| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.47 | 44.10 | 12.42 | 26.81 | -18.01 | 77.93 | -30.64 | 123.00 | 0.5798 | 119.1 | 12.9 | |
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back to the solar disc SDO HMI 2011-12-05 08:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.71 | -17.25 | 80.29 | -28.28 | 123.71 | 0.5461 | 727.0 | 395.9 | |
| 9.30 | 16.21 | 5.55 | 9.68 | -17.44 | 79.34 | -29.23 | 123.21 | 0.5591 | 935.6 | 678.2 | |
| 0.00 | 1.28 | 0.00 | 0.77 | -17.38 | 78.82 | -29.76 | 122.69 | 0.5650 | 846.0 | 632.7 | |
| 2.30 | 3.50 | 1.38 | 2.10 | -17.25 | 78.59 | -29.99 | 122.32 | 0.5670 | 791.4 | 693.4 | |
| 0.00 | 1.11 | 0.00 | 0.67 | -17.84 | 78.48 | -30.09 | 123.15 | 0.5723 | 498.0 | 402.6 | |
| 0.00 | 1.96 | 0.00 | 1.20 | -18.69 | 77.44 | -31.13 | 123.63 | 0.5904 | -722.0 | -584.2 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -18.32 | 76.97 | -31.60 | 122.71 | 0.5935 | 489.0 | 236.7 | |
| 2.90 | 3.41 | 1.79 | 2.11 | -18.75 | 76.81 | -31.77 | 123.24 | 0.5983 | -770.1 | -536.7 | |
| 1.45 | 12.03 | 0.90 | 7.45 | -18.57 | 76.63 | -31.95 | 122.83 | 0.5992 | -910.9 | -686.8 | |
| 3.33 | -9.00 | 2.06 | -9.00 | -18.76 | 76.44 | -32.13 | 122.97 | 0.6026 | -803.5 | 999999 | |
| 1.19 | -9.00 | 0.74 | -9.00 | -18.63 | 76.32 | -32.26 | 122.70 | 0.6032 | -789.0 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.90 | -18.29 | 75.91 | -32.66 | 121.90 | 0.6059 | -752.0 | -553.2 | |
| 0.00 | 1.02 | 0.00 | 0.64 | -18.79 | 75.73 | -32.85 | 122.51 | 0.6112 | -621.0 | -520.6 | |
| 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. | |