SDO HMI 2014-08-10 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 51.24 | 0.00 | 29.30 | 10.03 | 175.18 | 29.69 | 279.24 | 0.4953 | 177.3 | 127.6 | |
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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 | 0.62 | 10.49 | 183.27 | 37.78 | 278.93 | 0.6120 | -608.0 | -527.5 | |
| 0.00 | 1.72 | 0.00 | 1.04 | 12.04 | 180.72 | 35.23 | 281.87 | 0.5786 | -534.0 | -562.8 | |
| 0.00 | 1.90 | 0.00 | 1.15 | 12.03 | 180.41 | 34.92 | 281.91 | 0.5743 | -815.0 | -709.1 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 12.60 | 180.20 | 34.70 | 282.93 | 0.5722 | -757.0 | -636.6 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 12.99 | 180.26 | 34.77 | 283.61 | 0.5738 | -517.0 | -383.2 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 12.78 | 180.22 | 34.73 | 283.25 | 0.5730 | -638.0 | -595.5 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 11.48 | 179.95 | 34.46 | 281.02 | 0.5671 | -619.0 | -471.1 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 5.71 | 178.95 | 33.45 | 270.69 | 0.5507 | -758.0 | -568.2 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 10.76 | 179.18 | 33.69 | 279.86 | 0.5552 | -588.0 | -418.5 | |
| 0.00 | 1.90 | 0.00 | 1.13 | 11.50 | 179.06 | 33.56 | 281.22 | 0.5544 | -619.0 | -558.5 | |
| 0.00 | 4.15 | 0.00 | 2.44 | 8.84 | 178.08 | 32.58 | 276.46 | 0.5376 | -727.0 | -600.0 | |
| 0.00 | 1.81 | 0.00 | 1.07 | 11.42 | 178.38 | 32.88 | 281.20 | 0.5446 | -918.0 | -753.4 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 9.02 | 177.62 | 32.13 | 276.83 | 0.5310 | -676.0 | -505.4 | |
| 0.00 | 1.08 | 0.00 | 0.63 | 13.21 | 177.12 | 31.62 | 284.82 | 0.5301 | -602.0 | -584.5 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 7.47 | 174.94 | 29.45 | 273.90 | 0.4906 | 425.0 | 391.1 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 9.94 | 174.95 | 29.45 | 278.94 | 0.4923 | 553.0 | 465.3 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 10.04 | 174.81 | 29.32 | 279.16 | 0.4904 | 803.0 | 608.4 | |
| 0.00 | 2.26 | 0.00 | 1.28 | 10.18 | 174.44 | 28.95 | 279.52 | 0.4850 | 878.0 | 713.4 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 9.46 | 173.60 | 28.10 | 278.16 | 0.4713 | 666.0 | 433.9 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 9.32 | 173.34 | 27.85 | 277.91 | 0.4673 | 706.0 | 593.2 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 9.93 | 173.33 | 27.83 | 279.22 | 0.4678 | 564.0 | 485.2 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 9.24 | 173.19 | 27.70 | 277.75 | 0.4649 | 706.0 | 645.6 | |
| 0.00 | 2.26 | 0.00 | 1.26 | 8.66 | 173.11 | 27.62 | 276.52 | 0.4631 | 842.0 | 677.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 9.39 | 173.17 | 27.68 | 278.08 | 0.4648 | 987.0 | 853.3 | |
| 0.00 | 1.81 | 0.00 | 1.01 | 9.09 | 173.15 | 27.65 | 277.43 | 0.4641 | 868.0 | 718.5 | |
| 0.00 | 1.99 | 0.00 | 1.11 | 8.91 | 173.06 | 27.57 | 277.06 | 0.4626 | 843.0 | 673.5 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 9.67 | 173.06 | 27.56 | 278.71 | 0.4634 | 877.0 | 725.7 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 9.04 | 172.90 | 27.41 | 277.36 | 0.4602 | 912.0 | 812.0 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 9.35 | 172.72 | 27.22 | 278.07 | 0.4578 | 853.0 | 673.5 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 9.90 | 172.73 | 27.24 | 279.27 | 0.4587 | 834.0 | 614.4 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 9.18 | 172.56 | 27.07 | 277.71 | 0.4552 | 773.0 | 680.8 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 9.64 | 172.46 | 26.97 | 278.75 | 0.4543 | 709.0 | 538.5 | |
| 0.00 | 4.15 | 0.00 | 2.31 | 9.46 | 172.38 | 26.89 | 278.37 | 0.4527 | 990.0 | 777.8 | |
| 0.00 | 1.90 | 0.00 | 1.05 | 9.13 | 172.32 | 26.82 | 277.64 | 0.4514 | 927.0 | 701.1 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 9.30 | 171.95 | 26.46 | 278.08 | 0.4459 | 823.0 | 673.8 | |
| 0.00 | 1.99 | 0.00 | 1.03 | 12.91 | 162.12 | 16.63 | 292.98 | 0.3043 | -780.0 | -590.7 | |
| 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. | |