| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.96 | 27.52 | 2.05 | 14.41 | -12.15 | 139.28 | 1.27 | 183.88 | 0.3246 | 243.9 | 218.5 | |
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back to the solar disc SDO HMI 2014-10-04 13:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.51 | -13.22 | 143.66 | 5.65 | 195.84 | 0.3524 | 849.0 | 666.3 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -9.44 | 141.18 | 3.17 | 191.20 | 0.2818 | 704.0 | 454.7 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -16.54 | 140.73 | 2.72 | 186.62 | 0.3963 | 550.0 | 498.8 | |
| 0.00 | 2.20 | 0.00 | 1.18 | -15.89 | 140.69 | 2.68 | 186.72 | 0.3858 | 710.0 | 646.8 | |
| 1.49 | 10.55 | 0.77 | 5.46 | -10.03 | 140.42 | 2.41 | 188.26 | 0.2894 | 1141.3 | 874.5 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -16.12 | 140.45 | 2.43 | 186.04 | 0.3889 | 858.0 | 686.5 | |
| 1.85 | -5.00 | 0.96 | -5.00 | -10.16 | 140.24 | 2.23 | 187.59 | 0.2910 | 951.4 | 999999 | |
| 0.62 | -5.00 | 0.32 | -5.00 | -9.94 | 140.21 | 2.20 | 187.58 | 0.2873 | 1061.6 | 999999 | |
| 0.00 | 1.93 | 0.00 | 1.01 | -11.57 | 139.88 | 1.87 | 185.87 | 0.3138 | 768.0 | 691.7 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -15.49 | 138.42 | 0.40 | 181.03 | 0.3768 | -837.0 | -669.4 | |
| 0.00 | 2.29 | 0.00 | 1.22 | -14.88 | 137.95 | -0.06 | 179.83 | 0.3668 | -803.0 | -681.7 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -14.65 | 137.86 | -0.16 | 179.58 | 0.3631 | -1024.0 | -840.5 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -10.37 | 134.79 | -3.23 | 169.22 | 0.2973 | -860.0 | -694.7 | |
| 0.00 | 2.29 | 0.00 | 1.19 | -10.82 | 133.95 | -4.06 | 166.87 | 0.3074 | -681.0 | -555.0 | |
| 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. | |