SOHO MDI 2000-10-31 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50 | 468 | 33 | 309 | -10.68 | 274.14 | -38.44 | 111.86 | 0.6581 | -289.0 | -81.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 11 | 0 | 7 | -10.43 | 279.85 | -32.73 | 114.63 | 0.5872 | -528.0 | -298.9 | |
| 0 | 7 | 0 | 4 | -11.25 | 279.37 | -33.20 | 115.59 | 0.5978 | -744.0 | -566.6 | |
| 0 | 5 | 0 | 3 | -8.43 | 279.28 | -33.30 | 111.09 | 0.5844 | 329.0 | 67.4 | |
| 28 | 228 | 17 | 141 | -9.67 | 278.25 | -34.33 | 112.44 | 0.6038 | -1541.0 | -596.6 | |
| 0 | 3 | 0 | 2 | -9.92 | 277.07 | -35.51 | 112.16 | 0.6200 | -482.0 | -352.3 | |
| 0 | 5 | 0 | 3 | -8.14 | 275.24 | -37.34 | 108.54 | 0.6356 | -563.0 | -502.6 | |
| 0 | 6 | 0 | 4 | -10.57 | 273.38 | -39.20 | 111.21 | 0.6688 | 570.0 | 575.6 | |
| 0 | 2 | 0 | 2 | -11.18 | 273.18 | -39.40 | 111.97 | 0.6738 | 516.0 | 392.3 | |
| 0 | 10 | 0 | 7 | -10.92 | 272.66 | -39.92 | 111.37 | 0.6790 | -376.0 | 157.9 | |
| 0 | 3 | 0 | 2 | -12.31 | 271.43 | -41.15 | 112.68 | 0.6992 | 670.0 | 551.7 | |
| 0 | 10 | 0 | 7 | -11.32 | 271.13 | -41.44 | 111.21 | 0.6985 | 934.0 | 720.5 | |
| 0 | 4 | 0 | 3 | -12.73 | 270.23 | -42.35 | 112.69 | 0.7146 | 601.0 | 515.5 | |
| 2 | 9 | 1 | 6 | -11.16 | 270.48 | -42.10 | 110.70 | 0.7055 | 721.0 | 584.6 | |
| 0 | 4 | 0 | 3 | -13.12 | 268.95 | -43.63 | 112.64 | 0.7304 | 559.0 | 441.8 | |
| 18 | 154 | 13 | 110 | -11.78 | 269.18 | -43.40 | 110.98 | 0.7228 | 1081.3 | 423.5 | |
| 2 | 7 | 2 | 5 | -13.03 | 268.36 | -44.22 | 112.27 | 0.7365 | 446.5 | 389.3 | |
| 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. | |