SOHO MDI 2000-01-27 10:30:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 96 | 610 | 78 | 505 | 4.74 | 72.26 | 52.28 | 280.29 | 0.8021 | -140.7 | -77.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 199 | 15 | 181 | 3.76 | 76.60 | 56.62 | 278.11 | 0.8438 | 644.5 | 233.3 | |
| 0 | 3 | 0 | 3 | 2.66 | 75.95 | 55.97 | 276.93 | 0.8361 | 450.0 | 462.9 | |
| 11 | -1 | 10 | -1 | 4.17 | 76.02 | 56.04 | 278.72 | 0.8390 | 889.8 | 999999 | |
| 8 | 31 | 7 | 27 | 4.21 | 74.53 | 54.55 | 279.06 | 0.8249 | 847.8 | 523.7 | |
| 4 | 20 | 3 | 17 | 3.52 | 74.13 | 54.15 | 278.30 | 0.8198 | 554.7 | 435.0 | |
| 0 | 7 | 0 | 6 | 3.91 | 73.70 | 53.72 | 278.86 | 0.8163 | 922.0 | 749.5 | |
| 0 | 9 | 0 | 8 | 4.69 | 72.81 | 52.83 | 280.01 | 0.8088 | 871.0 | 666.2 | |
| 6 | 17 | 5 | 14 | 5.22 | 72.18 | 52.20 | 280.81 | 0.8033 | 736.4 | 579.5 | |
| 0 | 13 | 0 | 10 | 3.75 | 70.18 | 50.20 | 279.44 | 0.7795 | -546.0 | -492.5 | |
| 9 | 161 | 7 | 124 | 4.48 | 69.58 | 49.60 | 280.51 | 0.7745 | -743.4 | -466.5 | |
| 0 | 9 | 0 | 7 | 3.74 | 69.05 | 49.07 | 279.69 | 0.7671 | -429.0 | -488.4 | |
| 4 | -10 | 3 | -10 | 4.40 | 68.98 | 49.00 | 280.55 | 0.7678 | -1173.8 | 999999 | |
| 17 | -10 | 13 | -10 | 4.97 | 68.92 | 48.94 | 281.31 | 0.7684 | -1159.1 | 999999 | |
| 0 | 5 | 0 | 4 | 5.97 | 68.74 | 48.76 | 282.63 | 0.7687 | -575.0 | -410.0 | |
| 14 | 136 | 10 | 104 | 6.76 | 68.31 | 48.33 | 283.76 | 0.7661 | -1065.2 | -523.1 | |
| 7 | -15 | 5 | -15 | 6.44 | 68.15 | 48.17 | 283.39 | 0.7635 | -1336.9 | 999999 | |
| 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. | |