SDO HMI 2011-12-16 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 |
| 47.37 | 287.85 | 29.63 | 179.81 | -18.35 | 352.10 | 33.96 | 240.48 | 0.6117 | 937.9 | 382.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.68 | 0.00 | 0.43 | -18.68 | 353.19 | 35.05 | 240.66 | 0.6264 | -267.0 | -259.5 | |
| 6.21 | 26.03 | 3.91 | 16.46 | -19.21 | 352.52 | 34.38 | 239.47 | 0.6214 | 760.0 | 117.8 | |
| 41.16 | 244.18 | 25.72 | 152.51 | -18.16 | 352.20 | 34.06 | 240.83 | 0.6118 | 1246.0 | 404.9 | |
| 0.00 | 3.32 | 0.00 | 2.06 | -19.94 | 351.00 | 32.86 | 237.39 | 0.6078 | 706.0 | 584.5 | |
| 0.00 | 1.19 | 0.00 | 0.74 | -19.48 | 350.81 | 32.68 | 237.95 | 0.6028 | 999.0 | 846.4 | |
| 0.00 | 1.96 | 0.00 | 1.21 | -20.04 | 350.68 | 32.55 | 237.03 | 0.6048 | 825.0 | 683.9 | |
| 0.00 | 1.45 | 0.00 | 0.89 | -19.51 | 350.41 | 32.28 | 237.62 | 0.5983 | 817.0 | 684.7 | |
| 0.00 | 1.11 | 0.00 | 0.69 | -20.29 | 350.52 | 32.38 | 236.54 | 0.6044 | 198.0 | 294.8 | |
| 0.00 | 2.13 | 0.00 | 1.31 | -19.45 | 350.18 | 32.04 | 237.55 | 0.5951 | 844.0 | 764.3 | |
| 0.00 | 1.28 | 0.00 | 0.77 | -17.66 | 349.69 | 31.56 | 239.97 | 0.5782 | -469.0 | -353.5 | |
| 0.00 | 0.85 | 0.00 | 0.52 | -18.18 | 349.76 | 31.63 | 239.20 | 0.5822 | -549.0 | -420.9 | |
| 0.00 | 0.94 | 0.00 | 0.59 | -21.93 | 350.55 | 32.41 | 234.18 | 0.6155 | 649.0 | 541.2 | |
| 0.00 | 0.94 | 0.00 | 0.57 | -18.53 | 349.18 | 31.04 | 238.24 | 0.5772 | -397.0 | -338.4 | |
| 0.00 | 1.79 | 0.00 | 1.06 | -20.80 | 345.78 | 27.65 | 231.93 | 0.5531 | 669.0 | 602.1 | |
| 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. | |