SDO HMI 2014-05-18 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.19 | 273.43 | 25.45 | 147.47 | -24.07 | 191.66 | 8.63 | 200.30 | 0.3968 | 777.3 | 369.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.48 | 264.61 | 7.27 | 142.76 | -24.00 | 192.09 | 9.06 | 201.28 | 0.3979 | 1217.8 | 405.7 | |
| 0.27 | -1.00 | 0.15 | -1.00 | -24.32 | 192.11 | 9.08 | 201.00 | 0.4028 | 844.0 | 999999 | |
| 11.24 | -1.00 | 6.05 | -1.00 | -23.90 | 191.68 | 8.65 | 200.50 | 0.3941 | 1447.4 | 999999 | |
| 20.04 | -1.00 | 10.82 | -1.00 | -24.23 | 191.70 | 8.67 | 200.23 | 0.3991 | 1131.5 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -21.31 | 191.52 | 8.49 | 202.91 | 0.3546 | -743.0 | -607.2 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -21.06 | 191.31 | 8.27 | 202.70 | 0.3495 | -790.0 | -652.7 | |
| 2.16 | -1.00 | 1.16 | -1.00 | -23.87 | 191.11 | 8.07 | 199.29 | 0.3905 | 877.2 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -22.51 | 190.43 | 7.40 | 199.03 | 0.3663 | -674.0 | -512.5 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -26.11 | 190.27 | 7.23 | 195.67 | 0.4204 | 568.0 | 511.9 | |
| 0.00 | 1.98 | 0.00 | 1.06 | -23.82 | 187.54 | 4.50 | 191.10 | 0.3745 | -983.0 | -741.0 | |
| 0.00 | 0.36 | 0.00 | 0.19 | -24.21 | 187.18 | 4.15 | 190.05 | 0.3797 | -845.0 | -680.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -25.79 | 185.65 | 2.62 | 185.90 | 0.4015 | -928.0 | -733.2 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -24.89 | 180.38 | -2.65 | 173.75 | 0.3872 | -670.0 | -537.6 | |
| 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. | |