SDO HMI 2014-12-01 14:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.58 | 443.97 | 34.87 | 239.47 | 16.68 | 110.04 | 17.38 | 313.79 | 0.3979 | -916.0 | -335.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.58 | 423.04 | 34.87 | 228.36 | 16.63 | 110.27 | 17.61 | 313.26 | 0.3997 | -1558.6 | -393.8 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 17.88 | 107.62 | 14.95 | 320.09 | 0.3843 | 653.0 | 547.3 | |
| 0.00 | 3.50 | 0.00 | 1.87 | 17.45 | 106.84 | 14.18 | 320.78 | 0.3711 | 738.0 | 661.9 | |
| 0.00 | 3.42 | 0.00 | 1.82 | 17.72 | 106.83 | 14.17 | 321.29 | 0.3744 | 966.0 | 783.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 17.05 | 106.68 | 14.02 | 320.36 | 0.3646 | 661.0 | 561.4 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 18.25 | 106.75 | 14.08 | 322.37 | 0.3801 | 743.0 | 435.8 | |
| 0.00 | 0.51 | 0.00 | 0.27 | 17.91 | 106.62 | 13.96 | 322.02 | 0.3746 | 719.0 | 739.2 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 17.11 | 105.32 | 12.65 | 323.27 | 0.3516 | 1057.0 | 835.5 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 17.27 | 104.76 | 12.09 | 324.76 | 0.3483 | 965.0 | 915.2 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 16.13 | 104.28 | 11.61 | 323.79 | 0.3288 | 764.0 | 635.2 | |
| 0.00 | 2.65 | 0.00 | 1.40 | 17.36 | 104.20 | 11.53 | 326.17 | 0.3443 | 947.0 | 736.2 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 19.60 | 102.92 | 10.25 | 332.49 | 0.3646 | 743.0 | 680.2 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 19.42 | 102.02 | 9.35 | 334.34 | 0.3553 | 732.0 | 574.4 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 19.39 | 101.79 | 9.12 | 334.83 | 0.3533 | 812.0 | 688.7 | |
| 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. | |