SDO HMI 2014-05-22 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 |
| 0.54 | 60.03 | 0.32 | 35.26 | -18.34 | 147.90 | 28.24 | 236.99 | 0.5359 | 530.1 | 527.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.35 | 0.00 | 0.88 | -16.69 | 157.86 | 38.20 | 246.03 | 0.6505 | 733.0 | 542.2 | |
| 0.00 | 1.35 | 0.00 | 0.86 | -18.51 | 155.22 | 35.56 | 242.02 | 0.6267 | 644.0 | 565.1 | |
| 0.00 | 1.17 | 0.00 | 0.74 | -18.48 | 155.02 | 35.35 | 241.95 | 0.6241 | 633.0 | 575.9 | |
| 0.00 | 1.26 | 0.00 | 0.80 | -20.02 | 154.18 | 34.51 | 239.16 | 0.6222 | -602.0 | -546.7 | |
| 0.00 | 1.89 | 0.00 | 1.14 | -19.57 | 149.94 | 30.28 | 236.94 | 0.5690 | 641.0 | 451.3 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -16.29 | 149.11 | 29.45 | 241.70 | 0.5380 | 793.0 | 598.2 | |
| 0.54 | 7.47 | 0.32 | 4.47 | -19.58 | 149.68 | 30.02 | 236.73 | 0.5659 | 737.5 | 701.2 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -16.23 | 148.88 | 29.22 | 241.64 | 0.5347 | 703.0 | 566.0 | |
| 0.00 | 1.62 | 0.00 | 0.97 | -19.17 | 149.19 | 29.53 | 237.00 | 0.5572 | 740.0 | 585.7 | |
| 0.00 | 5.49 | 0.00 | 3.20 | -15.95 | 148.59 | 28.92 | 241.90 | 0.5292 | 782.0 | 695.6 | |
| 0.00 | 1.89 | 0.00 | 1.12 | -19.43 | 148.94 | 29.28 | 236.39 | 0.5560 | 636.0 | 588.3 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -18.41 | 148.71 | 29.05 | 237.85 | 0.5463 | 660.0 | 502.6 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -16.34 | 148.28 | 28.62 | 241.02 | 0.5275 | 664.0 | 568.4 | |
| 0.00 | 2.07 | 0.00 | 1.20 | -15.56 | 147.98 | 28.32 | 242.16 | 0.5189 | 726.0 | 635.3 | |
| 0.00 | 1.71 | 0.00 | 0.99 | -16.25 | 147.91 | 28.25 | 240.89 | 0.5221 | 734.0 | 633.2 | |
| 0.00 | 3.24 | 0.00 | 1.91 | -19.25 | 148.10 | 28.44 | 235.99 | 0.5445 | 739.0 | 733.6 | |
| 0.00 | 1.62 | 0.00 | 0.96 | -19.63 | 148.14 | 28.47 | 235.41 | 0.5476 | 852.0 | 697.1 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -18.08 | 147.60 | 27.94 | 237.50 | 0.5301 | -201.0 | -273.1 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -19.74 | 147.32 | 27.65 | 234.53 | 0.5385 | 793.0 | 681.2 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -20.73 | 147.40 | 27.73 | 233.02 | 0.5469 | 345.0 | 316.6 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -20.18 | 147.22 | 27.56 | 233.72 | 0.5407 | 599.0 | 486.6 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -19.61 | 147.04 | 27.37 | 234.48 | 0.5342 | 806.0 | 645.3 | |
| 0.00 | 3.15 | 0.00 | 1.83 | -18.85 | 146.79 | 27.13 | 235.52 | 0.5256 | 913.0 | 785.9 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -21.12 | 146.60 | 26.93 | 231.67 | 0.5407 | 628.0 | 504.2 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -18.29 | 145.91 | 26.25 | 235.66 | 0.5106 | 648.0 | 521.6 | |
| 0.00 | 1.26 | 0.00 | 0.74 | -20.94 | 146.20 | 26.53 | 231.59 | 0.5346 | 541.0 | 552.0 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -17.98 | 145.50 | 25.84 | 235.82 | 0.5032 | 774.0 | 578.5 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -18.55 | 145.10 | 25.43 | 234.44 | 0.5025 | 817.0 | 713.9 | |
| 0.00 | 1.71 | 0.00 | 0.97 | -17.76 | 144.83 | 25.17 | 235.55 | 0.4932 | 635.0 | 654.5 | |
| 0.00 | 1.26 | 0.00 | 0.72 | -17.58 | 144.70 | 25.04 | 235.76 | 0.4900 | 878.0 | 742.1 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -18.68 | 144.76 | 25.10 | 233.89 | 0.4994 | 616.0 | 612.9 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -17.67 | 144.54 | 24.88 | 235.43 | 0.4887 | 795.0 | 677.6 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -17.83 | 144.46 | 24.79 | 235.06 | 0.4889 | 865.0 | 727.4 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -17.93 | 137.75 | 18.08 | 226.61 | 0.4082 | -871.0 | -667.9 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -17.12 | 136.93 | 17.27 | 226.91 | 0.3902 | -595.0 | -483.8 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -17.09 | 136.50 | 16.83 | 226.26 | 0.3848 | -784.0 | -663.9 | |
| 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. | |