SOHO MDI 2000-11-08 11:25:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67 | 366 | 38 | 212 | -12.30 | 176.46 | -26.18 | 121.76 | 0.5092 | 754.9 | 372.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14 | 265 | 8 | 152 | -13.55 | 177.93 | -24.71 | 125.30 | 0.5001 | 1228.2 | 657.8 | |
| -1 | -1 | -1 | -1 | -13.60 | 177.58 | -25.07 | 125.01 | 0.5048 | 999999 | 999999 | |
| 0 | 10 | 0 | 6 | -10.61 | 177.84 | -24.81 | 120.00 | 0.4782 | 311.0 | 455.5 | |
| 13 | -1 | 7 | -1 | -12.48 | 177.61 | -25.03 | 123.13 | 0.4954 | 1742.8 | 999999 | |
| 6 | -1 | 4 | -1 | -12.33 | 177.37 | -25.28 | 122.62 | 0.4973 | 1510.0 | 999999 | |
| 8 | -1 | 4 | -1 | -12.58 | 176.86 | -25.79 | 122.55 | 0.5057 | 1344.4 | 999999 | |
| 7 | -1 | 4 | -1 | -13.10 | 176.80 | -25.84 | 123.38 | 0.5105 | 941.6 | 999999 | |
| 0 | 3 | 0 | 2 | -11.94 | 176.80 | -25.85 | 121.39 | 0.5018 | 569.0 | 524.1 | |
| 3 | -1 | 2 | -1 | -12.39 | 176.71 | -25.94 | 122.06 | 0.5062 | 1198.2 | 999999 | |
| 0 | 3 | 0 | 2 | -13.64 | 176.21 | -26.44 | 123.69 | 0.5221 | 392.0 | 337.8 | |
| 0 | 4 | 0 | 2 | -10.14 | 176.18 | -26.46 | 117.61 | 0.4970 | -601.0 | -665.8 | |
| 0 | 5 | 0 | 3 | -12.34 | 175.61 | -27.03 | 120.95 | 0.5199 | 749.0 | 566.0 | |
| 0 | 12 | 0 | 7 | -10.63 | 174.24 | -28.40 | 116.86 | 0.5262 | -849.0 | -697.0 | |
| 0 | 4 | 0 | 2 | -9.65 | 174.03 | -28.62 | 114.98 | 0.5231 | -754.0 | -678.8 | |
| 0 | 3 | 0 | 2 | -8.83 | 173.74 | -28.90 | 113.32 | 0.5222 | -650.0 | -592.0 | |
| 11 | 38 | 6 | 22 | -10.73 | 173.38 | -29.26 | 116.37 | 0.5382 | -1119.2 | -568.9 | |
| 0 | 3 | 0 | 2 | -9.51 | 173.41 | -29.23 | 114.29 | 0.5305 | -455.0 | -582.2 | |
| 5 | 11 | 3 | 7 | -10.91 | 172.78 | -29.87 | 116.22 | 0.5473 | -791.3 | -520.8 | |
| 0 | 5 | 0 | 3 | -12.88 | 172.26 | -30.39 | 119.04 | 0.5662 | -309.0 | -336.9 | |
| 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. | |