SDO HMI 2014-04-08 04:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.47 | 368.93 | 41.06 | 212.06 | 12.78 | 13.36 | 23.98 | 308.48 | 0.5085 | -1036.5 | -400.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.51 | 11.14 | 14.78 | 25.40 | 304.26 | 0.5113 | -657.0 | -479.9 | |
| 0.00 | 1.15 | 0.00 | 0.67 | 13.62 | 14.43 | 25.05 | 308.57 | 0.5284 | 194.0 | 169.7 | |
| 42.21 | 353.60 | 24.27 | 203.35 | 12.60 | 13.64 | 24.26 | 307.87 | 0.5101 | -1336.7 | -414.9 | |
| 16.04 | -3.00 | 9.21 | -3.00 | 12.90 | 13.20 | 23.82 | 308.85 | 0.5076 | -1285.1 | 999999 | |
| 10.13 | -3.00 | 5.82 | -3.00 | 13.21 | 13.06 | 23.69 | 309.50 | 0.5089 | -1007.4 | 999999 | |
| 0.62 | 1.76 | 0.35 | 1.00 | 12.57 | 11.46 | 22.08 | 310.46 | 0.4843 | -804.7 | -729.9 | |
| 1.06 | 2.20 | 0.60 | 1.25 | 13.39 | 11.27 | 21.90 | 312.00 | 0.4901 | -740.5 | -622.5 | |
| 0.00 | 1.32 | 0.00 | 0.75 | 12.59 | 11.13 | 21.75 | 310.92 | 0.4806 | -787.0 | -584.9 | |
| 1.41 | 2.82 | 0.81 | 1.61 | 14.88 | 10.99 | 21.61 | 314.61 | 0.5021 | -805.3 | -654.2 | |
| 0.00 | 2.47 | 0.00 | 1.39 | 12.69 | 10.41 | 21.04 | 312.03 | 0.4733 | 767.0 | 542.0 | |
| 0.00 | 1.06 | 0.00 | 0.59 | 12.08 | 10.29 | 20.92 | 311.20 | 0.4659 | 679.0 | 523.7 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 12.91 | 10.36 | 20.99 | 312.44 | 0.4750 | 564.0 | 476.9 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 14.34 | 7.70 | 18.33 | 318.51 | 0.4617 | 715.0 | 596.0 | |
| 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. | |