SDO HMI 2014-01-12 06:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.16 | 108.76 | 26.13 | 56.61 | -17.93 | 29.54 | -11.79 | 140.81 | 0.3085 | 55.6 | 190.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.76 | 50.76 | 11.27 | 26.31 | -17.55 | 30.52 | -10.81 | 142.26 | 0.2934 | 1131.6 | 603.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -17.00 | 30.40 | -10.93 | 140.72 | 0.2878 | 804.0 | 665.8 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -18.12 | 30.27 | -11.06 | 142.86 | 0.3034 | 839.0 | 740.5 | |
| 2.13 | -1.00 | 1.10 | -1.00 | -17.66 | 30.08 | -11.26 | 141.41 | 0.2995 | 754.1 | 999999 | |
| 0.00 | 4.51 | 0.00 | 2.34 | -18.30 | 30.03 | -11.30 | 142.67 | 0.3081 | 488.0 | 500.8 | |
| 0.00 | 2.38 | 0.00 | 1.24 | -18.02 | 29.86 | -11.47 | 141.68 | 0.3063 | -83.0 | -112.4 | |
| 0.00 | 1.79 | 0.00 | 0.93 | -17.44 | 29.59 | -11.75 | 139.75 | 0.3020 | 737.0 | 668.0 | |
| 0.00 | 2.64 | 0.00 | 1.37 | -18.26 | 29.50 | -11.83 | 141.33 | 0.3131 | -285.0 | -278.9 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -17.32 | 29.50 | -11.83 | 139.28 | 0.3014 | 707.0 | 582.8 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -18.41 | 29.07 | -12.26 | 140.68 | 0.3193 | -157.0 | -242.7 | |
| 1.11 | 41.49 | 0.58 | 21.72 | -18.58 | 28.74 | -12.59 | 140.32 | 0.3250 | -970.1 | -615.1 | |
| 11.56 | -11.00 | 6.06 | -11.00 | -18.49 | 28.37 | -12.96 | 139.31 | 0.3278 | -1030.5 | 999999 | |
| 13.60 | -11.00 | 7.12 | -11.00 | -18.21 | 28.23 | -13.10 | 138.43 | 0.3260 | -1113.6 | 999999 | |
| 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. | |