SDO HMI 2014-07-08 17:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.47 | 255.32 | 33.44 | 174.03 | 14.77 | 261.12 | 42.40 | 287.83 | 0.6864 | -461.0 | -242.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.82 | 0.00 | 1.35 | 13.63 | 266.68 | 47.96 | 285.01 | 0.7495 | -568.0 | -471.1 | |
| 0.00 | 1.91 | 0.00 | 1.34 | 12.50 | 263.58 | 44.85 | 284.01 | 0.7120 | -457.0 | -411.2 | |
| 0.00 | 1.27 | 0.00 | 0.89 | 11.83 | 263.26 | 44.53 | 283.12 | 0.7071 | -548.0 | -469.3 | |
| 1.36 | 6.17 | 0.96 | 4.33 | 12.97 | 263.46 | 44.74 | 284.68 | 0.7114 | -777.9 | -667.1 | |
| 1.54 | 3.99 | 1.08 | 2.81 | 13.22 | 263.39 | 44.66 | 285.05 | 0.7109 | -790.8 | -596.1 | |
| 0.00 | 1.27 | 0.00 | 0.91 | 15.63 | 263.97 | 45.25 | 288.25 | 0.7224 | 481.0 | 433.8 | |
| 1.18 | -4.00 | 0.83 | -4.00 | 12.92 | 263.23 | 44.51 | 284.66 | 0.7085 | -874.7 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.82 | 11.74 | 262.63 | 43.90 | 283.09 | 0.6993 | -655.0 | -554.1 | |
| 0.00 | 0.91 | 0.00 | 0.64 | 15.68 | 262.82 | 44.10 | 288.61 | 0.7092 | -548.0 | -438.0 | |
| 0.45 | 1.63 | 0.32 | 1.15 | 16.78 | 262.78 | 44.06 | 290.14 | 0.7114 | 518.4 | 418.5 | |
| 17.16 | 202.10 | 11.84 | 139.30 | 14.65 | 262.07 | 43.35 | 287.35 | 0.6980 | -982.0 | -320.2 | |
| 23.33 | -11.00 | 16.06 | -11.00 | 15.10 | 261.84 | 43.11 | 288.04 | 0.6962 | -1059.7 | 999999 | |
| 0.00 | 0.64 | 0.00 | 0.43 | 12.95 | 261.08 | 42.35 | 285.14 | 0.6824 | -701.0 | -628.0 | |
| 3.45 | -11.00 | 2.35 | -11.00 | 14.94 | 261.11 | 42.38 | 288.01 | 0.6871 | -856.6 | 999999 | |
| 0.00 | 3.27 | 0.00 | 2.20 | 14.81 | 260.60 | 41.88 | 287.95 | 0.6807 | -818.0 | -701.0 | |
| 0.00 | 1.27 | 0.00 | 0.85 | 13.64 | 260.21 | 41.49 | 286.35 | 0.6732 | -785.0 | -579.0 | |
| 0.00 | 0.91 | 0.00 | 0.61 | 14.85 | 260.32 | 41.59 | 288.09 | 0.6773 | -722.0 | -702.5 | |
| 0.00 | 0.82 | 0.00 | 0.54 | 14.70 | 258.74 | 40.01 | 288.31 | 0.6574 | -663.0 | -581.8 | |
| 0.00 | 1.09 | 0.00 | 0.71 | 16.67 | 258.05 | 39.32 | 291.48 | 0.6546 | 624.0 | 590.7 | |
| 0.00 | 1.09 | 0.00 | 0.68 | 13.22 | 255.16 | 36.43 | 287.13 | 0.6072 | 554.0 | 416.2 | |
| 0.00 | 1.18 | 0.00 | 0.73 | 13.57 | 254.06 | 35.33 | 288.08 | 0.5935 | 702.0 | 612.2 | |
| 0.00 | 0.73 | 0.00 | 0.45 | 13.73 | 254.08 | 35.36 | 288.33 | 0.5944 | 520.0 | 498.0 | |
| 0.00 | 0.73 | 0.00 | 0.46 | 18.79 | 254.53 | 35.80 | 296.19 | 0.6194 | -519.0 | -479.5 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 13.61 | 252.99 | 34.27 | 288.54 | 0.5793 | 556.0 | 513.9 | |
| 0.00 | 1.36 | 0.00 | 0.83 | 14.08 | 252.92 | 34.19 | 289.36 | 0.5799 | 557.0 | 474.9 | |
| 0.00 | 4.90 | 0.00 | 2.97 | 14.27 | 252.76 | 34.04 | 289.75 | 0.5785 | 399.0 | 590.6 | |
| 0.00 | 1.73 | 0.00 | 1.04 | 14.53 | 252.62 | 33.89 | 290.24 | 0.5775 | 705.0 | 627.7 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 11.88 | 252.12 | 33.40 | 285.88 | 0.5621 | 330.0 | 321.4 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 10.44 | 251.82 | 33.10 | 283.43 | 0.5542 | 679.0 | 488.9 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 10.81 | 251.79 | 33.07 | 284.10 | 0.5547 | 741.0 | 543.6 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 12.02 | 251.51 | 32.78 | 286.35 | 0.5540 | 753.0 | 560.5 | |
| 0.00 | 3.72 | 0.00 | 2.27 | 18.67 | 251.84 | 33.11 | 297.44 | 0.5853 | 661.0 | 545.8 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 15.02 | 250.86 | 32.13 | 291.89 | 0.5557 | 761.0 | 550.8 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 15.49 | 249.90 | 31.17 | 293.21 | 0.5448 | 721.0 | 558.8 | |
| 0.00 | 2.09 | 0.00 | 1.23 | 15.44 | 249.59 | 30.87 | 293.29 | 0.5405 | 758.0 | 539.8 | |
| 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. | |