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 |
| 64.64 | 248.28 | 35.01 | 134.54 | -16.54 | 194.76 | 19.41 | 231.99 | 0.4057 | 159.3 | 32.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 0.95 | -15.83 | 198.56 | 23.22 | 237.96 | 0.4493 | 872.0 | 686.0 | |
| 26.43 | 123.96 | 14.50 | 67.96 | -17.46 | 196.16 | 20.82 | 232.06 | 0.4316 | 1140.3 | 479.4 | |
| 7.55 | -2.00 | 4.12 | -2.00 | -16.58 | 195.86 | 20.51 | 233.40 | 0.4201 | 1080.5 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -16.59 | 195.35 | 20.01 | 232.74 | 0.4137 | 1036.0 | 887.9 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -16.50 | 195.01 | 19.66 | 232.47 | 0.4085 | 922.0 | 619.6 | |
| 0.36 | 4.58 | 0.19 | 2.48 | -16.63 | 194.75 | 19.41 | 231.86 | 0.4065 | 1075.2 | 893.6 | |
| 0.00 | 10.52 | 0.00 | 5.65 | -15.63 | 193.98 | 18.64 | 232.87 | 0.3877 | 7.0 | -132.6 | |
| 1.08 | 105.53 | 0.58 | 56.43 | -16.26 | 193.71 | 18.37 | 231.16 | 0.3900 | -746.3 | -576.6 | |
| 1.35 | -8.00 | 0.72 | -8.00 | -15.79 | 193.57 | 18.22 | 231.94 | 0.3838 | -790.4 | 999999 | |
| 6.74 | -8.00 | 3.61 | -8.00 | -15.95 | 193.32 | 17.97 | 231.23 | 0.3821 | -1086.6 | 999999 | |
| 3.33 | -8.00 | 1.78 | -8.00 | -15.55 | 193.18 | 17.84 | 231.90 | 0.3766 | -1211.9 | 999999 | |
| 9.26 | -8.00 | 4.94 | -8.00 | -15.36 | 193.03 | 17.69 | 232.08 | 0.3730 | -1346.5 | 999999 | |
| 8.54 | -8.00 | 4.57 | -8.00 | -16.11 | 193.00 | 17.65 | 230.41 | 0.3797 | -1093.2 | 999999 | |
| 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. | |