SOHO MDI 2000-10-27 01:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75 | 443 | 83 | 489 | -22.73 | 307.46 | -58.71 | 118.35 | 0.8969 | -461.8 | -62.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 51 | 10 | 53 | -24.06 | 310.02 | -56.15 | 120.61 | 0.8831 | -670.2 | -424.3 | |
| 6 | -1 | 6 | -1 | -23.66 | 309.60 | -56.57 | 120.04 | 0.8849 | -569.5 | 999999 | |
| 0 | 3 | 0 | 3 | -21.66 | 310.55 | -55.62 | 118.22 | 0.8725 | -351.0 | -242.7 | |
| 12 | 80 | 13 | 88 | -23.76 | 308.28 | -57.89 | 119.69 | 0.8943 | -620.6 | -119.8 | |
| 22 | 132 | 23 | 140 | -22.14 | 308.66 | -57.51 | 118.09 | 0.8876 | -775.5 | -119.4 | |
| 4 | 16 | 4 | 16 | -20.42 | 309.63 | -56.54 | 116.55 | 0.8761 | 781.7 | 543.3 | |
| 4 | -4 | 5 | -4 | -23.57 | 307.36 | -58.81 | 119.19 | 0.9000 | -124.8 | 999999 | |
| 1 | 8 | 2 | 9 | -22.32 | 306.77 | -59.40 | 117.69 | 0.9010 | -252.1 | -157.5 | |
| 4 | 33 | 4 | 36 | -20.21 | 307.90 | -58.26 | 115.77 | 0.8882 | 906.9 | 632.9 | |
| 7 | 89 | 9 | 109 | -23.94 | 304.78 | -61.39 | 118.78 | 0.9173 | -534.5 | -124.8 | |
| 0 | 2 | 0 | 2 | -20.00 | 307.32 | -58.85 | 115.37 | 0.8920 | 440.0 | 432.9 | |
| 5 | -10 | 6 | -10 | -23.53 | 304.49 | -61.68 | 118.27 | 0.9182 | -528.1 | 999999 | |
| 0 | 12 | 0 | 13 | -20.83 | 305.80 | -60.37 | 115.81 | 0.9043 | 613.0 | 561.8 | |
| 0 | 9 | 0 | 10 | -22.12 | 304.44 | -61.73 | 116.78 | 0.9157 | 177.0 | 10.6 | |
| 1 | 8 | 1 | 10 | -21.81 | 303.41 | -62.75 | 116.18 | 0.9214 | -500.0 | -471.5 | |
| 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. | |