SOHO MDI 2000-11-07 14:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59 | 438 | 38 | 286 | -12.17 | 176.11 | -38.08 | 113.27 | 0.6587 | 516.0 | 236.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -14.12 | 179.34 | -34.85 | 117.89 | 0.6294 | -444.0 | -326.5 | |
| 12 | 299 | 7 | 194 | -13.58 | 177.63 | -36.57 | 116.06 | 0.6470 | 980.6 | 540.6 | |
| 14 | -2 | 9 | -2 | -12.50 | 177.66 | -36.53 | 114.52 | 0.6411 | 1344.4 | 999999 | |
| -3 | -2 | -3 | -2 | -12.35 | 177.29 | -36.90 | 114.11 | 0.6449 | 999999 | 999999 | |
| 6 | -2 | 4 | -2 | -12.60 | 176.96 | -37.24 | 114.29 | 0.6502 | 1030.7 | 999999 | |
| 6 | -2 | 4 | -2 | -12.89 | 176.76 | -37.44 | 114.59 | 0.6540 | 882.3 | 999999 | |
| 3 | -2 | 2 | -2 | -12.37 | 176.75 | -37.45 | 113.84 | 0.6516 | 840.9 | 999999 | |
| 5 | -2 | 3 | -2 | -12.80 | 175.97 | -38.22 | 114.04 | 0.6630 | 594.8 | 999999 | |
| 0 | 20 | 0 | 13 | -11.81 | 175.79 | -38.40 | 112.54 | 0.6607 | 540.0 | 518.6 | |
| 0 | 5 | 0 | 3 | -10.73 | 175.11 | -39.08 | 110.66 | 0.6644 | -775.0 | -660.1 | |
| 0 | 6 | 0 | 4 | -10.20 | 174.38 | -39.82 | 109.58 | 0.6713 | -896.0 | -846.1 | |
| 0 | 9 | 0 | 6 | -11.04 | 174.24 | -39.95 | 110.71 | 0.6761 | -411.0 | -361.1 | |
| 0 | 3 | 0 | 2 | -9.41 | 174.49 | -39.70 | 108.49 | 0.6669 | -618.0 | -634.6 | |
| 0 | 14 | 0 | 10 | -10.53 | 174.12 | -40.07 | 109.94 | 0.6756 | -1120.0 | -870.0 | |
| 0 | 7 | 0 | 4 | -9.52 | 173.81 | -40.38 | 108.36 | 0.6756 | -721.0 | -557.7 | |
| 6 | 71 | 4 | 48 | -10.44 | 173.36 | -40.83 | 109.49 | 0.6845 | -1157.9 | -489.8 | |
| 3 | -16 | 2 | -16 | -10.62 | 173.07 | -41.12 | 109.61 | 0.6885 | -1045.9 | 999999 | |
| 4 | -16 | 3 | -16 | -10.79 | 172.57 | -41.62 | 109.65 | 0.6951 | -678.6 | 999999 | |
| 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. | |