SDO HMI 2014-05-19 07:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.57 | 245.42 | 23.92 | 144.59 | -24.46 | 190.79 | 24.83 | 224.99 | 0.5430 | 610.3 | 324.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.77 | 232.37 | 22.87 | 137.07 | -24.39 | 191.07 | 25.11 | 225.41 | 0.5449 | 1221.0 | 375.5 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -20.96 | 190.34 | 24.38 | 229.88 | 0.5062 | -664.0 | -595.6 | |
| 1.80 | -1.00 | 1.05 | -1.00 | -24.10 | 190.46 | 24.50 | 225.18 | 0.5359 | 987.0 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.00 | -24.27 | 189.73 | 23.77 | 224.12 | 0.5299 | 885.0 | 749.8 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -24.90 | 186.96 | 21.00 | 219.93 | 0.5085 | -662.0 | -472.8 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -24.62 | 185.88 | 19.92 | 218.92 | 0.4950 | -787.0 | -581.6 | |
| 0.00 | 0.63 | 0.00 | 0.36 | -25.94 | 185.60 | 19.64 | 216.75 | 0.5072 | -696.0 | -600.9 | |
| 0.00 | 1.89 | 0.00 | 1.09 | -27.04 | 185.65 | 19.70 | 215.41 | 0.5201 | -723.0 | -587.5 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -27.48 | 185.30 | 19.34 | 214.40 | 0.5221 | -494.0 | -562.0 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -27.18 | 185.14 | 19.18 | 214.55 | 0.5173 | -827.0 | -698.0 | |
| 0.00 | 1.80 | 0.00 | 1.04 | -27.42 | 185.10 | 19.15 | 214.22 | 0.5198 | -880.0 | -776.3 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -30.89 | 185.41 | 19.46 | 210.66 | 0.5626 | -664.0 | -537.6 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -27.12 | 184.26 | 18.30 | 213.44 | 0.5093 | -813.0 | -700.4 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -23.69 | 183.38 | 17.43 | 216.68 | 0.4610 | -712.0 | -556.7 | |
| 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. | |