SOHO MDI 2000-11-01 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3 | 105 | 2 | 62 | -27.26 | 292.68 | -3.21 | 174.53 | 0.5275 | 903.6 | 738.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -28.60 | 295.25 | -0.63 | 178.97 | 0.5447 | 756.0 | 686.5 | |
| 0 | 4 | 0 | 3 | -26.96 | 294.92 | -0.97 | 178.33 | 0.5205 | 673.0 | 510.0 | |
| 0 | 5 | 0 | 3 | -29.15 | 294.81 | -1.08 | 178.29 | 0.5529 | 457.0 | 454.0 | |
| 0 | 4 | 0 | 2 | -28.00 | 294.82 | -1.07 | 178.24 | 0.5361 | 794.0 | 669.3 | |
| 0 | 3 | 0 | 2 | -29.52 | 294.14 | -1.75 | 177.27 | 0.5587 | 411.0 | 529.6 | |
| 0 | 9 | 0 | 5 | -26.92 | 293.23 | -2.66 | 175.44 | 0.5213 | 914.0 | 839.1 | |
| 0 | 8 | 0 | 5 | -27.05 | 292.97 | -2.92 | 175.01 | 0.5236 | 900.0 | 678.9 | |
| 0 | 7 | 0 | 4 | -25.31 | 292.76 | -3.13 | 174.28 | 0.4978 | 689.0 | 726.7 | |
| 0 | 11 | 0 | 7 | -26.56 | 292.59 | -3.29 | 174.27 | 0.5168 | 1333.0 | 1049.4 | |
| 0 | 5 | 0 | 3 | -29.67 | 292.50 | -3.39 | 174.74 | 0.5625 | 704.0 | 573.7 | |
| 3 | 18 | 2 | 10 | -26.61 | 292.16 | -3.73 | 173.54 | 0.5182 | 1139.0 | 950.8 | |
| 0 | 6 | 0 | 3 | -26.70 | 291.51 | -4.38 | 172.45 | 0.5208 | 873.0 | 704.8 | |
| 0 | 8 | 0 | 4 | -27.61 | 291.39 | -4.50 | 172.49 | 0.5343 | 798.0 | 663.9 | |
| 0 | 6 | 0 | 4 | -27.16 | 290.80 | -5.09 | 171.38 | 0.5290 | 459.0 | 486.4 | |
| 0 | 3 | 0 | 2 | -27.93 | 290.15 | -5.74 | 170.58 | 0.5418 | 743.0 | 692.8 | |
| 0 | 3 | 0 | 2 | -26.98 | 290.07 | -5.82 | 170.11 | 0.5282 | 695.0 | 638.6 | |
| 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. | |