SDO HMI 2014-01-13 14:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95.70 | 463.61 | 49.29 | 239.00 | -16.50 | 13.13 | -10.66 | 140.12 | 0.2774 | 1027.1 | 371.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.51 | 0.00 | 0.26 | -14.79 | 14.53 | -9.26 | 139.40 | 0.2402 | -786.0 | -698.3 | |
| 60.86 | 293.57 | 31.30 | 150.94 | -16.59 | 13.82 | -9.97 | 142.01 | 0.2708 | 1377.0 | 444.4 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -15.76 | 12.80 | -10.99 | 137.27 | 0.2715 | 706.0 | 590.7 | |
| 0.00 | 1.78 | 0.00 | 0.92 | -15.48 | 12.69 | -11.10 | 136.27 | 0.2696 | 745.0 | 627.2 | |
| 7.39 | 156.73 | 3.82 | 81.03 | -16.75 | 12.56 | -11.23 | 139.12 | 0.2863 | 1064.6 | 314.8 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -14.88 | 12.45 | -11.34 | 134.01 | 0.2655 | -734.0 | -384.5 | |
| 27.45 | -5.00 | 14.17 | -5.00 | -16.26 | 12.27 | -11.52 | 137.24 | 0.2836 | 1291.9 | 999999 | |
| 0.00 | 1.95 | 0.00 | 1.03 | -15.46 | 6.86 | -16.93 | 124.84 | 0.3435 | -947.0 | -682.9 | |
| 0.00 | 0.42 | 0.00 | 0.22 | -15.79 | 6.51 | -17.28 | 125.12 | 0.3510 | -712.0 | -519.4 | |
| 0.00 | 3.14 | 0.00 | 1.69 | -18.57 | 5.16 | -18.63 | 129.41 | 0.3937 | -798.0 | -677.0 | |
| 0.00 | 0.42 | 0.00 | 0.23 | -18.44 | 4.84 | -18.95 | 128.70 | 0.3964 | -457.0 | -418.2 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -10.10 | 3.73 | -20.06 | 107.15 | 0.3550 | -788.0 | -572.9 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -20.09 | 2.46 | -21.33 | 128.90 | 0.4407 | -806.0 | -614.2 | |
| 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. | |