SDO HMI 2014-08-19 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.84 | 96.81 | 12.24 | 49.55 | -4.82 | 30.18 | 8.07 | 213.96 | 0.2532 | 179.3 | 180.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.23 | 19.43 | 6.31 | 10.02 | -4.17 | 33.91 | 11.80 | 227.27 | 0.2789 | 1125.0 | 653.2 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -4.68 | 32.36 | 10.26 | 221.89 | 0.2670 | 964.0 | 759.7 | |
| 1.71 | 4.86 | 0.88 | 2.49 | -4.10 | 32.32 | 10.22 | 223.30 | 0.2592 | 1092.7 | 822.1 | |
| 3.60 | 11.15 | 1.84 | 5.72 | -4.34 | 32.05 | 9.95 | 221.88 | 0.2591 | 1186.1 | 855.6 | |
| 0.00 | 2.07 | 0.00 | 1.06 | -4.89 | 31.78 | 9.67 | 219.72 | 0.2632 | 1032.0 | 858.3 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -3.99 | 31.49 | 9.39 | 221.14 | 0.2484 | 852.0 | 620.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -4.88 | 31.38 | 9.27 | 218.54 | 0.2589 | 983.0 | 731.5 | |
| 1.08 | 9.80 | 0.55 | 5.02 | -4.63 | 31.22 | 9.12 | 218.67 | 0.2539 | 1156.4 | 952.0 | |
| 0.00 | 2.97 | 0.00 | 1.52 | -5.09 | 31.20 | 9.09 | 217.48 | 0.2598 | 853.0 | 715.4 | |
| 0.00 | 2.79 | 0.00 | 1.43 | -5.21 | 30.70 | 8.60 | 215.68 | 0.2564 | 903.0 | 770.7 | |
| 1.44 | 4.41 | 0.74 | 2.25 | -4.73 | 30.14 | 8.04 | 214.95 | 0.2444 | 995.4 | 666.4 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -5.68 | 29.33 | 7.22 | 210.10 | 0.2506 | -567.0 | -480.2 | |
| 0.00 | 6.93 | 0.00 | 3.54 | -5.36 | 29.11 | 7.00 | 209.97 | 0.2441 | -1055.0 | -853.3 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -5.98 | 29.05 | 6.95 | 208.56 | 0.2528 | -932.0 | -812.1 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -5.73 | 28.99 | 6.88 | 208.81 | 0.2486 | -1045.0 | -939.3 | |
| 1.89 | 3.87 | 0.96 | 1.97 | -4.25 | 28.85 | 6.75 | 211.47 | 0.2255 | -1157.1 | -875.4 | |
| 1.53 | 4.05 | 0.78 | 2.06 | -4.58 | 28.73 | 6.63 | 210.25 | 0.2294 | -1006.7 | -703.0 | |
| 0.36 | 1.17 | 0.18 | 0.59 | -4.30 | 28.64 | 6.53 | 210.52 | 0.2245 | -1000.2 | -858.6 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -3.62 | 26.01 | 3.91 | 200.55 | 0.1945 | 896.0 | 637.9 | |
| 0.00 | 1.62 | 0.00 | 0.81 | -2.91 | 25.13 | 3.02 | 197.29 | 0.1779 | -322.0 | -367.6 | |
| 0.00 | 0.36 | 0.00 | 0.19 | -13.80 | 24.70 | 2.59 | 187.11 | 0.3566 | -339.0 | -472.2 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -4.93 | 22.91 | 0.80 | 183.92 | 0.2054 | -647.0 | -571.3 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -6.08 | 22.39 | 0.29 | 181.27 | 0.2247 | -738.0 | -640.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -7.70 | 22.11 | 0.01 | 180.04 | 0.2522 | -875.0 | -768.9 | |
| 0.00 | 4.59 | 0.00 | 2.34 | -6.55 | 21.84 | -0.26 | 178.87 | 0.2326 | -1023.0 | -715.3 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -7.14 | 21.81 | -0.30 | 178.78 | 0.2427 | -883.0 | -673.2 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -9.35 | 18.73 | -3.38 | 168.22 | 0.2858 | -814.0 | -615.1 | |
| 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. | |