SDO HMI 2014-07-07 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.80 | 44.22 | 2.59 | 23.73 | 7.36 | 252.10 | 22.36 | 280.60 | 0.3856 | 436.0 | 391.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.45 | 1.82 | 0.25 | 0.99 | 7.23 | 254.36 | 24.63 | 279.52 | 0.4209 | -916.6 | -756.1 | |
| 0.00 | 1.82 | 0.00 | 0.99 | 6.93 | 254.01 | 24.27 | 278.91 | 0.4148 | -845.0 | -719.4 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 6.91 | 253.77 | 24.03 | 278.92 | 0.4110 | -788.0 | -708.3 | |
| 1.72 | 6.54 | 0.94 | 3.54 | 6.85 | 253.60 | 23.86 | 278.83 | 0.4082 | -1096.7 | -824.6 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 6.49 | 252.41 | 22.67 | 278.25 | 0.3887 | 765.0 | 562.5 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 7.62 | 252.11 | 22.37 | 281.27 | 0.3863 | 630.0 | 665.1 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 8.02 | 252.06 | 22.33 | 282.31 | 0.3866 | 849.0 | 697.9 | |
| 0.00 | 8.53 | 0.00 | 4.58 | 8.30 | 252.05 | 22.31 | 283.03 | 0.3872 | 988.0 | 815.3 | |
| 0.00 | 2.27 | 0.00 | 1.22 | 7.26 | 251.89 | 22.15 | 280.43 | 0.3819 | 833.0 | 708.1 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 8.67 | 251.94 | 22.20 | 284.02 | 0.3866 | 776.0 | 690.2 | |
| 0.00 | 2.18 | 0.00 | 1.17 | 8.61 | 251.77 | 22.03 | 283.97 | 0.3838 | 906.0 | 858.9 | |
| 2.63 | 6.90 | 1.40 | 3.68 | 7.19 | 251.29 | 21.55 | 280.45 | 0.3721 | 998.8 | 769.5 | |
| 0.00 | 2.36 | 0.00 | 1.26 | 7.19 | 250.93 | 21.19 | 280.62 | 0.3664 | 1058.0 | 824.4 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 5.98 | 250.48 | 20.74 | 277.44 | 0.3567 | 783.0 | 649.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 6.17 | 250.39 | 20.65 | 277.98 | 0.3555 | 892.0 | 759.3 | |
| 0.00 | 2.54 | 0.00 | 1.35 | 6.38 | 250.36 | 20.62 | 278.59 | 0.3555 | 854.0 | 715.5 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 7.33 | 250.21 | 20.47 | 281.31 | 0.3553 | 746.0 | 607.0 | |
| 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. | |