SDO HMI 2014-05-18 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.94 | 217.59 | 38.58 | 120.26 | -16.68 | 194.84 | 22.26 | 235.24 | 0.4433 | 19.6 | 63.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.56 | -15.71 | 198.84 | 26.26 | 240.97 | 0.4890 | 699.0 | 623.4 | |
| 0.00 | 4.31 | 0.00 | 2.41 | -17.00 | 196.43 | 23.85 | 236.34 | 0.4665 | 353.0 | 605.8 | |
| 24.27 | 109.11 | 13.60 | 61.12 | -17.60 | 196.30 | 23.72 | 235.10 | 0.4695 | 1106.9 | 440.5 | |
| 2.25 | -3.00 | 1.26 | -3.00 | -18.01 | 196.36 | 23.78 | 234.41 | 0.4735 | 824.8 | 999999 | |
| 8.09 | -3.00 | 4.50 | -3.00 | -16.72 | 195.98 | 23.40 | 236.40 | 0.4585 | 1093.6 | 999999 | |
| 0.99 | 3.33 | 0.55 | 1.84 | -16.74 | 194.95 | 22.37 | 235.26 | 0.4453 | 991.5 | 800.1 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -16.55 | 194.72 | 22.14 | 235.37 | 0.4409 | 901.0 | 675.9 | |
| 1.44 | 97.15 | 0.79 | 52.86 | -16.35 | 193.54 | 20.96 | 234.40 | 0.4239 | -682.7 | -474.9 | |
| 0.72 | -8.00 | 0.39 | -8.00 | -15.91 | 193.32 | 20.74 | 235.02 | 0.4175 | -920.9 | 999999 | |
| 8.90 | -8.00 | 4.85 | -8.00 | -16.16 | 193.21 | 20.64 | 234.37 | 0.4182 | -1026.8 | 999999 | |
| 13.84 | -8.00 | 7.51 | -8.00 | -15.42 | 193.13 | 20.56 | 235.82 | 0.4109 | -1204.1 | 999999 | |
| 7.19 | -8.00 | 3.91 | -8.00 | -15.92 | 193.05 | 20.47 | 234.68 | 0.4140 | -1238.4 | 999999 | |
| 2.25 | -8.00 | 1.22 | -8.00 | -16.14 | 192.97 | 20.40 | 234.13 | 0.4149 | -1004.7 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -15.99 | 191.95 | 19.37 | 233.11 | 0.4004 | -747.0 | -565.8 | |
| 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. | |