SDO HMI 2014-01-01 18:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.81 | 466.54 | 225.71 | 1391.23 | -8.17 | 99.33 | -80.28 | 97.75 | 0.9843 | 130.2 | -45.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 6.37 | 0.00 | 70.77 | -13.99 | 92.02 | -87.59 | 103.86 | 0.9988 | -193.0 | -213.3 | |
| 42.30 | 352.40 | 96.13 | 909.26 | -7.36 | 101.88 | -77.73 | 96.86 | 0.9771 | 436.5 | 24.2 | |
| 0.93 | -2.00 | 2.28 | -2.00 | -7.48 | 101.22 | -78.40 | 97.00 | 0.9795 | -449.5 | 999999 | |
| 6.20 | 85.27 | 18.21 | 292.91 | -10.06 | 99.00 | -80.61 | 99.68 | 0.9863 | 343.9 | -105.5 | |
| 12.66 | -4.00 | 42.34 | -4.00 | -10.95 | 97.67 | -81.94 | 100.62 | 0.9897 | -104.6 | 999999 | |
| 0.00 | 0.68 | 0.00 | 1.69 | -4.75 | 100.87 | -78.75 | 94.23 | 0.9810 | -386.0 | -386.8 | |
| 12.66 | -2.00 | 36.88 | -2.00 | -6.38 | 99.12 | -80.49 | 95.95 | 0.9863 | 63.6 | 999999 | |
| 0.00 | 2.12 | 0.00 | 5.86 | -4.69 | 99.74 | -79.87 | 94.21 | 0.9846 | -268.0 | -279.9 | |
| 5.35 | -2.00 | 15.75 | -2.00 | -5.49 | 99.14 | -80.47 | 95.05 | 0.9863 | -495.6 | 999999 | |
| 1.95 | 5.44 | 11.06 | 30.32 | -9.45 | 94.27 | -85.34 | 99.22 | 0.9965 | -408.7 | -428.2 | |
| 0.76 | 1.87 | 3.06 | 7.54 | -7.61 | 96.26 | -83.35 | 97.29 | 0.9931 | -297.4 | -329.6 | |
| 0.00 | 2.12 | 0.00 | 8.65 | -6.95 | 96.22 | -83.40 | 96.63 | 0.9933 | -396.0 | -369.0 | |
| 0.00 | 6.62 | 0.00 | 45.04 | -8.24 | 93.55 | -86.07 | 98.04 | 0.9975 | -480.0 | -399.8 | |
| 0.00 | 3.65 | 0.00 | 19.19 | -6.82 | 94.86 | -84.75 | 96.55 | 0.9957 | 15.0 | 99.4 | |
| 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. | |