| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.90 | 171.76 | 22.88 | 131.28 | 20.07 | 194.26 | 46.70 | 296.13 | 0.7635 | -485.3 | -246.2 | |
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back to the solar disc SDO HMI 2011-12-02 09:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.57 | 155.62 | 7.44 | 119.93 | 20.05 | 195.22 | 47.66 | 295.72 | 0.7731 | -635.9 | -278.2 | |
| 17.68 | -1.00 | 13.56 | -1.00 | 19.83 | 194.58 | 47.02 | 295.68 | 0.7659 | -951.9 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.31 | 19.92 | 191.37 | 43.81 | 297.02 | 0.7329 | -582.0 | -534.6 | |
| 0.00 | 0.77 | 0.00 | 0.56 | 20.84 | 191.39 | 43.83 | 298.19 | 0.7367 | -601.0 | -520.7 | |
| 0.00 | 0.51 | 0.00 | 0.35 | 15.60 | 189.49 | 41.92 | 291.96 | 0.6962 | -670.0 | -593.3 | |
| 0.00 | 1.96 | 0.00 | 1.43 | 21.38 | 191.11 | 43.55 | 299.00 | 0.7359 | -675.0 | -612.7 | |
| 2.65 | 4.70 | 1.88 | 3.33 | 20.41 | 189.81 | 42.25 | 298.32 | 0.7182 | 698.4 | 473.1 | |
| 0.00 | 0.94 | 0.00 | 0.65 | 18.20 | 188.70 | 41.13 | 295.86 | 0.6968 | -707.0 | -603.5 | |
| 0.00 | 0.68 | 0.00 | 0.48 | 22.09 | 188.31 | 40.75 | 301.24 | 0.7098 | 532.0 | 399.4 | |
| 0.00 | 1.37 | 0.00 | 0.94 | 21.15 | 187.66 | 40.09 | 300.33 | 0.6983 | 387.0 | 369.2 | |
| 0.00 | 1.02 | 0.00 | 0.71 | 21.24 | 187.48 | 39.92 | 300.55 | 0.6968 | 415.0 | 450.8 | |
| 0.00 | 1.54 | 0.00 | 1.06 | 25.17 | 185.53 | 37.97 | 306.76 | 0.6974 | 582.0 | 464.3 | |
| 0.00 | 1.11 | 0.00 | 0.77 | 26.75 | 184.88 | 37.31 | 309.15 | 0.7004 | 618.0 | 502.8 | |
| 0.00 | 1.11 | 0.00 | 0.76 | 26.85 | 184.17 | 36.60 | 309.74 | 0.6942 | 585.0 | 447.6 | |
| 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. | |