| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.13 | 23.29 | 2.14 | 12.23 | -12.12 | 138.77 | 2.96 | 189.05 | 0.3282 | 39.5 | 12.0 | |
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back to the solar disc SDO HMI 2014-10-04 17:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.61 | -13.66 | 143.82 | 8.01 | 201.48 | 0.3716 | 835.0 | 648.9 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -15.48 | 140.79 | 4.98 | 192.59 | 0.3854 | 701.0 | 664.0 | |
| 1.93 | 8.44 | 1.00 | 4.38 | -10.04 | 140.41 | 4.60 | 195.50 | 0.2971 | 1200.3 | 798.9 | |
| 2.20 | -3.00 | 1.14 | -3.00 | -10.17 | 140.35 | 4.54 | 195.19 | 0.2989 | 926.8 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -9.94 | 140.20 | 4.39 | 194.89 | 0.2946 | 954.0 | 868.5 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -15.40 | 139.32 | 3.51 | 188.99 | 0.3797 | -935.0 | -773.1 | |
| 0.00 | 1.67 | 0.00 | 0.91 | -18.60 | 138.71 | 2.90 | 186.45 | 0.4293 | -847.0 | -715.7 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -8.84 | 138.30 | 2.49 | 189.20 | 0.2698 | 763.0 | 664.3 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -10.34 | 138.28 | 2.47 | 188.31 | 0.2946 | 1012.0 | 749.4 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -14.97 | 138.04 | 2.23 | 185.86 | 0.3702 | -862.0 | -661.7 | |
| 0.00 | 1.67 | 0.00 | 0.89 | -14.68 | 137.91 | 2.10 | 185.61 | 0.3652 | -853.0 | -710.9 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -11.77 | 135.87 | 0.06 | 180.19 | 0.3156 | -953.0 | -757.9 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -10.58 | 133.92 | -1.89 | 173.72 | 0.2974 | -791.0 | -684.4 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -11.37 | 132.20 | -3.61 | 168.65 | 0.3149 | -722.0 | -608.2 | |
| 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. | |