SDO HMI 2014-05-21 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.97 | 97.47 | 1.54 | 51.45 | -18.13 | 141.89 | 10.67 | 210.13 | 0.3399 | 479.2 | 401.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.43 | 0.00 | 1.33 | -20.03 | 149.52 | 18.29 | 223.33 | 0.4315 | 761.0 | 638.9 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -16.58 | 149.08 | 17.85 | 229.07 | 0.3906 | 637.0 | 539.1 | |
| 0.00 | 2.07 | 0.00 | 1.13 | -19.68 | 149.31 | 18.08 | 223.61 | 0.4254 | 799.0 | 715.7 | |
| 0.00 | 6.30 | 0.00 | 3.37 | -16.08 | 148.70 | 17.48 | 229.51 | 0.3810 | 464.0 | 582.5 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -16.05 | 148.30 | 17.08 | 228.94 | 0.3758 | 801.0 | 693.2 | |
| 0.00 | 2.70 | 0.00 | 1.47 | -19.68 | 148.63 | 17.40 | 222.56 | 0.4182 | 794.0 | 680.7 | |
| 0.00 | 1.35 | 0.00 | 0.73 | -19.08 | 148.56 | 17.34 | 223.51 | 0.4108 | 829.0 | 605.5 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -15.83 | 148.19 | 16.96 | 229.21 | 0.3722 | 776.0 | 593.4 | |
| 0.00 | 3.24 | 0.00 | 1.73 | -16.02 | 148.04 | 16.81 | 228.57 | 0.3723 | 860.0 | 700.3 | |
| 0.00 | 1.44 | 0.00 | 0.78 | -19.40 | 147.76 | 16.53 | 221.63 | 0.4057 | 868.0 | 749.2 | |
| 0.00 | 2.25 | 0.00 | 1.22 | -19.37 | 147.25 | 16.03 | 220.83 | 0.4000 | 780.0 | 655.4 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -18.99 | 147.11 | 15.89 | 221.26 | 0.3942 | 677.0 | 644.4 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -15.22 | 146.63 | 15.40 | 227.91 | 0.3468 | 806.0 | 579.9 | |
| 0.00 | 0.27 | 0.00 | 0.14 | -15.57 | 146.56 | 15.33 | 227.02 | 0.3496 | 24.0 | 27.0 | |
| 0.00 | 2.70 | 0.00 | 1.45 | -19.19 | 146.80 | 15.57 | 220.37 | 0.3931 | 854.0 | 704.1 | |
| 0.00 | 4.23 | 0.00 | 2.29 | -20.30 | 146.84 | 15.62 | 218.56 | 0.4068 | 683.0 | 614.6 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -20.98 | 146.71 | 15.48 | 217.25 | 0.4136 | 658.0 | 534.3 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -20.88 | 146.57 | 15.34 | 217.14 | 0.4111 | 609.0 | 610.8 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -20.63 | 146.44 | 15.21 | 217.33 | 0.4067 | 653.0 | 562.2 | |
| 0.00 | 2.25 | 0.00 | 1.20 | -18.40 | 145.47 | 14.24 | 219.33 | 0.3699 | 797.0 | 676.0 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -16.86 | 145.28 | 14.05 | 221.90 | 0.3495 | 12.0 | 6.2 | |
| 0.00 | 2.16 | 0.00 | 1.16 | -19.45 | 145.43 | 14.20 | 217.41 | 0.3824 | 857.0 | 737.1 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -18.18 | 145.06 | 13.83 | 218.92 | 0.3630 | 936.0 | 736.0 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -17.24 | 144.53 | 13.30 | 219.62 | 0.3460 | 874.0 | 696.7 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -16.02 | 143.66 | 12.44 | 220.23 | 0.3219 | 832.0 | 666.1 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -22.48 | 143.22 | 12.00 | 208.61 | 0.4028 | 551.0 | 429.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -22.39 | 143.01 | 11.79 | 208.32 | 0.3999 | 738.0 | 579.2 | |
| 0.00 | 1.26 | 0.00 | 0.66 | -18.64 | 142.37 | 11.14 | 212.40 | 0.3432 | 754.0 | 604.1 | |
| 0.00 | 1.35 | 0.00 | 0.71 | -20.60 | 139.61 | 8.38 | 203.05 | 0.3501 | 15.0 | 15.9 | |
| 0.00 | 2.07 | 0.00 | 1.07 | -17.43 | 136.92 | 5.70 | 199.48 | 0.2853 | -870.0 | -601.5 | |
| 0.00 | 4.41 | 0.00 | 2.28 | -17.49 | 136.38 | 5.16 | 197.68 | 0.2834 | -732.0 | -762.7 | |
| 2.97 | 36.63 | 1.54 | 18.98 | -17.81 | 136.36 | 5.13 | 197.26 | 0.2883 | -282.9 | 371.2 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -17.59 | 136.00 | 4.78 | 196.36 | 0.2831 | -650.0 | -517.3 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -17.12 | 135.93 | 4.70 | 196.61 | 0.2751 | -815.0 | -664.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -14.99 | 134.56 | 3.33 | 193.92 | 0.2343 | 835.0 | 589.2 | |
| 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. | |