SOHO MDI 2000-11-09 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61 | 389 | 31 | 200 | -12.63 | 176.72 | -6.73 | 157.47 | 0.3002 | 1449.2 | 540.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | -11.75 | 178.36 | -5.09 | 161.52 | 0.2754 | 597.0 | 459.0 | |
| 14 | 324 | 7 | 168 | -13.31 | 177.81 | -5.64 | 161.53 | 0.3031 | 1354.4 | 699.1 | |
| 22 | -2 | 11 | -2 | -12.32 | 177.48 | -5.97 | 159.33 | 0.2893 | 1921.9 | 999999 | |
| 6 | -2 | 3 | -2 | -13.00 | 177.34 | -6.11 | 159.74 | 0.3007 | 1139.6 | 999999 | |
| 11 | -2 | 6 | -2 | -12.60 | 176.88 | -6.57 | 157.83 | 0.2973 | 1659.2 | 999999 | |
| 8 | -2 | 4 | -2 | -13.00 | 176.83 | -6.62 | 158.19 | 0.3038 | 1260.8 | 999999 | |
| 0 | 3 | 0 | 1 | -19.33 | 175.91 | -7.54 | 162.17 | 0.4060 | -634.0 | -516.5 | |
| 0 | 9 | 0 | 5 | -13.57 | 175.38 | -8.07 | 154.81 | 0.3222 | 766.0 | 611.9 | |
| 0 | 4 | 0 | 2 | -14.91 | 174.08 | -9.37 | 153.27 | 0.3513 | -674.0 | -569.6 | |
| 0 | 6 | 0 | 3 | -8.98 | 174.21 | -9.24 | 143.25 | 0.2663 | -817.0 | -654.9 | |
| 0 | 6 | 0 | 3 | -11.67 | 173.45 | -10.00 | 146.62 | 0.3104 | -398.0 | -427.1 | |
| 0 | 4 | 0 | 2 | -9.34 | 173.01 | -10.44 | 140.71 | 0.2835 | -770.0 | -745.1 | |
| 0 | 10 | 0 | 5 | -12.65 | 171.77 | -11.68 | 144.22 | 0.3394 | -735.0 | -595.7 | |
| 0 | 5 | 0 | 2 | -11.81 | 171.65 | -11.80 | 142.41 | 0.3297 | -545.0 | -470.7 | |
| 0 | 6 | 0 | 3 | -10.31 | 171.19 | -12.26 | 138.31 | 0.3155 | -634.0 | -510.4 | |
| 0 | 6 | 0 | 3 | -10.96 | 169.92 | -13.53 | 136.88 | 0.3376 | -790.0 | -627.1 | |
| 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. | |