SDO HMI 2014-05-27 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.42 | 35.88 | 9.42 | 21.47 | -10.51 | 83.99 | 32.70 | 252.37 | 0.5589 | 327.9 | 147.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.80 | 17.41 | 8.45 | 10.66 | -9.78 | 86.41 | 35.12 | 254.88 | 0.5894 | 872.1 | 539.9 | |
| 0.00 | 1.53 | 0.00 | 0.93 | -9.70 | 85.20 | 33.91 | 254.59 | 0.5726 | 776.0 | 628.7 | |
| 0.00 | 1.26 | 0.00 | 0.76 | -9.89 | 85.04 | 33.75 | 254.21 | 0.5709 | 647.0 | 561.5 | |
| 1.62 | 3.07 | 0.97 | 1.84 | -10.20 | 84.48 | 33.19 | 253.46 | 0.5642 | 784.4 | 622.8 | |
| 0.00 | 1.35 | 0.00 | 0.82 | -12.02 | 84.68 | 33.39 | 250.43 | 0.5734 | 564.0 | 453.7 | |
| 0.00 | 1.71 | 0.00 | 1.02 | -10.08 | 84.06 | 32.77 | 253.50 | 0.5579 | 827.0 | 720.0 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -12.07 | 83.13 | 31.84 | 249.61 | 0.5525 | 653.0 | 554.4 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -10.58 | 80.33 | 29.04 | 250.85 | 0.5071 | -493.0 | -420.8 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -10.18 | 80.15 | 28.86 | 251.51 | 0.5029 | -485.0 | -370.6 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -10.83 | 80.18 | 28.89 | 250.29 | 0.5060 | -827.0 | -723.0 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -11.78 | 80.07 | 28.78 | 248.42 | 0.5088 | -737.0 | -494.4 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -12.44 | 80.04 | 28.75 | 247.19 | 0.5116 | -625.0 | -479.7 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -9.92 | 77.65 | 26.36 | 250.60 | 0.4656 | -757.0 | -651.5 | |
| 0.00 | 2.98 | 0.00 | 1.65 | -14.37 | 74.63 | 23.33 | 239.09 | 0.4491 | -650.0 | -577.9 | |
| 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. | |