| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.04 | 281.32 | 28.25 | 194.38 | 17.43 | 223.09 | -41.99 | 66.60 | 0.6978 | -509.5 | -240.2 | |
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back to the solar disc SDO HMI 2011-11-23 11:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.77 | 19.08 | 223.86 | -41.23 | 64.02 | 0.6952 | -547.0 | -517.5 | |
| 0.00 | 1.88 | 0.00 | 1.31 | 18.76 | 223.16 | -41.92 | 64.75 | 0.7019 | -511.0 | -426.6 | |
| 35.21 | 257.01 | 24.16 | 177.08 | 17.40 | 223.39 | -41.69 | 66.53 | 0.6943 | -985.9 | -290.8 | |
| 1.03 | -3.00 | 0.71 | -3.00 | 17.97 | 222.72 | -42.36 | 65.99 | 0.7040 | -695.1 | 999999 | |
| 3.34 | -3.00 | 2.34 | -3.00 | 17.90 | 222.27 | -42.81 | 66.26 | 0.7088 | -655.1 | 999999 | |
| 0.00 | 2.74 | 0.00 | 1.91 | 16.17 | 222.13 | -42.95 | 68.68 | 0.7048 | -531.0 | -387.4 | |
| 0.00 | 0.94 | 0.00 | 0.68 | 19.67 | 220.79 | -44.29 | 64.44 | 0.7312 | 577.0 | 454.2 | |
| 0.00 | 5.31 | 0.00 | 3.74 | 16.47 | 221.54 | -43.54 | 68.47 | 0.7125 | 402.0 | 215.8 | |
| 0.00 | 3.08 | 0.00 | 2.19 | 17.23 | 221.32 | -43.76 | 67.51 | 0.7174 | 484.0 | 489.7 | |
| 1.46 | 2.14 | 1.04 | 1.53 | 16.11 | 220.70 | -44.39 | 69.22 | 0.7211 | 684.6 | 501.9 | |
| 0.00 | 1.54 | 0.00 | 1.11 | 16.81 | 220.27 | -44.81 | 68.42 | 0.7279 | 707.0 | 645.6 | |
| 0.00 | 1.46 | 0.00 | 1.05 | 16.38 | 220.31 | -44.77 | 68.98 | 0.7262 | 792.0 | 672.5 | |
| 0.00 | 1.03 | 0.00 | 0.75 | 18.37 | 219.60 | -45.49 | 66.57 | 0.7399 | 648.0 | 544.4 | |
| 0.00 | 0.43 | 0.00 | 0.31 | 16.16 | 219.99 | -45.10 | 69.38 | 0.7293 | 454.0 | 514.2 | |
| 0.00 | 0.43 | 0.00 | 0.31 | 16.79 | 219.57 | -45.51 | 68.66 | 0.7356 | 471.0 | 491.8 | |
| 0.00 | 1.11 | 0.00 | 0.82 | 17.59 | 219.19 | -45.90 | 67.73 | 0.7420 | 580.0 | 476.5 | |
| 0.00 | 1.11 | 0.00 | 0.82 | 17.40 | 219.16 | -45.92 | 67.98 | 0.7418 | 591.0 | 508.2 | |
| 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. | |