SOHO MDI 2000-10-05 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69 | 503 | 46 | 329 | -21.76 | 315.80 | 30.15 | 225.30 | 0.6567 | -806.4 | -235.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20 | 276 | 13 | 187 | -21.66 | 318.72 | 33.07 | 228.17 | 0.6829 | -1261.4 | -465.1 | |
| 11 | -1 | 8 | -1 | -22.26 | 318.63 | 32.98 | 227.39 | 0.6868 | -786.4 | 999999 | |
| 12 | -1 | 8 | -1 | -21.70 | 317.99 | 32.33 | 227.51 | 0.6763 | -1274.2 | 999999 | |
| 0 | 7 | 0 | 5 | -21.11 | 317.06 | 31.40 | 227.39 | 0.6627 | -454.0 | -332.2 | |
| 14 | 50 | 9 | 32 | -20.92 | 316.04 | 30.39 | 226.72 | 0.6514 | -896.1 | -437.2 | |
| 6 | 50 | 4 | 31 | -21.34 | 312.66 | 27.01 | 222.94 | 0.6231 | -812.2 | -185.9 | |
| 0 | 5 | 0 | 3 | -21.21 | 311.98 | 26.33 | 222.38 | 0.6156 | -786.0 | -529.6 | |
| 0 | 13 | 0 | 8 | -23.68 | 311.78 | 26.13 | 219.40 | 0.6378 | -318.0 | -83.7 | |
| 0 | 11 | 0 | 7 | -21.55 | 310.98 | 25.33 | 220.91 | 0.6098 | -783.0 | -567.8 | |
| 0 | 6 | 0 | 4 | -21.09 | 310.48 | 24.83 | 220.89 | 0.6007 | 860.0 | 707.8 | |
| 0 | 8 | 0 | 5 | -24.58 | 311.08 | 25.43 | 217.69 | 0.6409 | 971.0 | 659.2 | |
| 0 | 8 | 0 | 5 | -21.11 | 310.02 | 24.37 | 220.35 | 0.5968 | 847.0 | 806.4 | |
| 0 | 13 | 0 | 8 | -22.22 | 310.18 | 24.53 | 219.27 | 0.6094 | 804.0 | 596.4 | |
| 0 | 7 | 0 | 4 | -20.15 | 309.81 | 24.16 | 221.25 | 0.5850 | 752.0 | 578.0 | |
| 0 | 5 | 0 | 3 | -21.09 | 309.52 | 23.87 | 219.80 | 0.5919 | 987.0 | 898.2 | |
| 6 | 17 | 4 | 11 | -22.09 | 309.47 | 23.81 | 218.60 | 0.6019 | 996.4 | 671.6 | |
| 0 | 4 | 0 | 3 | -19.94 | 309.06 | 23.40 | 220.62 | 0.5758 | 732.0 | 598.4 | |
| 0 | 12 | 0 | 7 | -23.56 | 309.56 | 23.90 | 217.10 | 0.6180 | 682.0 | 516.0 | |
| 0 | 11 | 0 | 6 | -22.15 | 307.79 | 22.14 | 216.56 | 0.5882 | 796.0 | 738.9 | |
| 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. | |