SDO HMI 2011-10-25 12:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.01 | 179.03 | 22.78 | 140.81 | -21.87 | 331.12 | 44.24 | 236.41 | 0.7793 | -520.5 | -324.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 0.62 | -19.61 | 338.38 | 51.50 | 242.38 | 0.8342 | 296.0 | 319.6 | |
| 0.00 | 1.13 | 0.00 | 0.99 | -19.03 | 337.97 | 51.09 | 242.87 | 0.8287 | 278.0 | 287.9 | |
| 0.96 | 5.65 | 0.83 | 4.88 | -18.85 | 337.30 | 50.42 | 242.80 | 0.8222 | 633.1 | 545.9 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -18.67 | 337.07 | 50.19 | 242.92 | 0.8196 | 537.0 | 611.7 | |
| 0.00 | 1.22 | 0.00 | 1.05 | -19.50 | 336.83 | 49.94 | 241.87 | 0.8203 | 499.0 | 458.0 | |
| 0.00 | 0.61 | 0.00 | 0.52 | -19.55 | 336.60 | 49.72 | 241.72 | 0.8185 | 289.0 | 271.6 | |
| 0.00 | 2.17 | 0.00 | 1.82 | -19.11 | 335.83 | 48.95 | 241.90 | 0.8101 | 644.0 | 597.8 | |
| 0.00 | 0.61 | 0.00 | 0.51 | -19.31 | 335.53 | 48.65 | 241.53 | 0.8081 | 532.0 | 472.1 | |
| 2.61 | 165.82 | 2.04 | 129.53 | -21.30 | 331.03 | 44.15 | 237.06 | 0.7755 | -854.9 | -397.5 | |
| 1.13 | -9.00 | 0.89 | -9.00 | -21.83 | 331.10 | 44.22 | 236.48 | 0.7788 | -412.2 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.67 | -21.05 | 330.71 | 43.83 | 237.18 | 0.7714 | -760.0 | -568.0 | |
| 3.21 | -9.00 | 2.52 | -9.00 | -22.05 | 330.87 | 43.99 | 236.11 | 0.7778 | -669.5 | 999999 | |
| 13.46 | -9.00 | 10.56 | -9.00 | -22.37 | 330.64 | 43.76 | 235.61 | 0.7773 | -772.5 | 999999 | |
| 7.64 | -9.00 | 5.94 | -9.00 | -21.98 | 330.35 | 43.47 | 235.90 | 0.7727 | -1162.8 | 999999 | |
| 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. | |