| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.26 | 0.00 | 10.36 | -16.82 | 104.82 | 16.84 | 215.27 | 0.4890 | 84.9 | 117.5 | |
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back to the solar disc SDO HMI 2014-10-08 08:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.35 | -11.39 | 110.64 | 22.67 | 231.92 | 0.4819 | 604.0 | 515.6 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -13.37 | 110.49 | 22.51 | 228.56 | 0.4990 | 846.0 | 666.5 | |
| 0.00 | 1.49 | 0.00 | 0.87 | -16.45 | 110.46 | 22.48 | 224.05 | 0.5296 | 729.0 | 561.5 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -15.90 | 110.36 | 22.38 | 224.68 | 0.5229 | 577.0 | 523.6 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -12.88 | 109.25 | 21.27 | 227.72 | 0.4800 | 679.0 | 508.3 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -14.22 | 109.37 | 21.40 | 225.83 | 0.4951 | 653.0 | 576.6 | |
| 0.00 | 2.02 | 0.00 | 1.17 | -18.21 | 108.01 | 20.03 | 218.51 | 0.5247 | 747.0 | 598.5 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -18.87 | 108.05 | 20.08 | 217.76 | 0.5326 | 691.0 | 496.4 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -15.54 | 107.29 | 19.31 | 221.00 | 0.4876 | 789.0 | 600.2 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -9.28 | 102.69 | 14.71 | 223.36 | 0.3667 | -816.0 | -649.2 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -19.55 | 99.60 | 11.62 | 203.61 | 0.4760 | -552.0 | -443.8 | |
| 0.00 | 1.76 | 0.00 | 0.98 | -19.08 | 99.27 | 11.30 | 203.44 | 0.4674 | -680.0 | -485.0 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -19.19 | 98.47 | 10.50 | 201.85 | 0.4642 | -796.0 | -579.3 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -19.05 | 97.92 | 9.94 | 200.92 | 0.4590 | -848.0 | -740.0 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -23.62 | 93.97 | 5.99 | 190.86 | 0.5097 | -525.0 | -370.9 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -19.84 | 89.44 | 1.47 | 183.13 | 0.4434 | -740.0 | -618.2 | |
| 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. | |