SDO HMI 2011-06-03 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.38 | 287.23 | 30.58 | 150.47 | 17.36 | 19.69 | -6.54 | 19.16 | 0.3264 | -302.6 | -288.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.47 | 17.77 | 22.03 | -4.19 | 12.59 | 0.3208 | 695.0 | 469.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 18.61 | 21.21 | -5.02 | 14.29 | 0.3374 | -916.0 | -741.3 | |
| 21.78 | 182.39 | 11.33 | 94.88 | 16.63 | 21.17 | -5.06 | 16.11 | 0.3059 | -1312.2 | -501.6 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 22.06 | 20.99 | -5.23 | 12.48 | 0.3927 | -704.0 | -566.8 | |
| 9.40 | 33.89 | 4.91 | 17.71 | 17.30 | 21.02 | -5.21 | 15.92 | 0.3173 | -993.3 | -290.6 | |
| 14.64 | -3.00 | 7.64 | -3.00 | 16.95 | 20.68 | -5.55 | 17.24 | 0.3133 | -1064.0 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 18.51 | 19.95 | -6.27 | 17.73 | 0.3416 | -926.0 | -740.7 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 18.13 | 19.81 | -6.42 | 18.50 | 0.3363 | -764.0 | -636.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 17.90 | 19.69 | -6.54 | 19.05 | 0.3335 | -807.0 | -583.4 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 17.84 | 19.40 | -6.83 | 19.89 | 0.3341 | -896.0 | -746.5 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 17.87 | 19.14 | -7.09 | 20.54 | 0.3361 | -820.0 | -688.0 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 19.68 | 17.04 | -9.19 | 23.66 | 0.3762 | 766.0 | 577.8 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 18.04 | 17.00 | -9.22 | 25.75 | 0.3524 | -899.0 | -679.2 | |
| 0.00 | 3.98 | 0.00 | 2.10 | 17.81 | 16.95 | -9.28 | 26.17 | 0.3495 | -901.0 | -819.4 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 18.07 | 16.71 | -9.52 | 26.41 | 0.3549 | -829.0 | -731.6 | |
| 2.08 | 4.88 | 1.10 | 2.59 | 18.32 | 16.63 | -9.60 | 26.26 | 0.3592 | -843.7 | -633.2 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 18.97 | 15.42 | -10.81 | 28.16 | 0.3775 | 851.0 | 707.6 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 20.95 | 15.11 | -11.11 | 26.33 | 0.4076 | 778.0 | 638.4 | |
| 0.00 | 2.80 | 0.00 | 1.51 | 20.10 | 15.14 | -11.09 | 27.29 | 0.3955 | 1018.0 | 749.0 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 19.00 | 15.15 | -11.07 | 28.68 | 0.3800 | 989.0 | 786.6 | |
| 0.00 | 3.34 | 0.00 | 1.78 | 18.07 | 15.05 | -11.18 | 30.20 | 0.3678 | 914.0 | 783.5 | |
| 1.08 | 3.62 | 0.58 | 1.94 | 19.04 | 14.92 | -11.31 | 29.14 | 0.3823 | 1058.5 | 797.0 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 16.19 | 15.07 | -11.16 | 33.09 | 0.3419 | 618.0 | 525.4 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 21.97 | 14.56 | -11.66 | 26.24 | 0.4257 | 518.0 | 508.2 | |
| 2.62 | 11.57 | 1.40 | 6.20 | 18.78 | 14.77 | -11.45 | 29.80 | 0.3799 | 1142.4 | 818.6 | |
| 0.00 | 2.26 | 0.00 | 1.20 | 17.69 | 14.68 | -11.54 | 31.57 | 0.3656 | 934.0 | 720.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 19.10 | 14.59 | -11.64 | 29.75 | 0.3858 | 702.0 | 567.5 | |
| 3.89 | -25.00 | 2.08 | -25.00 | 18.87 | 14.54 | -11.69 | 30.17 | 0.3831 | 858.8 | 999999 | |
| 2.89 | 5.06 | 1.54 | 2.69 | 17.46 | 14.60 | -11.62 | 32.10 | 0.3633 | 1022.5 | 868.2 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 17.75 | 14.42 | -11.81 | 32.05 | 0.3688 | 923.0 | 719.2 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 23.42 | 13.96 | -12.26 | 25.77 | 0.4501 | 729.0 | 508.1 | |
| 0.00 | 3.16 | 0.00 | 1.69 | 18.30 | 14.28 | -11.94 | 31.53 | 0.3773 | 874.0 | 711.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 23.26 | 13.78 | -12.45 | 26.29 | 0.4491 | 689.0 | 553.3 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 20.07 | 14.05 | -12.17 | 29.54 | 0.4034 | 820.0 | 620.1 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 23.69 | 13.67 | -12.56 | 26.02 | 0.4558 | 431.0 | 376.4 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 18.52 | 14.07 | -12.16 | 31.64 | 0.3822 | 715.0 | 555.8 | |
| 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. | |