SDO HMI 2014-02-25 22:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.34 | 128.55 | 27.11 | 88.16 | 8.44 | 132.31 | -40.86 | 69.70 | 0.6920 | 512.2 | 215.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.46 | 0.00 | 0.89 | 7.41 | 141.05 | -32.13 | 66.18 | 0.5787 | -652.0 | -594.4 | |
| 0.00 | 1.12 | 0.00 | 0.68 | 7.39 | 140.87 | -32.30 | 66.33 | 0.5809 | -568.0 | -488.2 | |
| 0.00 | 1.38 | 0.00 | 0.85 | 8.29 | 139.90 | -33.28 | 65.59 | 0.5985 | -638.0 | -517.7 | |
| 0.00 | 1.38 | 0.00 | 0.85 | 8.91 | 139.77 | -33.41 | 64.73 | 0.6038 | -750.0 | -568.2 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 5.08 | 139.61 | -33.57 | 70.83 | 0.5853 | -556.0 | -491.7 | |
| 0.00 | 1.38 | 0.00 | 0.90 | 7.59 | 135.35 | -37.82 | 69.37 | 0.6518 | -729.0 | -625.7 | |
| 0.00 | 1.55 | 0.00 | 1.03 | 6.87 | 133.35 | -39.83 | 71.41 | 0.6732 | -622.0 | -417.0 | |
| 0.00 | 1.21 | 0.00 | 0.81 | 7.33 | 132.91 | -40.27 | 70.97 | 0.6805 | 755.0 | 555.9 | |
| 8.95 | 33.92 | 6.12 | 23.19 | 8.69 | 132.51 | -40.67 | 69.30 | 0.6910 | 1071.9 | 416.7 | |
| 0.00 | 2.67 | 0.00 | 1.82 | 7.21 | 132.17 | -41.01 | 71.48 | 0.6889 | 500.0 | 508.9 | |
| 30.39 | 76.36 | 20.99 | 52.89 | 8.42 | 131.70 | -41.47 | 70.05 | 0.6993 | 791.4 | 254.5 | |
| 0.00 | 1.38 | 0.00 | 0.97 | 8.94 | 130.94 | -42.23 | 69.70 | 0.7103 | 386.0 | 249.4 | |
| 0.00 | 1.21 | 0.00 | 0.85 | 9.17 | 130.87 | -42.30 | 69.44 | 0.7120 | 369.0 | 295.1 | |
| 0.00 | 2.67 | 0.00 | 1.91 | 10.02 | 130.24 | -42.93 | 68.61 | 0.7227 | -635.0 | -480.6 | |
| 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. | |