SDO HMI 2014-08-19 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.33 | 290.50 | 29.50 | 146.67 | 16.26 | 26.11 | -4.80 | 23.25 | 0.1900 | -88.8 | -169.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.94 | 185.73 | 17.04 | 93.25 | 15.89 | 28.55 | -2.36 | 14.11 | 0.1633 | -1395.1 | -412.6 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 17.95 | 27.98 | -2.93 | 14.12 | 0.2000 | -934.0 | -822.7 | |
| 0.00 | 2.61 | 0.00 | 1.33 | 19.56 | 27.47 | -3.44 | 14.36 | 0.2288 | -774.0 | -684.9 | |
| 0.54 | 2.61 | 0.27 | 1.31 | 16.41 | 27.40 | -3.51 | 19.40 | 0.1775 | -1001.2 | -785.1 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 15.61 | 26.81 | -4.09 | 24.21 | 0.1684 | -835.0 | -679.6 | |
| 2.07 | 12.33 | 1.04 | 6.22 | 16.50 | 26.54 | -4.36 | 23.44 | 0.1842 | -1138.9 | -844.7 | |
| 0.00 | 3.51 | 0.00 | 1.77 | 16.99 | 26.34 | -4.57 | 23.30 | 0.1933 | -916.0 | -773.9 | |
| 1.53 | -6.00 | 0.77 | -6.00 | 16.46 | 26.29 | -4.62 | 24.71 | 0.1855 | -1037.4 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 16.71 | 26.19 | -4.72 | 24.61 | 0.1900 | -831.0 | -694.5 | |
| 0.00 | 2.25 | 0.00 | 1.14 | 16.98 | 25.96 | -4.95 | 25.02 | 0.1959 | -795.0 | -620.7 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 16.82 | 24.95 | -5.96 | 29.73 | 0.2014 | -704.0 | -586.1 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 16.16 | 24.08 | -6.83 | 35.03 | 0.2000 | -910.0 | -793.1 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 18.35 | 21.48 | -9.43 | 37.70 | 0.2554 | 843.0 | 652.8 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 17.32 | 20.98 | -9.92 | 41.85 | 0.2477 | 849.0 | 619.6 | |
| 1.89 | 5.67 | 0.97 | 2.90 | 16.82 | 20.98 | -9.93 | 43.29 | 0.2418 | 1112.8 | 882.1 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 17.53 | 20.94 | -9.97 | 41.37 | 0.2509 | 905.0 | 768.2 | |
| 1.26 | 3.24 | 0.64 | 1.65 | 16.14 | 20.85 | -10.06 | 45.71 | 0.2354 | 1183.6 | 952.9 | |
| 0.00 | 2.16 | 0.00 | 1.10 | 16.51 | 20.83 | -10.08 | 44.62 | 0.2399 | 981.0 | 808.5 | |
| 0.00 | 3.24 | 0.00 | 1.66 | 17.25 | 20.73 | -10.18 | 42.74 | 0.2498 | 817.0 | 719.0 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 18.89 | 20.63 | -10.27 | 38.69 | 0.2712 | 860.0 | 690.5 | |
| 0.00 | 2.70 | 0.00 | 1.38 | 17.62 | 20.68 | -10.23 | 41.85 | 0.2549 | 1070.0 | 861.3 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 15.90 | 20.73 | -10.17 | 46.82 | 0.2340 | 946.0 | 750.0 | |
| 0.00 | 4.23 | 0.00 | 2.16 | 16.91 | 20.55 | -10.35 | 44.20 | 0.2478 | 1005.0 | 828.2 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 17.12 | 20.54 | -10.37 | 43.60 | 0.2505 | 798.0 | 737.3 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 17.21 | 20.38 | -10.53 | 43.79 | 0.2535 | 1037.0 | 838.1 | |
| 0.00 | 2.52 | 0.00 | 1.29 | 17.89 | 20.21 | -10.70 | 42.36 | 0.2634 | 906.0 | 739.9 | |
| 0.00 | 3.24 | 0.00 | 1.66 | 16.93 | 20.20 | -10.71 | 45.06 | 0.2523 | 787.0 | 795.7 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 18.04 | 20.00 | -10.91 | 42.48 | 0.2676 | 829.0 | 664.6 | |
| 0.00 | 5.58 | 0.00 | 2.86 | 17.42 | 20.01 | -10.90 | 44.15 | 0.2602 | 1115.0 | 924.8 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 17.76 | 19.76 | -11.15 | 43.85 | 0.2670 | 792.0 | 507.7 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 17.02 | 19.77 | -11.14 | 45.89 | 0.2583 | 763.0 | 620.8 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 17.32 | 19.69 | -11.22 | 45.22 | 0.2628 | 836.0 | 631.3 | |
| 12.96 | 19.18 | 6.64 | 9.82 | 16.21 | 19.53 | -11.38 | 48.91 | 0.2525 | 1130.9 | 706.9 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 17.07 | 19.28 | -11.62 | 46.93 | 0.2648 | 229.0 | 470.2 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 16.45 | 19.22 | -11.68 | 48.89 | 0.2589 | 657.0 | 535.7 | |
| 4.14 | 7.47 | 2.13 | 3.84 | 17.06 | 19.02 | -11.88 | 47.55 | 0.2680 | 1015.1 | 763.0 | |
| 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. | |