SDO HMI 2011-12-18 18:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.99 | 0.00 | 9.64 | -18.98 | 322.45 | 30.67 | 237.56 | 0.5743 | -340.7 | -307.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 1.00 | -17.29 | 325.88 | 34.09 | 242.47 | 0.6058 | 744.0 | 663.8 | |
| 0.00 | 0.85 | 0.00 | 0.52 | -16.60 | 324.12 | 32.33 | 242.47 | 0.5802 | 753.0 | 596.1 | |
| 0.00 | 0.68 | 0.00 | 0.41 | -17.51 | 323.09 | 31.30 | 240.35 | 0.5723 | -696.0 | -603.6 | |
| 0.00 | 1.02 | 0.00 | 0.61 | -17.17 | 322.88 | 31.09 | 240.75 | 0.5677 | -330.0 | -369.7 | |
| 0.00 | 0.85 | 0.00 | 0.51 | -18.59 | 322.94 | 31.15 | 238.54 | 0.5771 | 650.0 | 514.0 | |
| 0.00 | 1.36 | 0.00 | 0.85 | -23.16 | 323.42 | 31.63 | 232.11 | 0.6133 | -576.0 | -513.8 | |
| 0.00 | 0.26 | 0.00 | 0.15 | -17.92 | 322.16 | 30.37 | 239.03 | 0.5632 | -823.0 | -742.7 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -17.21 | 321.95 | 30.17 | 240.03 | 0.5563 | -688.0 | -480.4 | |
| 0.00 | 1.36 | 0.00 | 0.82 | -20.18 | 322.11 | 30.32 | 235.45 | 0.5776 | -715.0 | -608.9 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -18.48 | 321.51 | 29.72 | 237.64 | 0.5589 | -680.0 | -441.8 | |
| 0.00 | 0.85 | 0.00 | 0.51 | -19.19 | 321.65 | 29.86 | 236.62 | 0.5653 | -582.0 | -450.6 | |
| 0.00 | 3.06 | 0.00 | 1.83 | -19.07 | 321.55 | 29.77 | 236.74 | 0.5633 | -732.0 | -630.3 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -21.46 | 319.60 | 27.81 | 231.38 | 0.5579 | -754.0 | -683.3 | |
| 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. | |