SDO HMI 2011-12-04 21:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.35 | 293.36 | 38.90 | 155.81 | 19.48 | 123.76 | 9.17 | 335.68 | 0.3622 | 319.2 | 195.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.39 | 0.00 | 1.41 | 19.59 | 141.91 | 27.31 | 307.25 | 0.5452 | 629.0 | 404.0 | |
| 0.00 | 1.79 | 0.00 | 1.02 | 19.76 | 136.89 | 22.29 | 312.86 | 0.4890 | 809.0 | 733.3 | |
| 1.54 | 1.71 | 0.83 | 0.92 | 20.44 | 127.94 | 13.34 | 327.70 | 0.4063 | -590.1 | -535.0 | |
| 2.47 | 10.66 | 1.34 | 5.76 | 20.22 | 127.85 | 13.25 | 327.55 | 0.4027 | -830.9 | -686.4 | |
| 0.00 | 3.58 | 0.00 | 1.93 | 19.94 | 127.76 | 13.17 | 327.32 | 0.3982 | -838.0 | -745.0 | |
| 3.58 | 11.35 | 1.93 | 6.11 | 20.00 | 127.41 | 12.82 | 328.09 | 0.3961 | -969.0 | -830.1 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 19.10 | 126.76 | 12.17 | 328.09 | 0.3784 | -955.0 | -778.1 | |
| 1.71 | 20.30 | 0.92 | 10.88 | 19.69 | 126.78 | 12.18 | 328.92 | 0.3865 | -993.7 | -838.7 | |
| 1.02 | -8.00 | 0.55 | -8.00 | 19.63 | 126.61 | 12.01 | 329.18 | 0.3843 | -1158.8 | 999999 | |
| 0.00 | 2.56 | 0.00 | 1.38 | 20.51 | 126.52 | 11.92 | 330.57 | 0.3955 | -936.0 | -734.1 | |
| 3.67 | -8.00 | 1.97 | -8.00 | 19.69 | 126.43 | 11.83 | 329.65 | 0.3836 | -982.6 | 999999 | |
| 0.00 | 6.91 | 0.00 | 3.74 | 21.07 | 126.44 | 11.84 | 331.48 | 0.4027 | -1101.0 | -789.9 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 20.79 | 126.38 | 11.78 | 331.23 | 0.3984 | -931.0 | -712.4 | |
| 2.13 | 4.35 | 1.14 | 2.33 | 19.97 | 126.22 | 11.62 | 330.47 | 0.3858 | -1043.6 | -868.0 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 20.26 | 126.18 | 11.58 | 330.94 | 0.3894 | -831.0 | -669.3 | |
| 2.73 | 3.41 | 1.46 | 1.82 | 19.66 | 125.59 | 10.99 | 331.38 | 0.3765 | -937.8 | -764.2 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 20.04 | 125.62 | 11.02 | 331.83 | 0.3820 | -837.0 | -722.5 | |
| 0.00 | 2.05 | 0.00 | 1.09 | 18.85 | 125.41 | 10.81 | 330.65 | 0.3638 | -858.0 | -779.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 19.07 | 125.33 | 10.73 | 331.14 | 0.3662 | -716.0 | -525.7 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 22.06 | 125.19 | 10.59 | 335.18 | 0.4075 | -797.0 | -612.2 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 21.45 | 124.66 | 10.06 | 335.61 | 0.3953 | -876.0 | -607.3 | |
| 0.00 | 5.29 | 0.00 | 2.81 | 19.60 | 123.96 | 9.36 | 334.96 | 0.3637 | 890.0 | 637.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 18.94 | 123.73 | 9.14 | 334.67 | 0.3525 | 864.0 | 720.3 | |
| 1.19 | 1.88 | 0.64 | 1.01 | 21.58 | 123.70 | 9.10 | 337.80 | 0.3911 | 741.9 | 667.2 | |
| 1.19 | 196.72 | 0.63 | 103.75 | 19.57 | 122.88 | 8.28 | 337.49 | 0.3561 | 924.4 | 518.0 | |
| 1.54 | -25.00 | 0.81 | -25.00 | 19.79 | 122.83 | 8.23 | 337.86 | 0.3591 | 867.8 | 999999 | |
| 4.35 | -25.00 | 2.30 | -25.00 | 19.66 | 122.63 | 8.04 | 338.20 | 0.3560 | 854.9 | 999999 | |
| 2.64 | -25.00 | 1.40 | -25.00 | 19.19 | 122.58 | 7.98 | 337.80 | 0.3486 | 841.5 | 999999 | |
| 1.36 | -25.00 | 0.72 | -25.00 | 19.48 | 122.53 | 7.93 | 338.25 | 0.3525 | 955.7 | 999999 | |
| 27.04 | -25.00 | 14.24 | -25.00 | 18.79 | 122.28 | 7.68 | 338.10 | 0.3406 | 1276.1 | 999999 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 19.76 | 122.32 | 7.72 | 339.07 | 0.3556 | 298.0 | 307.7 | |
| 12.97 | -25.00 | 6.85 | -25.00 | 19.38 | 122.18 | 7.58 | 339.02 | 0.3490 | 935.1 | 999999 | |
| 0.00 | 2.13 | 0.00 | 1.14 | 21.96 | 121.92 | 7.32 | 342.13 | 0.3870 | 865.0 | 668.7 | |
| 0.00 | 2.22 | 0.00 | 1.19 | 21.74 | 121.91 | 7.31 | 341.96 | 0.3836 | 664.0 | 659.8 | |
| 2.22 | -25.00 | 1.17 | -25.00 | 19.76 | 121.75 | 7.15 | 340.48 | 0.3523 | 799.4 | 999999 | |
| 0.00 | 3.24 | 0.00 | 1.73 | 20.95 | 121.43 | 6.83 | 342.41 | 0.3690 | 970.0 | 738.7 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 20.67 | 121.41 | 6.81 | 342.19 | 0.3646 | 904.0 | 795.1 | |
| 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. | |