SDO HMI 2011-11-25 11:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.26 | 53.51 | 14.33 | 30.29 | 17.79 | 214.30 | -24.42 | 54.46 | 0.4857 | 317.6 | 169.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.80 | 0.00 | 0.99 | 18.11 | 217.66 | -21.07 | 50.11 | 0.4471 | 761.0 | 652.5 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 18.54 | 217.23 | -21.49 | 49.87 | 0.4562 | 679.0 | 741.0 | |
| 0.00 | 1.97 | 0.00 | 1.11 | 19.26 | 215.54 | -23.18 | 50.61 | 0.4829 | 775.0 | 645.8 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 19.45 | 215.44 | -23.28 | 50.40 | 0.4856 | 681.0 | 580.1 | |
| 8.30 | 11.81 | 4.65 | 6.61 | 17.25 | 215.39 | -23.34 | 54.33 | 0.4677 | -842.0 | -678.4 | |
| 0.00 | 2.65 | 0.00 | 1.49 | 17.77 | 215.01 | -23.71 | 53.79 | 0.4766 | -937.0 | -770.5 | |
| 0.86 | 3.60 | 0.48 | 2.03 | 18.05 | 214.80 | -23.92 | 53.53 | 0.4815 | -785.5 | -579.8 | |
| 0.00 | 2.40 | 0.00 | 1.35 | 17.43 | 214.85 | -23.87 | 54.57 | 0.4758 | -468.0 | -338.2 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 18.16 | 213.89 | -24.83 | 54.26 | 0.4936 | 646.0 | 486.8 | |
| 0.00 | 2.14 | 0.00 | 1.22 | 17.66 | 213.59 | -25.13 | 55.43 | 0.4935 | 741.0 | 572.0 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 17.82 | 213.47 | -25.26 | 55.29 | 0.4962 | 1028.0 | 861.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 16.95 | 213.49 | -25.23 | 56.79 | 0.4894 | 754.0 | 559.0 | |
| 3.60 | 21.83 | 2.05 | 12.48 | 17.66 | 213.21 | -25.51 | 55.80 | 0.4982 | 1008.8 | 758.0 | |
| 12.50 | -13.00 | 7.15 | -13.00 | 17.84 | 213.01 | -25.71 | 55.68 | 0.5021 | 894.2 | 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. | |