SDO HMI 2014-10-10 16:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.88 | 21.87 | 0.54 | 13.68 | 12.58 | 94.10 | 36.90 | 283.73 | 0.6031 | 80.5 | -91.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.92 | 10.35 | 102.80 | 45.60 | 278.46 | 0.7129 | -240.0 | -281.8 | |
| 0.00 | 0.96 | 0.00 | 0.67 | 10.92 | 101.70 | 44.50 | 279.32 | 0.6997 | -508.0 | -412.9 | |
| 0.00 | 4.64 | 0.00 | 3.19 | 10.91 | 101.40 | 44.20 | 279.32 | 0.6960 | -812.0 | -682.7 | |
| 0.00 | 0.53 | 0.00 | 0.34 | 8.17 | 96.80 | 39.60 | 275.35 | 0.6360 | -575.0 | -470.7 | |
| 0.00 | 2.45 | 0.00 | 1.54 | 10.64 | 95.46 | 38.26 | 279.37 | 0.6190 | -756.0 | -654.9 | |
| 0.00 | 0.61 | 0.00 | 0.38 | 10.45 | 95.08 | 37.88 | 279.10 | 0.6138 | -467.0 | -506.6 | |
| 0.00 | 1.14 | 0.00 | 0.71 | 10.26 | 94.82 | 37.62 | 278.81 | 0.6101 | -648.0 | -473.6 | |
| 0.88 | 2.10 | 0.54 | 1.30 | 11.14 | 93.87 | 36.67 | 280.37 | 0.5980 | 697.0 | 562.5 | |
| 0.00 | 0.96 | 0.00 | 0.56 | 14.92 | 87.87 | 30.67 | 288.65 | 0.5224 | 714.0 | 513.4 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 14.16 | 87.33 | 30.13 | 287.43 | 0.5121 | 649.0 | 483.6 | |
| 0.00 | 2.71 | 0.00 | 1.56 | 15.45 | 86.95 | 29.75 | 290.07 | 0.5113 | 872.0 | 757.7 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 17.02 | 84.36 | 27.16 | 294.54 | 0.4819 | 690.0 | 544.0 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 21.96 | 84.52 | 27.32 | 303.61 | 0.5132 | 709.0 | 586.7 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 16.67 | 82.67 | 25.47 | 294.99 | 0.4564 | 503.0 | 525.2 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 16.85 | 82.11 | 24.91 | 295.78 | 0.4495 | 663.0 | 503.6 | |
| 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. | |