SDO HMI 2011-06-03 17:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.32 | 294.18 | 28.00 | 154.48 | 17.36 | 19.68 | -7.65 | 22.17 | 0.3329 | -213.2 | -286.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.52 | 17.22 | 21.72 | -5.62 | 17.17 | 0.3182 | -106.0 | -81.0 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 18.60 | 21.19 | -6.15 | 17.31 | 0.3425 | -915.0 | -705.7 | |
| 18.44 | 221.51 | 9.61 | 115.53 | 16.62 | 21.23 | -6.11 | 19.22 | 0.3112 | -1353.9 | -475.0 | |
| 8.40 | -3.00 | 4.40 | -3.00 | 17.29 | 21.04 | -6.29 | 19.01 | 0.3227 | -1021.4 | 999999 | |
| 14.73 | -3.00 | 7.70 | -3.00 | 16.91 | 20.67 | -6.66 | 20.47 | 0.3188 | -1070.8 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 17.45 | 20.46 | -6.88 | 20.44 | 0.3284 | -472.0 | -352.2 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 18.47 | 19.94 | -7.40 | 20.69 | 0.3472 | -653.0 | -509.6 | |
| 0.00 | 2.17 | 0.00 | 1.14 | 18.12 | 19.76 | -7.58 | 21.54 | 0.3429 | -836.0 | -718.4 | |
| 0.00 | 2.80 | 0.00 | 1.48 | 17.80 | 19.42 | -7.92 | 22.79 | 0.3402 | -854.0 | -672.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.83 | 19.16 | -8.18 | 23.41 | 0.3423 | -872.0 | -729.4 | |
| 0.00 | 8.40 | 0.00 | 4.46 | 18.03 | 16.82 | -10.52 | 28.79 | 0.3621 | -1005.0 | -757.6 | |
| 0.00 | 2.26 | 0.00 | 1.21 | 19.03 | 16.52 | -10.81 | 28.08 | 0.3784 | 735.0 | 604.3 | |
| 2.26 | 2.62 | 1.20 | 1.40 | 18.38 | 16.50 | -10.84 | 29.00 | 0.3696 | -724.2 | -719.5 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 18.90 | 15.42 | -11.92 | 30.60 | 0.3854 | 517.0 | 548.1 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 21.17 | 15.14 | -12.20 | 28.19 | 0.4187 | 751.0 | 604.1 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 21.43 | 15.12 | -12.22 | 27.92 | 0.4225 | 685.0 | 589.1 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 20.06 | 15.16 | -12.17 | 29.54 | 0.4034 | 853.0 | 762.2 | |
| 0.00 | 1.72 | 0.00 | 0.93 | 20.26 | 15.15 | -12.19 | 29.32 | 0.4061 | 687.0 | 501.5 | |
| 0.00 | 2.26 | 0.00 | 1.21 | 18.03 | 15.19 | -12.15 | 32.35 | 0.3757 | 851.0 | 746.2 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 19.00 | 15.12 | -12.22 | 31.09 | 0.3893 | 922.0 | 737.9 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 19.97 | 15.04 | -12.30 | 29.92 | 0.4030 | 811.0 | 615.9 | |
| 2.35 | 3.71 | 1.26 | 1.99 | 19.03 | 14.88 | -12.45 | 31.52 | 0.3917 | 960.2 | 804.9 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 16.21 | 15.01 | -12.32 | 35.65 | 0.3532 | 683.0 | 502.4 | |
| 2.17 | 13.10 | 1.17 | 7.04 | 18.74 | 14.81 | -12.53 | 32.09 | 0.3884 | 1068.6 | 854.2 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 21.96 | 14.54 | -12.80 | 28.39 | 0.4340 | 707.0 | 436.0 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 17.78 | 14.75 | -12.59 | 33.66 | 0.3761 | 1025.0 | 819.1 | |
| 2.62 | 3.89 | 1.40 | 2.07 | 17.49 | 14.70 | -12.64 | 34.20 | 0.3728 | 1021.8 | 914.0 | |
| 2.35 | -24.00 | 1.26 | -24.00 | 18.80 | 14.57 | -12.77 | 32.47 | 0.3913 | 907.7 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 19.06 | 14.55 | -12.79 | 32.14 | 0.3949 | 713.0 | 546.1 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 17.68 | 14.56 | -12.78 | 34.20 | 0.3766 | 820.0 | 712.5 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 17.81 | 14.42 | -12.92 | 34.28 | 0.3796 | 890.0 | 691.6 | |
| 0.00 | 1.99 | 0.00 | 1.07 | 18.32 | 14.25 | -13.09 | 33.83 | 0.3878 | 820.0 | 730.7 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 19.97 | 14.08 | -13.26 | 31.79 | 0.4110 | 896.0 | 707.3 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 17.87 | 14.21 | -13.12 | 34.59 | 0.3823 | 698.0 | 490.9 | |
| 0.00 | 2.89 | 0.00 | 1.61 | 22.66 | 13.32 | -14.02 | 29.73 | 0.4526 | 588.0 | 520.5 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 20.13 | 13.03 | -14.31 | 33.50 | 0.4221 | 708.0 | 541.1 | |
| 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. | |