SDO HMI 2014-05-22 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 |
| 0.36 | 59.40 | 0.21 | 33.91 | -18.05 | 147.37 | 24.94 | 234.47 | 0.4936 | 514.6 | 533.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.73 | -16.49 | 157.86 | 35.43 | 245.01 | 0.6154 | 646.0 | 497.4 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -18.90 | 155.26 | 32.82 | 239.78 | 0.5957 | 562.0 | 387.2 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -18.43 | 155.04 | 32.61 | 240.37 | 0.5903 | 505.0 | 459.0 | |
| 0.00 | 1.35 | 0.00 | 0.78 | -16.32 | 150.59 | 28.16 | 240.71 | 0.5213 | 682.0 | 539.2 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -17.55 | 150.07 | 27.64 | 238.16 | 0.5227 | 562.0 | 470.9 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -19.33 | 149.87 | 27.44 | 235.01 | 0.5328 | 616.0 | 507.0 | |
| 0.00 | 2.25 | 0.00 | 1.29 | -16.21 | 149.04 | 26.61 | 239.65 | 0.5004 | 777.0 | 655.1 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -16.25 | 148.83 | 26.40 | 239.41 | 0.4979 | 923.0 | 739.7 | |
| 0.00 | 2.16 | 0.00 | 1.26 | -19.56 | 149.33 | 26.90 | 234.15 | 0.5281 | 653.0 | 658.0 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -17.98 | 149.03 | 26.60 | 236.53 | 0.5125 | 710.0 | 597.7 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -19.47 | 149.21 | 26.78 | 234.19 | 0.5258 | 935.0 | 745.3 | |
| 0.00 | 3.96 | 0.00 | 2.25 | -15.97 | 148.41 | 25.98 | 239.54 | 0.4905 | 902.0 | 799.1 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -16.41 | 148.26 | 25.83 | 238.60 | 0.4915 | 765.0 | 622.6 | |
| 0.00 | 2.97 | 0.00 | 1.72 | -19.38 | 148.51 | 26.08 | 233.68 | 0.5167 | 571.0 | 551.9 | |
| 0.00 | 3.06 | 0.00 | 1.72 | -15.16 | 147.84 | 25.41 | 240.55 | 0.4776 | 570.0 | 591.3 | |
| 0.00 | 1.98 | 0.00 | 1.12 | -15.57 | 147.79 | 25.36 | 239.74 | 0.4796 | 840.0 | 715.7 | |
| 0.00 | 3.60 | 0.00 | 2.04 | -15.94 | 147.84 | 25.41 | 239.09 | 0.4829 | 600.0 | 599.5 | |
| 0.36 | 1.35 | 0.21 | 0.78 | -19.61 | 147.98 | 25.54 | 232.78 | 0.5121 | 861.5 | 730.0 | |
| 0.00 | 1.98 | 0.00 | 1.14 | -19.10 | 147.82 | 25.39 | 233.48 | 0.5062 | 833.0 | 690.6 | |
| 0.00 | 1.71 | 0.00 | 0.98 | -19.04 | 147.38 | 24.95 | 233.14 | 0.5004 | 529.0 | 552.4 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -19.59 | 147.01 | 24.58 | 231.84 | 0.5004 | 940.0 | 796.9 | |
| 0.00 | 5.04 | 0.00 | 2.87 | -18.79 | 146.85 | 24.42 | 233.02 | 0.4919 | 732.0 | 687.5 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -18.51 | 146.77 | 24.34 | 233.43 | 0.4886 | 793.0 | 658.6 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -21.00 | 146.57 | 24.14 | 229.05 | 0.5075 | 683.0 | 565.6 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -20.62 | 146.05 | 23.61 | 229.09 | 0.4981 | 772.0 | 580.7 | |
| 0.00 | 2.16 | 0.00 | 1.24 | -21.04 | 146.08 | 23.65 | 228.45 | 0.5022 | 661.0 | 536.6 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -18.59 | 145.18 | 22.74 | 231.55 | 0.4698 | 837.0 | 640.6 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -18.44 | 144.77 | 22.34 | 231.36 | 0.4636 | 698.0 | 531.1 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -18.69 | 144.77 | 22.34 | 230.91 | 0.4658 | 831.0 | 706.0 | |
| 0.00 | 2.07 | 0.00 | 1.15 | -18.60 | 144.21 | 21.78 | 230.39 | 0.4582 | 372.0 | 391.7 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -22.38 | 144.32 | 21.89 | 224.28 | 0.4957 | 484.0 | 546.3 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -18.20 | 138.88 | 16.45 | 223.50 | 0.3924 | -660.0 | -424.1 | |
| 0.00 | 0.63 | 0.00 | 0.34 | -18.11 | 138.01 | 15.57 | 222.16 | 0.3818 | -542.0 | -541.1 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -17.42 | 137.29 | 14.85 | 222.16 | 0.3660 | -736.0 | -569.7 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -17.43 | 136.83 | 14.39 | 221.29 | 0.3610 | -803.0 | -728.6 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -17.65 | 136.15 | 13.72 | 219.54 | 0.3566 | -652.0 | -556.0 | |
| 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. | |