SDO HMI 2014-05-19 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.68 | 46.69 | 7.23 | 24.60 | 9.64 | 180.27 | 15.96 | 307.12 | 0.3418 | -359.2 | -335.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.89 | 0.00 | 1.00 | 7.34 | 183.03 | 18.71 | 297.18 | 0.3592 | -841.0 | -712.0 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 9.00 | 181.85 | 17.54 | 302.82 | 0.3557 | -791.0 | -580.5 | |
| 8.28 | 30.13 | 4.38 | 15.94 | 9.58 | 181.33 | 17.02 | 304.99 | 0.3538 | -1044.9 | -716.1 | |
| 5.40 | -3.00 | 2.85 | -3.00 | 9.27 | 181.22 | 16.91 | 304.43 | 0.3495 | -1124.4 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 8.49 | 180.90 | 16.58 | 303.03 | 0.3381 | -696.0 | -607.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 10.67 | 178.99 | 14.67 | 311.62 | 0.3344 | -799.0 | -641.7 | |
| 0.00 | 3.51 | 0.00 | 1.85 | 12.11 | 178.59 | 14.27 | 315.53 | 0.3455 | -420.0 | -282.6 | |
| 0.00 | 2.07 | 0.00 | 1.07 | 6.71 | 177.97 | 13.66 | 303.19 | 0.2815 | 912.0 | 689.1 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 10.41 | 177.70 | 13.39 | 313.61 | 0.3159 | 625.0 | 523.5 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 10.13 | 177.66 | 13.34 | 313.04 | 0.3122 | 849.0 | 671.5 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 12.06 | 176.35 | 12.04 | 320.22 | 0.3202 | 814.0 | 634.1 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 11.64 | 174.13 | 9.81 | 324.98 | 0.2921 | 899.0 | 667.4 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 10.76 | 173.81 | 9.50 | 324.03 | 0.2772 | 682.0 | 458.1 | |
| 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. | |