SDO HMI 2014-05-18 14:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.44 | 269.69 | 23.02 | 149.65 | -24.31 | 191.05 | 15.70 | 213.16 | 0.4526 | 603.8 | 315.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.82 | 250.43 | 13.23 | 139.11 | -24.10 | 191.55 | 16.20 | 214.31 | 0.4537 | 1304.9 | 397.0 | |
| 17.62 | -1.00 | 9.79 | -1.00 | -24.37 | 191.38 | 16.03 | 213.68 | 0.4555 | 1221.0 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -24.15 | 189.94 | 14.59 | 211.59 | 0.4405 | 819.0 | 648.2 | |
| 0.00 | 1.44 | 0.00 | 0.78 | -24.20 | 187.17 | 11.83 | 206.55 | 0.4200 | -646.0 | -572.5 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -24.63 | 186.43 | 11.09 | 204.64 | 0.4210 | -749.0 | -642.7 | |
| 0.00 | 2.61 | 0.00 | 1.42 | -24.37 | 186.34 | 11.00 | 204.75 | 0.4167 | -992.0 | -796.0 | |
| 0.00 | 2.07 | 0.00 | 1.13 | -24.60 | 186.16 | 10.81 | 204.15 | 0.4187 | -834.0 | -701.1 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -25.69 | 186.19 | 10.84 | 203.07 | 0.4344 | -827.0 | -734.9 | |
| 0.00 | 1.71 | 0.00 | 0.94 | -25.79 | 185.61 | 10.27 | 201.88 | 0.4324 | -854.0 | -776.1 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -27.29 | 185.54 | 10.19 | 200.38 | 0.4535 | -890.0 | -727.5 | |
| 0.00 | 1.89 | 0.00 | 1.05 | -27.93 | 184.59 | 9.24 | 198.13 | 0.4579 | -742.0 | -572.0 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -27.13 | 184.18 | 8.83 | 198.00 | 0.4442 | -879.0 | -756.2 | |
| 0.00 | 1.80 | 0.00 | 0.98 | -25.84 | 180.48 | 5.14 | 191.39 | 0.4097 | -754.0 | -462.7 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -24.20 | 180.01 | 4.67 | 191.24 | 0.3824 | -726.0 | -585.5 | |
| 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. | |