SDO HMI 2014-05-19 23:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.63 | 220.09 | 22.20 | 140.85 | -24.67 | 190.43 | 33.30 | 232.03 | 0.6350 | 556.5 | 315.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.63 | 205.96 | 22.20 | 132.05 | -24.53 | 190.71 | 33.58 | 232.46 | 0.6368 | 1073.5 | 363.9 | |
| 0.00 | 1.35 | 0.00 | 0.88 | -26.35 | 190.64 | 33.51 | 229.95 | 0.6485 | 612.0 | 519.5 | |
| 0.00 | 1.53 | 0.00 | 0.99 | -26.59 | 190.47 | 33.34 | 229.52 | 0.6484 | 685.0 | 558.9 | |
| 0.00 | 1.62 | 0.00 | 0.99 | -24.48 | 185.74 | 28.61 | 228.59 | 0.5833 | -721.0 | -561.2 | |
| 0.00 | 1.35 | 0.00 | 0.83 | -26.33 | 185.84 | 28.71 | 226.12 | 0.5995 | -725.0 | -560.5 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -26.50 | 185.81 | 28.68 | 225.87 | 0.6006 | -631.0 | -515.2 | |
| 0.00 | 1.80 | 0.00 | 1.11 | -26.64 | 185.65 | 28.52 | 225.54 | 0.6001 | -724.0 | -612.2 | |
| 0.00 | 1.53 | 0.00 | 0.95 | -27.07 | 185.65 | 28.52 | 224.97 | 0.6039 | -544.0 | -440.5 | |
| 0.00 | 0.45 | 0.00 | 0.28 | -27.55 | 185.01 | 27.88 | 223.75 | 0.6017 | -727.0 | -613.6 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -28.13 | 184.98 | 27.85 | 222.98 | 0.6065 | -593.0 | -438.1 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -28.57 | 184.95 | 27.82 | 222.39 | 0.6101 | -496.0 | -391.1 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -28.58 | 184.33 | 27.20 | 221.80 | 0.6044 | -746.0 | -639.8 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -28.37 | 179.74 | 22.61 | 217.27 | 0.5608 | -191.0 | -296.3 | |
| 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. | |