| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.53 | 48.85 | 20.25 | 56.88 | 16.75 | 297.82 | 64.06 | 287.83 | 0.9053 | 8.7 | -0.5 | |
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back to the solar disc SDO HMI 2011-11-25 20:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.93 | 17.46 | 8.97 | 22.72 | 16.42 | 300.79 | 67.03 | 287.13 | 0.9258 | -462.5 | -44.5 | |
| 0.00 | 2.31 | 0.00 | 2.91 | 15.79 | 300.20 | 66.44 | 286.50 | 0.9216 | -357.0 | -288.9 | |
| 0.00 | 1.20 | 0.00 | 1.39 | 16.06 | 297.84 | 64.08 | 287.04 | 0.9058 | -480.0 | -365.1 | |
| 0.00 | 0.77 | 0.00 | 0.89 | 16.24 | 297.88 | 64.12 | 287.23 | 0.9062 | -155.0 | -171.6 | |
| 0.00 | 2.48 | 0.00 | 2.82 | 16.94 | 297.18 | 63.42 | 288.08 | 0.9018 | -508.0 | -466.0 | |
| 0.00 | 1.03 | 0.00 | 1.10 | 16.15 | 295.44 | 61.68 | 287.42 | 0.8881 | 280.0 | 196.6 | |
| 1.54 | 2.05 | 1.66 | 2.21 | 16.64 | 295.64 | 61.88 | 287.94 | 0.8901 | 271.6 | 261.3 | |
| 0.00 | 1.45 | 0.00 | 1.55 | 16.37 | 295.23 | 61.47 | 287.69 | 0.8867 | 282.0 | 267.4 | |
| 3.25 | 4.79 | 3.48 | 5.14 | 17.32 | 295.31 | 61.55 | 288.75 | 0.8883 | 336.1 | 104.7 | |
| 0.00 | 3.51 | 0.00 | 3.71 | 16.84 | 295.03 | 61.27 | 288.24 | 0.8857 | 458.0 | 336.7 | |
| 0.00 | 1.28 | 0.00 | 1.38 | 17.63 | 295.43 | 61.66 | 289.08 | 0.8895 | 269.0 | 194.8 | |
| 2.22 | 2.91 | 2.36 | 3.09 | 17.80 | 295.00 | 61.24 | 289.33 | 0.8864 | 542.4 | 471.1 | |
| 3.59 | 5.90 | 3.78 | 6.21 | 17.43 | 294.72 | 60.96 | 288.96 | 0.8839 | 571.7 | 526.4 | |
| 0.00 | 1.71 | 0.00 | 1.76 | 17.08 | 294.01 | 60.25 | 288.66 | 0.8780 | -448.0 | -387.1 | |
| 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. | |