SDO HMI 2014-05-19 16:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.97 | 34.90 | 5.92 | 18.66 | 9.51 | 179.90 | 18.89 | 302.38 | 0.3796 | -414.2 | -166.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.54 | 7.43 | 183.02 | 22.01 | 293.78 | 0.4079 | -778.0 | -685.6 | |
| 7.28 | 16.09 | 3.93 | 8.68 | 9.50 | 181.37 | 20.36 | 300.22 | 0.3987 | -1006.3 | -729.7 | |
| 3.69 | -2.00 | 1.99 | -2.00 | 9.19 | 181.32 | 20.31 | 299.59 | 0.3956 | -1097.4 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 9.28 | 181.03 | 20.02 | 300.14 | 0.3923 | -467.0 | -444.9 | |
| 0.00 | 3.15 | 0.00 | 1.70 | 9.53 | 181.01 | 20.00 | 300.71 | 0.3940 | -1057.0 | -860.1 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 9.68 | 180.89 | 19.88 | 301.20 | 0.3935 | -590.0 | -438.5 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 8.65 | 179.76 | 18.74 | 300.29 | 0.3695 | -874.0 | -673.4 | |
| 0.00 | 1.98 | 0.00 | 1.05 | 8.99 | 179.48 | 18.47 | 301.45 | 0.3684 | -836.0 | -592.9 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 6.78 | 178.19 | 17.18 | 297.68 | 0.3326 | 808.0 | 682.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 10.27 | 178.26 | 17.25 | 306.21 | 0.3632 | 671.0 | 481.0 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 13.74 | 177.65 | 16.64 | 314.41 | 0.3909 | 729.0 | 625.5 | |
| 0.00 | 4.95 | 0.00 | 2.59 | 9.85 | 175.93 | 14.92 | 309.19 | 0.3287 | 685.0 | 687.1 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 11.67 | 173.95 | 12.94 | 317.35 | 0.3251 | 839.0 | 707.5 | |
| 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. | |