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 |
| 56.94 | 189.37 | 33.26 | 110.87 | -16.86 | 195.05 | 29.09 | 241.01 | 0.5338 | 1.9 | 68.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.26 | 85.82 | 0.76 | 51.29 | -18.21 | 196.90 | 30.94 | 240.07 | 0.5657 | 597.8 | 390.2 | |
| 5.58 | -1.00 | 3.34 | -1.00 | -17.99 | 196.78 | 30.82 | 240.35 | 0.5629 | 945.3 | 999999 | |
| 12.14 | -1.00 | 7.25 | -1.00 | -17.71 | 196.65 | 30.69 | 240.72 | 0.5596 | 1073.5 | 999999 | |
| 2.25 | -1.00 | 1.34 | -1.00 | -17.99 | 196.56 | 30.60 | 240.19 | 0.5601 | 1056.8 | 999999 | |
| 4.50 | 8.37 | 2.67 | 4.96 | -17.15 | 196.25 | 30.30 | 241.37 | 0.5513 | 1013.4 | 787.9 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -16.78 | 195.82 | 29.86 | 241.70 | 0.5436 | 699.0 | 574.8 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -14.41 | 195.41 | 29.45 | 245.55 | 0.5252 | 814.0 | 691.7 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -17.26 | 195.50 | 29.54 | 240.66 | 0.5423 | 682.0 | 591.8 | |
| 0.72 | 2.88 | 0.42 | 1.68 | -16.82 | 194.95 | 29.00 | 241.00 | 0.5326 | 914.4 | 767.2 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -18.66 | 194.59 | 28.63 | 237.61 | 0.5397 | 552.0 | 526.1 | |
| 1.44 | 85.91 | 0.83 | 49.24 | -15.88 | 193.48 | 27.52 | 241.55 | 0.5075 | -808.6 | -422.8 | |
| 13.13 | -11.00 | 7.52 | -11.00 | -15.54 | 193.28 | 27.33 | 242.02 | 0.5028 | -1125.1 | 999999 | |
| 14.12 | -11.00 | 8.10 | -11.00 | -16.10 | 193.30 | 27.34 | 241.01 | 0.5065 | -1037.4 | 999999 | |
| 1.80 | -11.00 | 1.03 | -11.00 | -16.20 | 193.06 | 27.10 | 240.64 | 0.5040 | -1036.2 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -15.94 | 191.58 | 25.62 | 239.87 | 0.4827 | -883.0 | -687.3 | |
| 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. | |