SDO HMI 2011-12-14 23:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.28 | 21.21 | 0.69 | 11.76 | -19.66 | 322.82 | -18.91 | 136.58 | 0.4455 | -44.0 | -121.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.73 | -16.58 | 326.29 | -15.44 | 136.80 | 0.3743 | 1010.0 | 844.6 | |
| 0.00 | 1.79 | 0.00 | 0.99 | -21.89 | 325.76 | -15.96 | 144.65 | 0.4430 | -874.0 | -644.5 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -15.75 | 326.29 | -15.44 | 135.18 | 0.3650 | 845.0 | 669.5 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -15.93 | 326.28 | -15.45 | 135.52 | 0.3672 | 770.0 | 616.1 | |
| 0.00 | 2.72 | 0.00 | 1.45 | -16.30 | 326.18 | -15.54 | 136.08 | 0.3724 | 832.0 | 539.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -16.02 | 326.14 | -15.59 | 135.46 | 0.3698 | 811.0 | 647.6 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -14.98 | 324.50 | -17.22 | 130.57 | 0.3782 | 718.0 | 475.1 | |
| 1.28 | 1.79 | 0.69 | 0.97 | -16.72 | 323.77 | -17.96 | 132.88 | 0.4048 | -725.5 | -672.7 | |
| 0.00 | 1.28 | 0.00 | 0.72 | -23.47 | 322.94 | -18.79 | 142.54 | 0.4877 | -736.0 | -573.9 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -18.38 | 322.38 | -19.35 | 133.86 | 0.4379 | -783.0 | -609.4 | |
| 0.00 | 1.28 | 0.00 | 0.70 | -18.07 | 322.12 | -19.61 | 132.95 | 0.4377 | -1005.0 | -856.1 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -22.47 | 319.50 | -22.22 | 136.61 | 0.5107 | -739.0 | -617.6 | |
| 0.00 | 2.98 | 0.00 | 1.79 | -26.59 | 317.71 | -24.02 | 140.12 | 0.5699 | -214.0 | -286.3 | |
| 0.00 | 2.13 | 0.00 | 1.22 | -20.19 | 318.37 | -23.36 | 131.78 | 0.5011 | -737.0 | -632.7 | |
| 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. | |