SDO HMI 2014-01-12 23:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.37 | 0.00 | 13.05 | 16.52 | 24.61 | -7.38 | 18.89 | 0.3794 | 433.9 | 275.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.54 | 16.42 | 30.33 | -1.66 | 4.50 | 0.3569 | -674.0 | -549.8 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.31 | 28.36 | -3.63 | 9.79 | 0.3590 | -846.0 | -667.6 | |
| 0.00 | 4.59 | 0.00 | 2.43 | 16.18 | 27.62 | -4.37 | 11.80 | 0.3593 | -893.0 | -760.3 | |
| 0.00 | 2.72 | 0.00 | 1.46 | 16.91 | 24.64 | -7.36 | 18.72 | 0.3835 | 761.0 | 624.4 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 17.22 | 24.62 | -7.37 | 18.47 | 0.3883 | 706.0 | 536.0 | |
| 0.00 | 3.48 | 0.00 | 1.86 | 16.13 | 23.86 | -8.13 | 21.29 | 0.3759 | 969.0 | 788.1 | |
| 0.00 | 0.76 | 0.00 | 0.41 | 15.88 | 23.81 | -8.18 | 21.67 | 0.3725 | 751.0 | 642.2 | |
| 0.00 | 1.10 | 0.00 | 0.59 | 15.88 | 23.44 | -8.56 | 22.55 | 0.3748 | 859.0 | 705.5 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.01 | 23.27 | -8.72 | 22.79 | 0.3777 | 752.0 | 640.4 | |
| 0.00 | 0.93 | 0.00 | 0.50 | 17.06 | 22.63 | -9.36 | 23.14 | 0.3972 | 784.0 | 657.4 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 17.32 | 22.34 | -9.65 | 23.52 | 0.4029 | 647.0 | 505.4 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 17.07 | 22.17 | -9.83 | 24.16 | 0.4004 | 816.0 | 674.8 | |
| 0.00 | 2.72 | 0.00 | 1.47 | 16.78 | 22.09 | -9.91 | 24.64 | 0.3968 | 722.0 | 603.2 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.88 | 21.71 | -10.29 | 25.35 | 0.4008 | 721.0 | 595.7 | |
| 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. | |