SOHO MDI 2000-10-31 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 139 | 5 | 85 | -27.51 | 292.57 | -9.47 | 164.50 | 0.5487 | 842.6 | 707.2 | |
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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 | -25.77 | 297.24 | -4.80 | 171.44 | 0.5085 | 673.0 | 443.0 | |
| 0 | 6 | 0 | 4 | -29.18 | 295.84 | -6.19 | 170.30 | 0.5615 | 727.0 | 695.4 | |
| 0 | 4 | 0 | 2 | -29.00 | 294.97 | -7.07 | 168.90 | 0.5613 | 722.0 | 641.5 | |
| 0 | 5 | 0 | 3 | -29.19 | 294.69 | -7.35 | 168.55 | 0.5647 | 654.0 | 450.4 | |
| 0 | 4 | 0 | 2 | -26.86 | 294.76 | -7.28 | 167.67 | 0.5313 | 839.0 | 753.5 | |
| 0 | 4 | 0 | 2 | -28.28 | 294.04 | -7.99 | 167.17 | 0.5538 | 678.0 | 527.8 | |
| 0 | 12 | 0 | 7 | -27.15 | 293.16 | -8.87 | 165.24 | 0.5409 | 751.0 | 707.2 | |
| 6 | 12 | 3 | 8 | -29.63 | 292.46 | -9.58 | 165.45 | 0.5781 | 915.8 | 643.1 | |
| 0 | 9 | 0 | 6 | -26.53 | 292.65 | -9.39 | 164.07 | 0.5341 | 992.0 | 956.2 | |
| 0 | 6 | 0 | 4 | -25.77 | 292.54 | -9.50 | 163.45 | 0.5239 | 685.0 | 548.8 | |
| 0 | 16 | 0 | 9 | -26.84 | 292.40 | -9.64 | 163.87 | 0.5396 | 711.0 | 662.8 | |
| 0 | 5 | 0 | 3 | -29.04 | 291.84 | -10.19 | 164.25 | 0.5722 | 734.0 | 509.8 | |
| 3 | 18 | 2 | 11 | -26.72 | 291.67 | -10.37 | 162.64 | 0.5410 | 906.4 | 1018.5 | |
| 0 | 4 | 0 | 2 | -27.90 | 291.51 | -10.53 | 163.11 | 0.5579 | 718.0 | 648.8 | |
| 0 | 6 | 0 | 4 | -27.27 | 291.22 | -10.82 | 162.29 | 0.5505 | 1062.0 | 881.4 | |
| 0 | 2 | 0 | 1 | -28.91 | 291.00 | -11.03 | 162.96 | 0.5739 | 545.0 | 497.8 | |
| 0 | 14 | 0 | 9 | -28.00 | 291.06 | -10.98 | 162.49 | 0.5612 | 830.0 | 692.2 | |
| 0 | 3 | 0 | 2 | -27.01 | 290.10 | -11.94 | 160.43 | 0.5523 | 691.0 | 569.3 | |
| 0 | 4 | 0 | 3 | -25.45 | 289.91 | -12.13 | 159.03 | 0.5320 | 575.0 | 463.4 | |
| 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. | |