SOHO MDI 2000-11-03 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79 | 450 | 54 | 314 | -23.36 | 305.31 | 36.66 | 230.73 | 0.7099 | -778.2 | -325.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 85 | 6 | 61 | -22.50 | 307.75 | 39.10 | 233.43 | 0.7279 | -957.8 | -481.9 | |
| 8 | -1 | 5 | -1 | -22.57 | 307.35 | 38.69 | 233.09 | 0.7244 | -1178.0 | 999999 | |
| 0 | 6 | 0 | 4 | -22.85 | 305.95 | 37.30 | 231.83 | 0.7127 | -617.0 | -603.3 | |
| 14 | 228 | 10 | 161 | -24.11 | 306.11 | 37.45 | 230.44 | 0.7223 | -986.4 | -353.1 | |
| 0 | 13 | 0 | 9 | -22.69 | 305.38 | 36.72 | 231.62 | 0.7061 | -769.0 | -506.0 | |
| 7 | -4 | 5 | -4 | -23.87 | 305.60 | 36.95 | 230.38 | 0.7160 | -1322.2 | 999999 | |
| 11 | -4 | 8 | -4 | -24.30 | 305.64 | 36.99 | 229.90 | 0.7193 | -1061.9 | 999999 | |
| 9 | -4 | 6 | -4 | -23.50 | 305.17 | 36.51 | 230.51 | 0.7094 | -1195.5 | 999999 | |
| 7 | 28 | 4 | 19 | -20.22 | 304.15 | 35.50 | 233.82 | 0.6775 | -837.4 | -672.7 | |
| 3 | 14 | 2 | 9 | -23.21 | 304.29 | 35.64 | 230.23 | 0.6991 | -870.2 | -734.6 | |
| 3 | 17 | 2 | 12 | -25.14 | 304.77 | 36.11 | 228.31 | 0.7169 | 22.1 | -60.1 | |
| 0 | 9 | 0 | 6 | -22.91 | 303.54 | 34.88 | 230.03 | 0.6898 | -883.0 | -674.9 | |
| 0 | 7 | 0 | 5 | -25.62 | 303.62 | 34.96 | 226.91 | 0.7099 | 686.0 | 527.0 | |
| 0 | 5 | 0 | 3 | -24.85 | 302.19 | 33.53 | 226.69 | 0.6912 | 353.0 | 283.2 | |
| 0 | 4 | 0 | 3 | -25.03 | 301.02 | 32.37 | 225.55 | 0.6819 | -623.0 | -471.8 | |
| 9 | 34 | 6 | 22 | -22.41 | 299.66 | 31.01 | 227.52 | 0.6481 | 1039.8 | 595.4 | |
| 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. | |