SDO HMI 2014-10-05 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.86 | 245.76 | 30.54 | 131.77 | -13.34 | 121.47 | -10.48 | 152.54 | 0.3839 | 516.9 | 258.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.86 | 210.68 | 23.44 | 112.63 | -13.29 | 122.17 | -9.78 | 153.92 | 0.3775 | 1288.2 | 355.7 | |
| 0.00 | 1.67 | 0.00 | 0.90 | -13.60 | 121.09 | -10.86 | 151.86 | 0.3899 | 845.0 | 545.1 | |
| 1.05 | 1.76 | 0.57 | 0.95 | -13.30 | 119.97 | -11.97 | 149.08 | 0.3946 | 929.1 | 845.8 | |
| 0.00 | 1.49 | 0.00 | 0.80 | -13.12 | 119.70 | -12.25 | 148.25 | 0.3943 | 967.0 | 734.8 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -14.46 | 119.59 | -12.35 | 149.80 | 0.4135 | -886.0 | -709.9 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -13.19 | 119.60 | -12.35 | 148.14 | 0.3961 | 326.0 | 453.6 | |
| 0.00 | 2.02 | 0.00 | 1.11 | -15.10 | 117.41 | -14.53 | 146.45 | 0.4402 | -724.0 | -598.2 | |
| 2.11 | 7.12 | 1.15 | 3.88 | -13.38 | 117.24 | -14.70 | 143.77 | 0.4196 | -1007.0 | -823.1 | |
| 0.79 | 2.81 | 0.43 | 1.53 | -13.13 | 117.07 | -14.88 | 143.09 | 0.4180 | -1038.6 | -841.4 | |
| 9.05 | 12.66 | 4.95 | 6.92 | -13.33 | 116.67 | -15.27 | 142.66 | 0.4244 | -987.7 | -697.1 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -13.73 | 116.13 | -15.81 | 142.28 | 0.4345 | -773.0 | -704.4 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -15.61 | 115.63 | -16.31 | 144.02 | 0.4624 | -850.0 | -630.8 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -14.02 | 115.11 | -16.83 | 140.96 | 0.4479 | -596.0 | -528.9 | |
| 0.00 | 0.53 | 0.00 | 0.29 | -15.22 | 114.76 | -17.19 | 142.06 | 0.4657 | -547.0 | -483.8 | |
| 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. | |