| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.74 | 79.96 | 17.82 | 43.42 | -17.71 | 100.15 | 11.60 | 207.87 | 0.4106 | 224.9 | -36.2 | |
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back to the solar disc SDO HMI 2011-11-09 13:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.93 | 47.39 | 1.60 | 25.88 | -17.85 | 101.63 | 13.09 | 210.72 | 0.4238 | 874.4 | 642.3 | |
| 1.46 | -1.00 | 0.80 | -1.00 | -17.59 | 101.23 | 12.69 | 210.28 | 0.4170 | 929.5 | 999999 | |
| 19.56 | -1.00 | 10.68 | -1.00 | -18.04 | 101.23 | 12.69 | 209.72 | 0.4231 | 1108.1 | 999999 | |
| 0.86 | -1.00 | 0.47 | -1.00 | -18.39 | 101.06 | 12.52 | 208.97 | 0.4266 | 577.1 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -17.48 | 99.95 | 11.41 | 207.85 | 0.4056 | -705.0 | -472.1 | |
| 0.00 | 2.15 | 0.00 | 1.16 | -17.15 | 99.26 | 10.72 | 206.80 | 0.3959 | -303.0 | -273.2 | |
| 0.00 | 3.71 | 0.00 | 2.00 | -17.24 | 98.92 | 10.38 | 205.96 | 0.3948 | -527.0 | -613.3 | |
| 0.86 | 4.57 | 0.47 | 2.47 | -17.78 | 98.67 | 10.12 | 204.80 | 0.4008 | -810.4 | -607.6 | |
| 0.00 | 1.29 | 0.00 | 0.70 | -17.15 | 98.60 | 10.06 | 205.37 | 0.3911 | -1066.0 | -909.1 | |
| 4.57 | 10.68 | 2.46 | 5.76 | -17.56 | 98.53 | 9.99 | 204.75 | 0.3966 | -911.5 | -795.0 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -16.95 | 98.08 | 9.54 | 204.45 | 0.3848 | -974.0 | -828.5 | |
| 2.50 | 6.12 | 1.34 | 3.27 | -16.57 | 97.88 | 9.33 | 204.41 | 0.3778 | -960.4 | -811.3 | |
| 0.00 | 2.15 | 0.00 | 1.16 | -17.04 | 97.90 | 9.36 | 203.93 | 0.3849 | -723.0 | -480.4 | |
| 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. | |