SDO HMI 2014-01-06 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 114.90 | 427.31 | 61.93 | 230.90 | 9.09 | 99.54 | -19.72 | 56.77 | 0.3992 | 205.0 | 172.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.24 | 50.83 | 6.42 | 26.71 | 8.53 | 104.32 | -14.93 | 50.72 | 0.3307 | -1225.1 | -536.4 | |
| 0.00 | 2.63 | 0.00 | 1.38 | 8.03 | 103.85 | -15.41 | 52.80 | 0.3318 | -700.0 | -652.9 | |
| 0.00 | 1.87 | 0.00 | 0.98 | 8.24 | 103.62 | -15.63 | 52.68 | 0.3369 | -898.0 | -763.1 | |
| 14.19 | -1.00 | 7.48 | -1.00 | 8.69 | 103.57 | -15.68 | 51.70 | 0.3420 | -1038.8 | 999999 | |
| 3.65 | 5.61 | 1.93 | 2.97 | 8.98 | 103.06 | -16.19 | 51.94 | 0.3514 | -970.1 | -668.1 | |
| 0.00 | 3.57 | 0.00 | 1.88 | 8.61 | 103.05 | -16.21 | 52.79 | 0.3480 | -842.0 | -739.1 | |
| 0.00 | 0.59 | 0.00 | 0.32 | 9.40 | 103.01 | -16.24 | 51.07 | 0.3563 | -672.0 | -497.9 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 10.22 | 102.94 | -16.31 | 49.42 | 0.3656 | -710.0 | -573.9 | |
| 0.85 | 15.13 | 0.45 | 7.97 | 7.65 | 103.02 | -16.23 | 55.13 | 0.3391 | -1201.0 | -874.8 | |
| 0.00 | 2.29 | 0.00 | 1.22 | 9.07 | 102.65 | -16.60 | 52.40 | 0.3577 | -872.0 | -752.0 | |
| 2.38 | -9.00 | 1.26 | -9.00 | 7.78 | 102.62 | -16.64 | 55.48 | 0.3458 | -984.3 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 8.56 | 102.55 | -16.70 | 53.73 | 0.3540 | -886.0 | -709.6 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 9.23 | 102.43 | -16.83 | 52.43 | 0.3621 | -733.0 | -536.3 | |
| 0.00 | 2.55 | 0.00 | 1.36 | 9.46 | 101.70 | -17.56 | 53.10 | 0.3738 | -822.0 | -582.2 | |
| 1.10 | 2.12 | 0.59 | 1.13 | 9.07 | 101.37 | -17.88 | 54.44 | 0.3744 | -801.2 | -674.2 | |
| 2.63 | 4.67 | 1.41 | 2.50 | 9.65 | 101.25 | -18.01 | 53.38 | 0.3814 | -1062.2 | -754.0 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 8.11 | 101.32 | -17.93 | 56.69 | 0.3663 | -877.0 | -563.5 | |
| 0.51 | 3.40 | 0.27 | 1.81 | 8.17 | 101.07 | -18.18 | 56.90 | 0.3703 | -894.2 | -734.0 | |
| 0.00 | 2.55 | 0.00 | 1.37 | 9.87 | 100.70 | -18.56 | 53.72 | 0.3906 | -819.0 | -646.7 | |
| 0.00 | 2.38 | 0.00 | 1.27 | 8.51 | 100.74 | -18.51 | 56.61 | 0.3778 | -740.0 | -479.5 | |
| 0.00 | 2.80 | 0.00 | 1.51 | 9.66 | 100.65 | -18.61 | 54.24 | 0.3893 | -944.0 | -583.1 | |
| 0.00 | 1.61 | 0.00 | 0.87 | 9.39 | 100.57 | -18.69 | 54.93 | 0.3879 | 161.0 | 107.4 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 7.76 | 100.65 | -18.60 | 58.44 | 0.3726 | -847.0 | -648.8 | |
| 0.00 | 1.78 | 0.00 | 0.95 | 7.79 | 100.46 | -18.79 | 58.62 | 0.3755 | -792.0 | -613.2 | |
| 0.00 | 1.53 | 0.00 | 0.83 | 9.79 | 100.07 | -19.18 | 54.78 | 0.3981 | 445.0 | 493.7 | |
| 0.00 | 1.78 | 0.00 | 0.96 | 9.20 | 99.82 | -19.43 | 56.38 | 0.3961 | 952.0 | 781.2 | |
| 0.00 | 2.63 | 0.00 | 1.42 | 9.68 | 99.70 | -19.56 | 55.52 | 0.4020 | 817.0 | 764.7 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 8.62 | 99.76 | -19.50 | 57.71 | 0.3921 | 838.0 | 666.2 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 8.54 | 99.63 | -19.62 | 58.06 | 0.3930 | 1146.0 | 923.5 | |
| 0.00 | 2.46 | 0.00 | 1.33 | 8.00 | 99.47 | -19.78 | 59.46 | 0.3909 | -942.0 | -696.2 | |
| 1.02 | 303.27 | 0.55 | 165.22 | 9.24 | 99.21 | -20.04 | 57.09 | 0.4046 | 724.7 | 424.6 | |
| 12.41 | -31.00 | 6.74 | -31.00 | 9.73 | 99.06 | -20.20 | 56.28 | 0.4109 | 1095.4 | 999999 | |
| 0.00 | 2.38 | 0.00 | 1.28 | 8.04 | 99.12 | -20.13 | 59.81 | 0.3960 | -663.0 | -469.2 | |
| 3.23 | -31.00 | 1.76 | -31.00 | 9.44 | 98.56 | -20.69 | 57.51 | 0.4150 | 717.2 | 999999 | |
| 3.06 | -31.00 | 1.67 | -31.00 | 9.68 | 98.33 | -20.93 | 57.29 | 0.4203 | 772.1 | 999999 | |
| 57.63 | -31.00 | 31.40 | -31.00 | 9.14 | 98.13 | -21.12 | 58.63 | 0.4184 | 1289.1 | 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. | |