SOHO MDI 2000-10-31 04:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73 | 405 | 48 | 264 | -10.75 | 273.82 | -37.88 | 112.22 | 0.6516 | -323.3 | -58.5 | |
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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 | -11.18 | 279.40 | -32.30 | 116.07 | 0.5859 | -658.0 | -587.5 | |
| 0 | 4 | 0 | 2 | -8.48 | 279.33 | -32.37 | 111.70 | 0.5722 | 199.0 | 146.8 | |
| 36 | 176 | 22 | 108 | -9.67 | 278.32 | -33.38 | 113.01 | 0.5915 | -1502.5 | -581.7 | |
| 8 | 24 | 5 | 15 | -9.10 | 276.92 | -34.78 | 111.29 | 0.6068 | -864.7 | -651.3 | |
| 0 | 4 | 0 | 2 | -10.74 | 275.80 | -35.90 | 113.16 | 0.6289 | -495.0 | -411.9 | |
| 0 | 4 | 0 | 3 | -11.23 | 273.06 | -38.64 | 112.41 | 0.6649 | 611.0 | 488.6 | |
| 0 | 6 | 0 | 4 | -10.76 | 272.73 | -38.97 | 111.59 | 0.6669 | -462.0 | -347.9 | |
| 0 | 5 | 0 | 3 | -12.43 | 271.42 | -40.28 | 113.26 | 0.6896 | 273.0 | 411.6 | |
| 6 | 18 | 4 | 12 | -11.28 | 271.11 | -40.59 | 111.54 | 0.6884 | 938.5 | 616.5 | |
| 0 | 4 | 0 | 3 | -12.69 | 270.27 | -41.43 | 113.06 | 0.7040 | 567.0 | 543.2 | |
| 2 | 8 | 2 | 5 | -11.16 | 270.45 | -41.25 | 111.07 | 0.6956 | 751.2 | 508.6 | |
| 18 | 129 | 13 | 91 | -11.78 | 269.17 | -42.53 | 111.35 | 0.7129 | 1147.9 | 450.2 | |
| 0 | 5 | 0 | 4 | -13.16 | 268.89 | -42.81 | 113.05 | 0.7216 | 578.0 | 537.1 | |
| 0 | 4 | 0 | 3 | -12.65 | 268.67 | -43.03 | 112.28 | 0.7219 | 565.0 | 448.0 | |
| 3 | 9 | 2 | 6 | -13.07 | 268.36 | -43.34 | 112.69 | 0.7270 | 431.6 | 348.5 | |
| 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. | |