| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.96 | 58.28 | 9.79 | 30.11 | -17.08 | 323.71 | 3.91 | 193.27 | 0.2859 | -315.0 | -278.5 | |
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back to the solar disc SDO HMI 2011-12-16 15:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.57 | -16.56 | 328.02 | 8.22 | 207.14 | 0.3020 | 863.0 | 693.2 | |
| 1.19 | 3.66 | 0.62 | 1.90 | -17.20 | 326.68 | 6.88 | 202.36 | 0.3023 | 998.1 | 808.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -17.61 | 325.42 | 5.62 | 198.14 | 0.3013 | 912.0 | 699.9 | |
| 3.06 | 5.95 | 1.59 | 3.09 | -17.58 | 325.07 | 5.28 | 197.13 | 0.2990 | 1032.3 | 521.5 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -17.58 | 324.82 | 5.03 | 196.37 | 0.2979 | 1016.0 | 832.1 | |
| 1.36 | 3.49 | 0.71 | 1.81 | -18.10 | 324.62 | 4.83 | 195.26 | 0.3053 | 1011.4 | 714.7 | |
| 0.00 | 2.38 | 0.00 | 1.27 | -22.13 | 324.30 | 4.51 | 191.44 | 0.3686 | -1109.0 | -841.8 | |
| 8.93 | 18.97 | 4.58 | 9.74 | -15.68 | 323.64 | 3.84 | 194.33 | 0.2619 | -1152.0 | -464.2 | |
| 0.00 | 1.96 | 0.00 | 1.01 | -16.53 | 322.82 | 3.03 | 190.74 | 0.2730 | -986.0 | -802.2 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -17.49 | 322.53 | 2.73 | 189.14 | 0.2879 | -549.0 | -567.1 | |
| 0.00 | 2.47 | 0.00 | 1.27 | -17.42 | 322.37 | 2.58 | 188.66 | 0.2865 | -757.0 | -636.8 | |
| 1.36 | 7.32 | 0.70 | 3.77 | -16.93 | 322.34 | 2.54 | 188.81 | 0.2782 | -1165.6 | -859.7 | |
| 1.19 | 6.55 | 0.62 | 3.39 | -18.16 | 321.64 | 1.84 | 185.93 | 0.2972 | -904.3 | -917.1 | |
| 1.87 | -13.00 | 0.97 | -13.00 | -18.04 | 321.45 | 1.66 | 185.37 | 0.2948 | -1034.8 | 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. | |