 | 125.60 | 0.3500 | |
| 8 | 15 | 4 | 8 | -14.68 | 251.90 | -17.28 | 119.93 | 0.3330 | |
| 0 | 4 | 0 | 2 | -17.69 | 250.44 | -18.74 | 125.40 | 0.3772 | |
| 0 | 8 | 0 | 4 | -15.83 | 248.48 | -20.71 | 118.77 | 0.3898 | |
| 0 | 3 | 0 | 2 | -15.27 | 248.15 | -21.03 | 117.14 | 0.3907 | |
| 0 | 5 | 0 | 3 | -14.76 | 248.08 | -21.10 | 115.86 | 0.3886 | |
| 0 | 7 | 0 | 4 | -14.86 | 247.60 | -21.58 | 115.66 | 0.3962 | |
| 0 | 7 | 0 | 4 | -14.32 | 247.53 | -21.65 | 114.30 | 0.3940 | |
| 0 | 4 | 0 | 2 | -17.07 | 247.17 | -22.01 | 120.25 | 0.4165 | |
| 0 | 3 | 0 | 1 | -16.94 | 246.80 | -22.38 | 119.59 | 0.4207 | |
| 0 | 3 | 0 | 2 | -14.13 | 246.74 | -22.45 | 113.21 | 0.4046 | |
| 0 | 5 | 0 | 3 | -13.92 | 246.07 | -23.11 | 112.19 | 0.4132 | |
| 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 | |