| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.84 | 66.42 | 17.38 | 37.52 | -25.23 | 85.32 | -1.57 | 177.01 | 0.4837 | -134.4 | 313.6 | |
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back to the solar disc SDO HMI 2011-11-09 16:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.10 | 3.62 | 1.74 | 2.03 | -24.53 | 86.70 | -0.19 | 179.63 | 0.4720 | 893.9 | 954.2 | |
| 3.79 | 14.56 | 2.16 | 8.27 | -26.06 | 86.50 | -0.39 | 179.29 | 0.4955 | 748.8 | 696.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -24.43 | 86.47 | -0.42 | 179.19 | 0.4705 | 898.0 | 583.9 | |
| 2.93 | 11.46 | 1.66 | 6.50 | -25.82 | 86.11 | -0.78 | 178.56 | 0.4919 | 917.2 | 708.1 | |
| 1.12 | -4.00 | 0.63 | -4.00 | -25.61 | 86.04 | -0.85 | 178.43 | 0.4889 | 809.7 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -23.96 | 85.89 | -1.00 | 178.02 | 0.4635 | 658.0 | 518.5 | |
| 0.00 | 3.70 | 0.00 | 2.11 | -25.85 | 85.78 | -1.11 | 177.96 | 0.4926 | 236.0 | 334.9 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -24.53 | 85.72 | -1.17 | 177.74 | 0.4724 | 794.0 | 606.9 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -26.02 | 85.48 | -1.41 | 177.42 | 0.4954 | 652.0 | 431.8 | |
| 15.16 | 20.59 | 8.49 | 11.53 | -24.20 | 84.33 | -2.56 | 174.98 | 0.4686 | -1044.4 | -605.2 | |
| 0.00 | 1.72 | 0.00 | 0.98 | -25.55 | 84.07 | -2.82 | 174.77 | 0.4897 | -614.0 | -472.7 | |
| 1.90 | 2.76 | 1.08 | 1.57 | -25.99 | 83.59 | -3.30 | 174.01 | 0.4971 | -586.9 | -597.8 | |
| 2.84 | 4.05 | 1.62 | 2.30 | -25.76 | 83.37 | -3.52 | 173.54 | 0.4939 | -907.5 | -728.1 | |
| 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. | |