| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.37 | 170.23 | 22.04 | 119.23 | 14.39 | 251.96 | 43.46 | 289.22 | 0.7077 | -629.4 | -322.0 | |
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back to the solar disc SDO HMI 2011-11-27 18:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.33 | 157.15 | 18.54 | 110.61 | 14.29 | 252.43 | 43.93 | 288.91 | 0.7130 | -1049.4 | -361.5 | |
| 3.42 | -1.00 | 2.37 | -1.00 | 13.88 | 251.66 | 43.15 | 288.57 | 0.7028 | -804.5 | 999999 | |
| 1.62 | -1.00 | 1.13 | -1.00 | 14.58 | 251.70 | 43.19 | 289.53 | 0.7052 | -804.0 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.89 | 16.42 | 251.21 | 42.70 | 292.23 | 0.7051 | -554.0 | -506.9 | |
| 0.00 | 1.37 | 0.00 | 0.95 | 16.58 | 251.17 | 42.66 | 292.46 | 0.7052 | -677.0 | -522.6 | |
| 0.00 | 0.60 | 0.00 | 0.42 | 18.05 | 251.60 | 43.09 | 294.30 | 0.7150 | -445.0 | -398.0 | |
| 0.00 | 1.11 | 0.00 | 0.78 | 17.31 | 251.29 | 42.79 | 293.42 | 0.7091 | -633.0 | -594.3 | |
| 0.00 | 1.28 | 0.00 | 0.88 | 17.98 | 249.85 | 41.34 | 294.91 | 0.6951 | -281.0 | -377.1 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 11.70 | 247.63 | 39.12 | 286.65 | 0.6472 | 761.0 | 660.6 | |
| 0.00 | 1.20 | 0.00 | 0.78 | 17.08 | 246.23 | 37.72 | 295.24 | 0.6488 | 531.0 | 419.6 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 17.56 | 244.63 | 36.12 | 296.76 | 0.6317 | 525.0 | 456.4 | |
| 0.00 | 1.54 | 0.00 | 0.94 | 10.63 | 242.94 | 34.43 | 286.55 | 0.5820 | 783.0 | 554.8 | |
| 0.00 | 1.88 | 0.00 | 1.18 | 17.70 | 243.63 | 35.12 | 297.51 | 0.6202 | 811.0 | 630.0 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 17.03 | 243.03 | 34.52 | 296.83 | 0.6095 | 654.0 | 609.4 | |
| 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. | |