| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.88 | 72.78 | 14.50 | 37.79 | 17.77 | 214.54 | -6.04 | 19.35 | 0.3010 | 435.6 | 351.6 | |
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back to the solar disc SDO HMI 2011-11-26 20:58:56 UT
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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 | 0.35 | 17.59 | 218.18 | -2.41 | 8.21 | 0.2817 | 802.0 | 649.2 | |
| 0.00 | 3.34 | 0.00 | 1.72 | 17.92 | 218.08 | -2.51 | 8.35 | 0.2875 | 789.0 | 624.3 | |
| 0.00 | 2.05 | 0.00 | 1.06 | 17.43 | 217.90 | -2.68 | 9.23 | 0.2798 | 877.0 | 773.1 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 17.49 | 217.68 | -2.90 | 9.93 | 0.2814 | 865.0 | 731.6 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.34 | 217.68 | -2.90 | 10.02 | 0.2789 | 727.0 | 607.8 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.65 | 217.55 | -3.03 | 10.25 | 0.2844 | 920.0 | 679.9 | |
| 6.07 | 9.58 | 3.12 | 4.92 | 16.57 | 217.08 | -3.51 | 12.68 | 0.2682 | -1060.4 | -766.1 | |
| 0.00 | 4.11 | 0.00 | 2.11 | 16.54 | 216.74 | -3.85 | 13.89 | 0.2690 | -792.0 | -659.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 20.81 | 216.26 | -4.33 | 12.01 | 0.3401 | 839.0 | 639.4 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 18.26 | 215.76 | -4.82 | 15.44 | 0.3011 | -836.0 | -556.6 | |
| 0.00 | 2.99 | 0.00 | 1.58 | 21.09 | 215.58 | -5.00 | 13.61 | 0.3471 | 734.0 | 681.7 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 16.54 | 215.69 | -4.90 | 17.47 | 0.2738 | -929.0 | -765.1 | |
| 0.00 | 2.05 | 0.00 | 1.05 | 15.47 | 214.76 | -5.83 | 22.02 | 0.2621 | -847.0 | -694.3 | |
| 1.97 | 42.08 | 1.03 | 21.93 | 18.07 | 213.17 | -7.41 | 23.22 | 0.3124 | 953.8 | 729.9 | |
| 19.84 | -14.00 | 10.35 | -14.00 | 18.01 | 212.83 | -7.75 | 24.25 | 0.3137 | 1035.7 | 999999 | |
| 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. | |