SDO HMI 2014-08-21 15:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.94 | 162.39 | 17.38 | 93.90 | 16.44 | 27.96 | 30.07 | 290.76 | 0.5158 | -682.5 | -300.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.60 | 136.75 | 16.03 | 79.52 | 16.24 | 28.64 | 30.75 | 289.99 | 0.5244 | -1166.1 | -308.5 | |
| 2.34 | -1.00 | 1.35 | -1.00 | 16.33 | 28.17 | 30.29 | 290.36 | 0.5183 | -1137.2 | 999999 | |
| 0.00 | 2.79 | 0.00 | 1.59 | 17.54 | 26.52 | 28.64 | 293.50 | 0.5003 | -804.0 | -616.8 | |
| 0.00 | 1.71 | 0.00 | 0.97 | 16.90 | 26.38 | 28.49 | 292.34 | 0.4955 | -693.0 | -562.0 | |
| 0.00 | 5.03 | 0.00 | 2.87 | 17.54 | 26.09 | 28.20 | 293.74 | 0.4942 | -613.0 | -533.3 | |
| 0.00 | 4.41 | 0.00 | 2.50 | 17.12 | 25.80 | 27.92 | 293.09 | 0.4884 | -815.0 | -726.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 17.29 | 25.51 | 27.62 | 293.60 | 0.4850 | -595.0 | -514.2 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 16.88 | 25.08 | 27.20 | 293.04 | 0.4772 | -858.0 | -683.9 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 16.93 | 24.77 | 26.88 | 293.33 | 0.4730 | -835.0 | -715.2 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 17.26 | 23.72 | 25.84 | 294.69 | 0.4599 | -657.0 | -426.0 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 18.60 | 21.75 | 23.86 | 299.00 | 0.4401 | 764.0 | 615.2 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 18.21 | 21.48 | 23.59 | 298.41 | 0.4340 | 789.0 | 540.6 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 18.64 | 20.95 | 23.06 | 299.79 | 0.4295 | 846.0 | 670.6 | |
| 0.00 | 1.35 | 0.00 | 0.73 | 16.90 | 20.30 | 22.41 | 296.56 | 0.4095 | 775.0 | 621.5 | |
| 0.00 | 1.53 | 0.00 | 0.83 | 17.27 | 20.31 | 22.42 | 297.39 | 0.4120 | 777.0 | 666.9 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 18.92 | 20.26 | 22.37 | 301.05 | 0.4220 | 728.0 | 502.4 | |
| 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. | |