SDO HMI 2011-06-01 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.49 | 296.73 | 34.58 | 192.41 | 17.17 | 19.56 | -36.46 | 61.80 | 0.6455 | -361.3 | -184.7 | |
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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 | 0.56 | 17.95 | 22.93 | -33.08 | 58.58 | 0.6107 | -742.0 | -641.5 | |
| 1.81 | 4.61 | 1.17 | 2.98 | 21.27 | 21.71 | -34.30 | 54.74 | 0.6455 | -715.7 | -664.8 | |
| 0.00 | 0.90 | 0.00 | 0.58 | 19.45 | 20.84 | -35.18 | 57.84 | 0.6440 | -500.0 | -443.8 | |
| 18.34 | 207.05 | 11.54 | 130.67 | 16.27 | 21.44 | -34.58 | 62.05 | 0.6190 | -1162.8 | -363.8 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 22.17 | 19.89 | -36.12 | 54.76 | 0.6708 | -632.0 | -505.8 | |
| 18.25 | -4.00 | 11.54 | -4.00 | 16.62 | 21.18 | -34.84 | 61.69 | 0.6241 | -917.8 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.82 | 19.35 | 20.55 | -35.47 | 58.16 | 0.6468 | -709.0 | -559.1 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 19.09 | 20.53 | -35.49 | 58.53 | 0.6454 | -736.0 | -600.2 | |
| 0.00 | 0.81 | 0.00 | 0.53 | 19.71 | 20.26 | -35.76 | 57.84 | 0.6521 | -586.0 | -463.8 | |
| 0.00 | 0.81 | 0.00 | 0.53 | 19.03 | 20.23 | -35.79 | 58.80 | 0.6485 | -614.0 | -516.2 | |
| 0.00 | 1.45 | 0.00 | 0.94 | 19.16 | 20.16 | -35.86 | 58.67 | 0.6501 | -435.0 | -444.6 | |
| 1.54 | -4.00 | 0.97 | -4.00 | 16.34 | 20.77 | -35.25 | 62.35 | 0.6275 | -517.9 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 17.86 | 18.24 | -37.78 | 61.61 | 0.6651 | -423.0 | -363.7 | |
| 0.00 | 1.90 | 0.00 | 1.25 | 17.60 | 18.26 | -37.76 | 61.96 | 0.6635 | -651.0 | -525.1 | |
| 1.17 | 4.34 | 0.76 | 2.82 | 14.87 | 18.48 | -37.54 | 65.76 | 0.6481 | -618.8 | -530.3 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 17.15 | 17.97 | -38.05 | 62.74 | 0.6648 | -493.0 | -348.5 | |
| 2.98 | 5.51 | 2.02 | 3.73 | 18.38 | 16.87 | -39.15 | 61.62 | 0.6832 | 789.8 | 605.7 | |
| 0.00 | 1.54 | 0.00 | 1.06 | 20.10 | 15.95 | -40.06 | 59.80 | 0.7017 | 617.0 | 431.4 | |
| 1.72 | 4.07 | 1.18 | 2.79 | 18.68 | 16.04 | -39.98 | 61.65 | 0.6939 | -595.4 | -354.9 | |
| 0.00 | 2.17 | 0.00 | 1.50 | 19.29 | 15.86 | -40.16 | 60.92 | 0.6988 | 464.0 | 424.6 | |
| 0.00 | 2.80 | 0.00 | 1.91 | 17.71 | 16.10 | -39.92 | 62.92 | 0.6888 | 725.0 | 605.5 | |
| 0.00 | 1.08 | 0.00 | 0.75 | 19.33 | 15.64 | -40.38 | 60.99 | 0.7014 | 706.0 | 622.2 | |
| 0.00 | 2.44 | 0.00 | 1.68 | 18.39 | 15.70 | -40.32 | 62.20 | 0.6964 | -636.0 | -431.1 | |
| 0.00 | 0.90 | 0.00 | 0.63 | 20.08 | 15.11 | -40.91 | 60.27 | 0.7106 | 583.0 | 449.2 | |
| 0.00 | 0.90 | 0.00 | 0.63 | 19.07 | 15.29 | -40.73 | 61.50 | 0.7040 | 586.0 | 468.9 | |
| 0.36 | 4.97 | 0.25 | 3.47 | 19.40 | 15.15 | -40.87 | 61.14 | 0.7070 | 840.2 | 691.5 | |
| 0.00 | 4.07 | 0.00 | 2.86 | 19.82 | 14.89 | -41.13 | 60.72 | 0.7118 | 233.0 | 377.7 | |
| 0.00 | 0.90 | 0.00 | 0.64 | 19.82 | 14.63 | -41.39 | 60.84 | 0.7146 | 274.0 | 248.6 | |
| 0.00 | 3.97 | 0.00 | 2.80 | 19.43 | 14.67 | -41.35 | 61.33 | 0.7124 | 690.0 | 543.7 | |
| 0.00 | 3.16 | 0.00 | 2.24 | 19.40 | 14.33 | -41.69 | 61.53 | 0.7159 | 599.0 | 466.6 | |
| 2.08 | 3.16 | 1.42 | 2.15 | 15.55 | 15.31 | -40.71 | 66.26 | 0.6887 | -672.9 | -543.0 | |
| 0.00 | 2.71 | 0.00 | 1.92 | 19.02 | 14.15 | -41.87 | 62.12 | 0.7162 | 746.0 | 589.1 | |
| 0.00 | 1.72 | 0.00 | 1.21 | 18.53 | 13.99 | -42.03 | 62.83 | 0.7158 | 813.0 | 683.4 | |
| 3.61 | 14.63 | 2.57 | 10.37 | 18.25 | 13.60 | -42.42 | 63.38 | 0.7188 | 774.5 | 470.7 | |
| 0.00 | 1.99 | 0.00 | 1.46 | 21.04 | 12.62 | -43.40 | 60.23 | 0.7410 | 431.0 | 352.3 | |
| 1.63 | 5.69 | 1.16 | 4.07 | 18.60 | 13.36 | -42.66 | 63.02 | 0.7229 | 556.2 | 374.2 | |
| 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. | |