SDO HMI 2011-12-01 13:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.68 | 266.88 | 38.85 | 143.22 | 18.98 | 172.04 | 13.49 | 324.98 | 0.3853 | -123.3 | -170.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.20 | 0.00 | 0.65 | 18.44 | 175.34 | 16.79 | 317.83 | 0.4100 | 724.0 | 474.1 | |
| 0.77 | 141.42 | 0.41 | 76.39 | 18.29 | 174.42 | 15.87 | 319.13 | 0.3985 | -1007.7 | -433.3 | |
| 28.27 | -2.00 | 15.26 | -2.00 | 18.63 | 174.13 | 15.58 | 320.22 | 0.3995 | -1263.6 | 999999 | |
| 2.99 | -2.00 | 1.61 | -2.00 | 19.01 | 173.87 | 15.32 | 321.30 | 0.4013 | -975.0 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 17.86 | 173.38 | 14.83 | 320.23 | 0.3825 | -815.0 | -550.1 | |
| 0.00 | 1.96 | 0.00 | 1.06 | 18.70 | 173.33 | 14.78 | 321.77 | 0.3921 | -884.0 | -723.7 | |
| 2.31 | 3.25 | 1.24 | 1.75 | 18.95 | 173.28 | 14.73 | 322.26 | 0.3947 | -885.8 | -763.4 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 18.26 | 173.22 | 14.67 | 321.23 | 0.3858 | -878.0 | -737.7 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 18.54 | 172.99 | 14.44 | 322.14 | 0.3869 | -801.0 | -564.9 | |
| 0.68 | 9.39 | 0.37 | 5.05 | 18.92 | 172.93 | 14.38 | 322.88 | 0.3909 | -1205.8 | -947.1 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 18.24 | 172.32 | 13.77 | 322.90 | 0.3765 | -768.0 | -608.1 | |
| 0.00 | 5.47 | 0.00 | 2.93 | 18.73 | 172.14 | 13.59 | 324.09 | 0.3810 | -504.0 | -692.0 | |
| 0.43 | 12.98 | 0.23 | 6.95 | 19.20 | 171.57 | 13.02 | 325.97 | 0.3817 | -1000.6 | -656.6 | |
| 3.07 | -13.00 | 1.64 | -13.00 | 19.17 | 171.34 | 12.79 | 326.38 | 0.3792 | -932.1 | 999999 | |
| 0.60 | -13.00 | 0.32 | -13.00 | 19.33 | 171.35 | 12.80 | 326.59 | 0.3814 | -950.0 | 999999 | |
| 1.28 | 4.36 | 0.68 | 2.32 | 18.18 | 171.26 | 12.71 | 324.94 | 0.3656 | 904.1 | 729.4 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 17.65 | 171.07 | 12.52 | 324.47 | 0.3569 | -741.0 | -540.1 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 18.21 | 170.88 | 12.33 | 325.79 | 0.3625 | 992.0 | 787.3 | |
| 0.00 | 2.05 | 0.00 | 1.09 | 18.46 | 170.71 | 12.16 | 326.56 | 0.3642 | 889.0 | 743.9 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 19.14 | 170.73 | 12.18 | 327.59 | 0.3735 | -946.0 | -732.1 | |
| 1.96 | 14.35 | 1.05 | 7.66 | 20.36 | 169.34 | 10.79 | 332.27 | 0.3790 | 851.3 | 711.8 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 20.68 | 169.37 | 10.82 | 332.63 | 0.3836 | 646.0 | 527.8 | |
| 7.43 | 8.03 | 3.94 | 4.26 | 19.11 | 169.04 | 10.48 | 331.25 | 0.3590 | 997.3 | 852.7 | |
| 2.22 | 9.14 | 1.18 | 4.85 | 19.40 | 168.35 | 9.80 | 333.21 | 0.3578 | 1162.4 | 822.2 | |
| 1.28 | -24.00 | 0.68 | -24.00 | 19.61 | 168.30 | 9.75 | 333.61 | 0.3606 | 836.7 | 999999 | |
| 0.00 | 2.90 | 0.00 | 1.55 | 20.59 | 168.24 | 9.69 | 334.99 | 0.3742 | 813.0 | 679.1 | |
| 0.00 | 4.78 | 0.00 | 2.55 | 20.52 | 167.98 | 9.43 | 335.50 | 0.3715 | 619.0 | 682.5 | |
| 0.00 | 2.05 | 0.00 | 1.09 | 20.37 | 167.87 | 9.32 | 335.55 | 0.3685 | 1210.0 | 940.8 | |
| 0.00 | 4.10 | 0.00 | 2.18 | 20.30 | 167.61 | 9.06 | 336.08 | 0.3659 | 914.0 | 837.1 | |
| 8.45 | 10.42 | 4.46 | 5.49 | 18.87 | 167.50 | 8.95 | 334.55 | 0.3440 | 1042.2 | 823.3 | |
| 8.97 | 11.61 | 4.74 | 6.14 | 19.40 | 167.31 | 8.76 | 335.70 | 0.3505 | 1087.2 | 724.9 | |
| 1.20 | 1.54 | 0.63 | 0.81 | 19.71 | 167.20 | 8.65 | 336.35 | 0.3544 | 920.1 | 850.0 | |
| 0.77 | 3.42 | 0.41 | 1.81 | 19.87 | 166.98 | 8.43 | 337.05 | 0.3553 | 949.0 | 758.6 | |
| 0.00 | 2.22 | 0.00 | 1.17 | 19.62 | 166.30 | 7.75 | 338.44 | 0.3474 | 943.0 | 714.1 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 20.06 | 165.66 | 7.11 | 340.53 | 0.3503 | 901.0 | 730.1 | |
| 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. | |