SDO HMI 2011-08-22 18:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.88 | 195.63 | 32.12 | 110.43 | -21.24 | 53.41 | 5.06 | 189.89 | 0.4826 | -74.3 | -100.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.65 | -18.27 | 59.18 | 10.84 | 202.84 | 0.4619 | 687.0 | 465.8 | |
| 0.00 | 2.43 | 0.00 | 1.35 | -18.19 | 58.76 | 10.41 | 202.09 | 0.4583 | 757.0 | 671.6 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -18.42 | 58.35 | 10.00 | 201.12 | 0.4592 | 632.0 | 513.6 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -17.82 | 57.02 | 8.68 | 198.98 | 0.4434 | 733.0 | 560.3 | |
| 0.00 | 1.98 | 0.00 | 1.13 | -21.96 | 56.56 | 8.21 | 195.37 | 0.5020 | 424.0 | 410.6 | |
| 16.98 | 44.56 | 9.65 | 25.32 | -21.43 | 56.17 | 7.82 | 194.96 | 0.4928 | 1018.9 | 469.0 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -23.69 | 55.30 | 6.95 | 192.29 | 0.5226 | 813.0 | 605.0 | |
| 13.47 | 33.51 | 7.59 | 18.88 | -20.76 | 54.99 | 6.64 | 193.12 | 0.4785 | 1026.5 | 658.2 | |
| 2.34 | -8.00 | 1.32 | -8.00 | -21.07 | 54.84 | 6.49 | 192.68 | 0.4826 | 645.4 | 999999 | |
| 0.00 | 5.30 | 0.00 | 2.98 | -20.65 | 53.98 | 5.63 | 191.22 | 0.4735 | 937.0 | 814.7 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -19.38 | 53.19 | 4.84 | 190.19 | 0.4519 | -719.0 | -457.4 | |
| 1.26 | 1.80 | 0.71 | 1.02 | -21.74 | 53.00 | 4.65 | 188.93 | 0.4874 | -649.3 | -690.5 | |
| 0.00 | 1.89 | 0.00 | 1.07 | -22.32 | 52.82 | 4.48 | 188.41 | 0.4958 | -858.0 | -690.1 | |
| 0.00 | 3.05 | 0.00 | 1.71 | -20.29 | 52.57 | 4.22 | 188.58 | 0.4643 | -729.0 | -488.0 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -19.23 | 52.44 | 4.10 | 188.70 | 0.4478 | -889.0 | -683.4 | |
| 0.00 | 2.96 | 0.00 | 1.67 | -20.94 | 52.42 | 4.08 | 188.08 | 0.4739 | -439.0 | -406.7 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -21.25 | 52.43 | 4.08 | 188.00 | 0.4787 | -583.0 | -472.8 | |
| 1.53 | 4.04 | 0.86 | 2.28 | -21.73 | 52.35 | 4.00 | 187.69 | 0.4858 | -716.6 | -688.7 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -20.32 | 52.15 | 3.80 | 187.73 | 0.4639 | -903.0 | -724.5 | |
| 0.00 | 0.54 | 0.00 | 0.30 | -20.76 | 52.13 | 3.78 | 187.55 | 0.4707 | -674.0 | -513.0 | |
| 1.98 | 48.87 | 1.11 | 27.44 | -21.24 | 52.04 | 3.69 | 187.25 | 0.4778 | -920.3 | -599.2 | |
| 0.00 | 0.63 | 0.00 | 0.36 | -22.77 | 51.95 | 3.60 | 186.67 | 0.5008 | -547.0 | -408.0 | |
| 11.32 | -21.00 | 6.36 | -21.00 | -21.07 | 51.61 | 3.26 | 186.46 | 0.4744 | -1130.0 | 999999 | |
| 1.89 | 7.46 | 1.06 | 4.20 | -21.30 | 51.06 | 2.72 | 185.33 | 0.4771 | -935.9 | -631.9 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -21.96 | 51.01 | 2.66 | 185.10 | 0.4871 | -738.0 | -672.9 | |
| 0.00 | 2.52 | 0.00 | 1.42 | -21.72 | 50.81 | 2.46 | 184.76 | 0.4831 | -958.0 | -852.7 | |
| 2.16 | 2.78 | 1.22 | 1.58 | -22.03 | 50.68 | 2.34 | 184.46 | 0.4877 | -882.2 | -788.3 | |
| 3.95 | 8.00 | 2.24 | 4.53 | -22.03 | 50.29 | 1.94 | 183.72 | 0.4872 | -906.8 | -640.7 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -21.68 | 50.29 | 1.94 | 183.76 | 0.4819 | -910.0 | -708.2 | |
| 0.00 | 1.98 | 0.00 | 1.12 | -22.06 | 49.61 | 1.26 | 182.40 | 0.4872 | -871.0 | -734.3 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -22.79 | 49.61 | 1.26 | 182.35 | 0.4983 | -812.0 | -558.3 | |
| 0.00 | 2.52 | 0.00 | 1.44 | -23.10 | 49.22 | 0.87 | 181.60 | 0.5029 | -803.0 | -626.3 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -23.21 | 48.92 | 0.58 | 181.05 | 0.5044 | -678.0 | -570.1 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -24.09 | 48.63 | 0.28 | 180.50 | 0.5176 | -874.0 | -766.6 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -24.45 | 48.26 | -0.08 | 179.85 | 0.5229 | -671.0 | -551.8 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -22.13 | 46.86 | -1.49 | 177.16 | 0.4884 | -738.0 | -700.8 | |
| 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. | |