SDO HMI 2011-06-01 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 |
| 49.13 | 279.80 | 30.81 | 173.41 | 17.16 | 19.94 | -32.76 | 59.50 | 0.6013 | -235.1 | -290.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.62 | 0.00 | 1.58 | 18.33 | 23.07 | -29.62 | 55.42 | 0.5721 | -807.0 | -629.0 | |
| 0.00 | 1.45 | 0.00 | 0.87 | 18.07 | 22.97 | -29.72 | 55.89 | 0.5715 | -845.0 | -666.1 | |
| 0.00 | 5.33 | 0.00 | 3.32 | 21.35 | 21.83 | -30.86 | 52.03 | 0.6083 | -658.0 | -688.9 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 18.46 | 22.34 | -30.35 | 55.81 | 0.5817 | -666.0 | -502.6 | |
| 15.54 | 205.67 | 9.42 | 125.02 | 16.29 | 21.37 | -31.32 | 59.87 | 0.5791 | -1240.1 | -425.0 | |
| 16.26 | -5.00 | 9.91 | -5.00 | 16.71 | 21.15 | -31.55 | 59.39 | 0.5844 | -1012.1 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.18 | 19.41 | 20.60 | -32.09 | 55.76 | 0.6084 | -664.0 | -621.3 | |
| 0.00 | 0.90 | 0.00 | 0.58 | 22.15 | 19.89 | -32.80 | 52.45 | 0.6351 | -701.0 | -556.8 | |
| 0.00 | 0.90 | 0.00 | 0.56 | 19.02 | 20.49 | -32.20 | 56.40 | 0.6070 | -741.0 | -652.9 | |
| 0.00 | 1.35 | 0.00 | 0.85 | 18.86 | 20.07 | -32.62 | 56.94 | 0.6109 | -603.0 | -460.9 | |
| 0.99 | 3.25 | 0.63 | 2.06 | 17.84 | 18.41 | -34.28 | 59.56 | 0.6242 | -587.3 | -491.2 | |
| 1.35 | 4.16 | 0.86 | 2.63 | 17.72 | 18.21 | -34.49 | 59.88 | 0.6258 | -704.7 | -502.3 | |
| 0.00 | 1.35 | 0.00 | 0.84 | 14.73 | 18.69 | -34.01 | 64.07 | 0.6037 | -711.0 | -610.7 | |
| 2.98 | 6.59 | 1.93 | 4.26 | 18.56 | 16.91 | -35.78 | 59.48 | 0.6457 | 881.0 | 745.5 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 20.09 | 15.55 | -37.14 | 58.19 | 0.6696 | 426.0 | 424.8 | |
| 0.00 | 2.71 | 0.00 | 1.78 | 18.70 | 15.80 | -36.89 | 59.95 | 0.6592 | -615.0 | -453.2 | |
| 0.00 | 2.17 | 0.00 | 1.45 | 20.19 | 15.28 | -37.42 | 58.22 | 0.6732 | 706.0 | 539.0 | |
| 0.00 | 0.54 | 0.00 | 0.35 | 17.76 | 15.87 | -36.82 | 61.22 | 0.6535 | 720.0 | 565.3 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 17.67 | 15.77 | -36.92 | 61.41 | 0.6541 | 659.0 | 553.1 | |
| 0.00 | 2.17 | 0.00 | 1.45 | 20.06 | 15.07 | -37.63 | 58.51 | 0.6748 | 500.0 | 456.5 | |
| 1.99 | 2.62 | 1.32 | 1.74 | 19.41 | 15.21 | -37.49 | 59.32 | 0.6697 | 791.2 | 658.9 | |
| 0.00 | 1.26 | 0.00 | 0.85 | 19.71 | 15.00 | -37.69 | 59.03 | 0.6735 | 640.0 | 547.6 | |
| 0.00 | 1.26 | 0.00 | 0.84 | 19.32 | 14.95 | -37.75 | 59.59 | 0.6721 | 654.0 | 593.8 | |
| 2.26 | 3.61 | 1.51 | 2.42 | 19.54 | 14.80 | -37.89 | 59.37 | 0.6749 | 629.5 | 606.1 | |
| 0.00 | 1.08 | 0.00 | 0.73 | 19.81 | 14.69 | -38.01 | 59.08 | 0.6776 | 428.0 | 305.1 | |
| 1.26 | 1.54 | 0.82 | 1.00 | 15.51 | 15.35 | -37.35 | 64.74 | 0.6486 | -688.1 | -654.0 | |
| 0.00 | 2.44 | 0.00 | 1.64 | 19.61 | 14.29 | -38.40 | 59.56 | 0.6810 | 625.0 | 537.3 | |
| 0.00 | 1.72 | 0.00 | 1.16 | 19.19 | 14.16 | -38.53 | 60.20 | 0.6803 | 775.0 | 709.9 | |
| 0.00 | 0.81 | 0.00 | 0.55 | 19.39 | 14.02 | -38.67 | 60.02 | 0.6828 | 571.0 | 487.4 | |
| 0.00 | 0.90 | 0.00 | 0.60 | 17.39 | 14.51 | -38.18 | 62.49 | 0.6674 | 625.0 | 455.2 | |
| 0.00 | 1.99 | 0.00 | 1.34 | 18.49 | 14.02 | -38.67 | 61.24 | 0.6783 | 801.0 | 706.2 | |
| 0.00 | 1.90 | 0.00 | 1.28 | 18.58 | 13.79 | -38.90 | 61.23 | 0.6814 | 905.0 | 702.6 | |
| 0.00 | 0.90 | 0.00 | 0.61 | 18.59 | 13.58 | -39.11 | 61.34 | 0.6837 | 725.0 | 616.4 | |
| 0.00 | 0.90 | 0.00 | 0.61 | 18.75 | 13.50 | -39.20 | 61.16 | 0.6854 | 639.0 | 524.5 | |
| 3.79 | 10.75 | 2.57 | 7.29 | 18.26 | 13.46 | -39.23 | 61.84 | 0.6835 | 727.7 | 576.9 | |
| 2.71 | -35.00 | 1.84 | -35.00 | 18.65 | 13.27 | -39.42 | 61.41 | 0.6875 | 512.1 | 999999 | |
| 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. | |