| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.38 | 299.09 | 29.08 | 183.48 | -18.37 | 352.14 | 32.35 | 239.39 | 0.5922 | 980.8 | 358.3 | |
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back to the solar disc SDO HMI 2011-12-16 15:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.25 | 282.06 | 5.10 | 173.18 | -19.19 | 352.52 | 32.72 | 238.40 | 0.6017 | 739.2 | 358.8 | |
| 39.13 | -1.00 | 23.98 | -1.00 | -18.14 | 352.18 | 32.39 | 239.78 | 0.5913 | 1291.2 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.52 | -20.14 | 351.21 | 31.42 | 236.05 | 0.5923 | 554.0 | 399.6 | |
| 0.00 | 0.77 | 0.00 | 0.47 | -19.76 | 351.02 | 31.23 | 236.47 | 0.5875 | 782.0 | 617.8 | |
| 0.00 | 1.19 | 0.00 | 0.73 | -19.92 | 351.02 | 31.22 | 236.23 | 0.5885 | 741.0 | 560.0 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -16.77 | 350.35 | 30.56 | 240.69 | 0.5605 | -603.0 | -466.9 | |
| 0.00 | 2.47 | 0.00 | 1.50 | -19.45 | 350.81 | 31.01 | 236.78 | 0.5830 | 958.0 | 726.5 | |
| 0.00 | 2.38 | 0.00 | 1.45 | -19.98 | 350.67 | 30.87 | 235.87 | 0.5848 | 770.0 | 646.0 | |
| 0.00 | 0.94 | 0.00 | 0.57 | -19.67 | 350.60 | 30.80 | 236.29 | 0.5819 | 863.0 | 723.7 | |
| 0.00 | 1.79 | 0.00 | 1.08 | -19.40 | 350.32 | 30.53 | 236.50 | 0.5768 | 758.0 | 668.0 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -19.46 | 350.12 | 30.32 | 236.24 | 0.5748 | 876.0 | 726.1 | |
| 0.00 | 2.04 | 0.00 | 1.22 | -17.73 | 349.67 | 29.87 | 238.63 | 0.5579 | -535.0 | -470.2 | |
| 0.00 | 0.68 | 0.00 | 0.42 | -21.59 | 350.44 | 30.65 | 233.31 | 0.5934 | 646.0 | 554.4 | |
| 0.00 | 1.28 | 0.00 | 0.76 | -18.44 | 349.23 | 29.44 | 237.14 | 0.5572 | -253.0 | -306.9 | |
| 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. | |