SOHO MDI 2000-11-02 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95 | 768 | 49 | 393 | 2.71 | 271.82 | -14.40 | 95.52 | 0.2509 | 1854.1 | 707.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29 | 687 | 15 | 351 | 2.26 | 273.01 | -13.22 | 97.86 | 0.2317 | 2300.4 | 750.4 | |
| 17 | -1 | 9 | -1 | 2.21 | 272.45 | -13.77 | 97.71 | 0.2411 | 1709.9 | 999999 | |
| 12 | -1 | 6 | -1 | 3.40 | 272.12 | -14.10 | 92.68 | 0.2446 | 1672.9 | 999999 | |
| 0 | 14 | 0 | 7 | 0.66 | 271.91 | -14.32 | 103.44 | 0.2554 | 727.0 | 598.3 | |
| 32 | -1 | 17 | -1 | 2.89 | 271.61 | -14.61 | 94.57 | 0.2539 | 1814.6 | 999999 | |
| 5 | -1 | 2 | -1 | 3.31 | 271.60 | -14.62 | 92.89 | 0.2535 | 1405.6 | 999999 | |
| 0 | 8 | 0 | 4 | 4.26 | 270.63 | -15.59 | 89.13 | 0.2694 | 466.0 | 382.2 | |
| 0 | 4 | 0 | 2 | 4.66 | 269.74 | -16.49 | 87.68 | 0.2844 | 419.0 | 370.4 | |
| 0 | 6 | 0 | 3 | 4.50 | 269.34 | -16.89 | 88.27 | 0.2910 | 865.0 | 653.4 | |
| 0 | 6 | 0 | 3 | 2.76 | 267.10 | -19.12 | 93.64 | 0.3294 | 866.0 | 752.1 | |
| 0 | 7 | 0 | 4 | 4.02 | 267.03 | -19.19 | 89.76 | 0.3294 | 232.0 | 270.8 | |
| 0 | 11 | 0 | 6 | 3.33 | 266.97 | -19.26 | 91.87 | 0.3309 | 861.0 | 698.0 | |
| 0 | 8 | 0 | 4 | 2.32 | 266.58 | -19.65 | 94.80 | 0.3387 | 741.0 | 708.3 | |
| 0 | 13 | 0 | 7 | 4.94 | 266.48 | -19.75 | 87.03 | 0.3386 | -716.0 | -673.3 | |
| 0 | 4 | 0 | 2 | 1.40 | 263.65 | -22.57 | 96.39 | 0.3878 | 377.0 | 306.1 | |
| 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. | |