SDO HMI 2014-04-15 15:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.14 | 381.17 | 30.35 | 217.42 | 11.91 | 275.09 | 24.15 | 306.16 | 0.4979 | -929.0 | -362.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.61 | 8.32 | 277.80 | 26.87 | 297.19 | 0.5047 | -712.0 | -534.1 | |
| 52.43 | 359.60 | 29.96 | 205.43 | 11.84 | 275.36 | 24.42 | 305.69 | 0.5003 | -1412.1 | -411.3 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 14.57 | 272.28 | 21.34 | 313.81 | 0.4902 | -711.0 | -510.4 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 14.18 | 272.04 | 21.10 | 313.53 | 0.4835 | -742.0 | -576.6 | |
| 0.71 | 7.69 | 0.39 | 4.27 | 12.68 | 270.95 | 20.01 | 312.65 | 0.4558 | 849.5 | 683.5 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 16.24 | 271.26 | 20.32 | 317.65 | 0.4970 | -570.0 | -499.9 | |
| 0.00 | 1.06 | 0.00 | 0.59 | 14.26 | 270.66 | 19.72 | 315.58 | 0.4692 | -764.0 | -573.7 | |
| 0.00 | 1.95 | 0.00 | 1.08 | 12.98 | 270.28 | 19.35 | 314.10 | 0.4514 | 1039.0 | 840.2 | |
| 0.00 | 2.83 | 0.00 | 1.56 | 13.08 | 269.41 | 18.47 | 315.57 | 0.4428 | 841.0 | 584.5 | |
| 0.00 | 0.71 | 0.00 | 0.39 | 14.67 | 268.50 | 17.56 | 319.49 | 0.4512 | 735.0 | 670.0 | |
| 0.00 | 1.15 | 0.00 | 0.64 | 14.47 | 268.12 | 17.19 | 319.80 | 0.4451 | 908.0 | 725.1 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 13.76 | 267.68 | 16.74 | 319.45 | 0.4321 | 943.0 | 759.9 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 12.23 | 266.22 | 15.29 | 319.56 | 0.3989 | 816.0 | 647.7 | |
| 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. | |