SDO HMI 2014-04-08 12:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.11 | 144.80 | 29.88 | 100.19 | 2.99 | 28.05 | 43.06 | 281.17 | 0.6954 | 134.5 | -68.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.59 | 5.37 | 1.20 | 4.06 | 1.77 | 33.47 | 48.48 | 277.69 | 0.7574 | -542.9 | -335.4 | |
| 0.88 | 2.47 | 0.67 | 1.86 | 2.19 | 33.35 | 48.36 | 278.26 | 0.7569 | -496.6 | -384.5 | |
| 6.61 | 13.74 | 4.96 | 10.30 | 1.86 | 33.11 | 48.12 | 277.89 | 0.7535 | -758.0 | -669.6 | |
| 0.00 | 1.32 | 0.00 | 0.97 | 1.77 | 31.94 | 46.95 | 278.04 | 0.7400 | -494.0 | -398.3 | |
| 0.00 | 0.53 | 0.00 | 0.39 | 3.47 | 31.90 | 46.91 | 280.30 | 0.7431 | -441.0 | -380.2 | |
| 4.32 | 16.47 | 3.15 | 11.98 | 1.90 | 31.60 | 46.60 | 278.29 | 0.7362 | -818.9 | -611.5 | |
| 5.02 | -6.00 | 3.65 | -6.00 | 1.62 | 31.50 | 46.51 | 277.93 | 0.7345 | -886.5 | 999999 | |
| 0.35 | 1.59 | 0.26 | 1.15 | 2.08 | 31.17 | 46.17 | 278.63 | 0.7315 | -716.2 | -617.2 | |
| 0.00 | 0.70 | 0.00 | 0.51 | 1.89 | 31.12 | 46.12 | 278.39 | 0.7305 | -810.0 | -777.0 | |
| 0.70 | 4.49 | 0.51 | 3.24 | 2.25 | 31.00 | 46.01 | 278.90 | 0.7299 | -766.6 | -586.5 | |
| 0.00 | 1.41 | 0.00 | 1.01 | 1.22 | 30.66 | 45.67 | 277.59 | 0.7238 | -474.0 | -381.9 | |
| 0.00 | 0.26 | 0.00 | 0.19 | 1.31 | 29.85 | 44.86 | 277.90 | 0.7142 | 214.0 | 301.7 | |
| 0.62 | 79.91 | 0.43 | 54.76 | 2.94 | 28.44 | 43.45 | 280.54 | 0.7009 | 510.4 | 40.1 | |
| 0.00 | 0.70 | 0.00 | 0.49 | 3.45 | 28.47 | 43.48 | 281.26 | 0.7026 | -330.0 | -408.0 | |
| 0.70 | -13.00 | 0.49 | -13.00 | 2.86 | 28.27 | 43.28 | 280.49 | 0.6986 | 543.8 | 999999 | |
| 5.90 | -13.00 | 4.05 | -13.00 | 2.99 | 27.95 | 42.95 | 280.77 | 0.6950 | 709.6 | 999999 | |
| 15.42 | -13.00 | 10.51 | -13.00 | 2.93 | 27.53 | 42.54 | 280.81 | 0.6897 | 964.8 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.18 | 2.41 | 26.58 | 41.58 | 280.34 | 0.6764 | -500.0 | -459.3 | |
| 0.00 | 1.76 | 0.00 | 1.15 | 7.86 | 23.56 | 38.57 | 289.45 | 0.6572 | 601.0 | 451.1 | |
| 0.00 | 1.85 | 0.00 | 1.07 | 8.21 | 12.66 | 27.67 | 297.07 | 0.5182 | 723.0 | 565.8 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 8.02 | 12.61 | 27.62 | 296.79 | 0.5163 | 654.0 | 564.0 | |
| 0.00 | 3.61 | 0.00 | 2.08 | 7.76 | 12.32 | 27.32 | 296.58 | 0.5106 | 885.0 | 676.1 | |
| 0.00 | 1.23 | 0.00 | 0.71 | 7.45 | 12.26 | 27.27 | 296.08 | 0.5078 | 809.0 | 692.9 | |
| 0.00 | 1.76 | 0.00 | 1.01 | 6.97 | 12.03 | 27.03 | 295.43 | 0.5015 | 702.0 | 569.3 | |
| 0.00 | 1.41 | 0.00 | 0.81 | 7.49 | 11.96 | 26.97 | 296.42 | 0.5040 | 848.0 | 760.2 | |
| 0.00 | 1.41 | 0.00 | 0.80 | 6.28 | 11.71 | 26.72 | 294.42 | 0.4928 | 871.0 | 710.8 | |
| 0.00 | 1.67 | 0.00 | 0.96 | 8.87 | 11.62 | 26.63 | 299.15 | 0.5091 | 614.0 | 408.4 | |
| 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. | |