| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 103.17 | 667.19 | 252.96 | 2005.40 | 18.91 | 106.70 | -79.07 | 71.54 | 0.9787 | 185.1 | 85.6 | |
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back to the solar disc SDO HMI 2011-11-02 04:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.34 | 6.58 | 5.13 | 14.41 | 22.20 | 108.03 | -77.74 | 68.19 | 0.9755 | -573.6 | -401.9 | |
| 14.89 | 587.29 | 27.31 | 1714.22 | 18.56 | 110.81 | -74.95 | 71.92 | 0.9643 | -710.2 | 49.4 | |
| 19.65 | -2.00 | 38.65 | -2.00 | 19.08 | 109.73 | -76.03 | 71.39 | 0.9689 | -376.5 | 999999 | |
| 12.20 | -2.00 | 24.91 | -2.00 | 18.98 | 109.20 | -76.57 | 71.49 | 0.9710 | 277.6 | 999999 | |
| 2.08 | 49.42 | 6.03 | 157.72 | 21.22 | 104.61 | -81.15 | 69.19 | 0.9862 | 562.8 | 452.1 | |
| 0.00 | 0.61 | 0.00 | 2.22 | 21.66 | 102.29 | -83.47 | 68.69 | 0.9917 | -191.0 | -59.0 | |
| 11.94 | -5.00 | 41.79 | -5.00 | 20.88 | 102.97 | -82.79 | 69.50 | 0.9903 | 620.4 | 999999 | |
| 9.43 | -2.00 | 21.41 | -2.00 | 18.37 | 107.65 | -78.12 | 72.12 | 0.9768 | 270.3 | 999999 | |
| 6.75 | -2.00 | 14.89 | -2.00 | 18.17 | 107.96 | -77.81 | 72.33 | 0.9757 | -180.3 | 999999 | |
| 3.20 | -2.00 | 9.14 | -2.00 | 19.55 | 104.86 | -80.90 | 70.88 | 0.9856 | 515.1 | 999999 | |
| 3.55 | -2.00 | 9.96 | -2.00 | 19.00 | 105.07 | -80.69 | 71.45 | 0.9850 | 684.8 | 999999 | |
| 7.62 | -2.00 | 27.18 | -2.00 | 19.46 | 102.76 | -83.00 | 70.92 | 0.9909 | 640.5 | 999999 | |
| 4.33 | -2.00 | 12.35 | -2.00 | 18.26 | 104.83 | -80.93 | 72.20 | 0.9857 | 866.7 | 999999 | |
| 3.98 | -2.00 | 10.95 | -2.00 | 17.76 | 105.26 | -80.50 | 72.71 | 0.9846 | 474.2 | 999999 | |
| 1.21 | -2.00 | 3.26 | -2.00 | 17.62 | 105.53 | -80.24 | 72.86 | 0.9838 | -159.5 | 999999 | |
| 0.00 | 6.32 | 0.00 | 28.48 | 18.32 | 100.99 | -84.77 | 72.01 | 0.9945 | 471.0 | 478.5 | |
| 0.00 | 16.97 | 0.00 | 88.35 | 17.42 | 100.29 | -85.47 | 72.88 | 0.9957 | 324.0 | 178.0 | |
| 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. | |