SDO HMI 2011-06-04 06:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.48 | 268.76 | 25.20 | 139.89 | 17.39 | 19.68 | -0.48 | 1.14 | 0.3083 | -514.7 | -249.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 1.01 | 20.71 | 25.26 | 5.10 | 346.95 | 0.3698 | -773.0 | -617.1 | |
| 0.00 | 2.71 | 0.00 | 1.44 | 20.25 | 24.01 | 3.85 | 349.84 | 0.3584 | -893.0 | -728.2 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 22.38 | 21.23 | 1.07 | 357.43 | 0.3878 | -629.0 | -501.4 | |
| 6.78 | 195.29 | 3.53 | 101.23 | 17.23 | 21.04 | 0.88 | 357.22 | 0.3030 | -962.7 | -479.6 | |
| 0.00 | 2.98 | 0.00 | 1.57 | 18.80 | 21.05 | 0.89 | 357.44 | 0.3291 | -847.0 | -727.7 | |
| 34.19 | -4.00 | 17.73 | -4.00 | 16.78 | 21.00 | 0.84 | 357.25 | 0.2955 | -1286.8 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 19.41 | 20.11 | -0.05 | 0.13 | 0.3389 | -742.0 | -650.9 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 17.93 | 19.54 | -0.62 | 1.89 | 0.3145 | -828.0 | -646.2 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 17.86 | 19.32 | -0.84 | 2.57 | 0.3136 | -958.0 | -783.8 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 17.86 | 19.12 | -1.04 | 3.16 | 0.3138 | -899.0 | -739.8 | |
| 0.00 | 3.44 | 0.00 | 1.79 | 17.48 | 17.15 | -3.01 | 9.31 | 0.3110 | -912.0 | -705.2 | |
| 2.08 | 2.44 | 1.09 | 1.27 | 17.71 | 16.98 | -3.18 | 9.68 | 0.3151 | -833.5 | -839.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.39 | 16.86 | -3.30 | 10.23 | 0.3102 | -774.0 | -613.7 | |
| 0.00 | 2.26 | 0.00 | 1.18 | 18.12 | 16.40 | -3.76 | 11.15 | 0.3237 | -801.0 | -601.3 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 19.02 | 15.54 | -4.62 | 12.95 | 0.3412 | 763.0 | 631.5 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 19.57 | 15.46 | -4.70 | 12.79 | 0.3502 | 744.0 | 649.4 | |
| 0.00 | 2.17 | 0.00 | 1.15 | 19.90 | 15.16 | -5.00 | 13.35 | 0.3565 | 735.0 | 423.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 20.12 | 15.12 | -5.04 | 13.29 | 0.3603 | 936.0 | 780.8 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 19.83 | 14.87 | -5.29 | 14.14 | 0.3566 | 742.0 | 607.6 | |
| 1.27 | 23.43 | 0.67 | 12.33 | 18.96 | 14.70 | -5.46 | 15.24 | 0.3435 | 830.2 | 806.4 | |
| 1.81 | -20.00 | 0.95 | -20.00 | 18.70 | 14.65 | -5.51 | 15.60 | 0.3397 | 957.0 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 20.74 | 14.38 | -5.78 | 14.69 | 0.3729 | 795.0 | 618.6 | |
| 2.35 | 11.04 | 1.23 | 5.77 | 17.29 | 14.40 | -5.76 | 17.57 | 0.3186 | 1135.1 | 750.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 17.67 | 14.33 | -5.83 | 17.41 | 0.3250 | 831.0 | 660.2 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 23.71 | 13.96 | -6.20 | 13.66 | 0.4206 | 825.0 | 573.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 18.48 | 14.14 | -6.02 | 17.17 | 0.3385 | 975.0 | 796.0 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 21.99 | 13.77 | -6.39 | 15.22 | 0.3948 | 872.0 | 677.2 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 18.41 | 13.75 | -6.40 | 18.25 | 0.3394 | 806.0 | 604.8 | |
| 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. | |