SDO HMI 2014-08-23 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.52 | 41.00 | 9.10 | 21.31 | -9.08 | 333.01 | -6.68 | 158.19 | 0.3048 | 662.8 | 477.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.55 | -6.35 | 338.88 | -0.82 | 176.47 | 0.2318 | 726.0 | 550.5 | |
| 0.00 | 2.79 | 0.00 | 1.44 | -10.21 | 338.40 | -1.29 | 175.70 | 0.2976 | 861.0 | 684.0 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -5.98 | 336.99 | -2.71 | 168.15 | 0.2299 | 907.0 | 703.9 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -9.18 | 335.40 | -4.30 | 165.08 | 0.2889 | 688.0 | 538.3 | |
| 0.00 | 1.35 | 0.00 | 0.70 | -8.59 | 335.22 | -4.48 | 163.92 | 0.2800 | 891.0 | 746.5 | |
| 17.52 | 24.98 | 9.10 | 12.98 | -9.52 | 333.73 | -5.97 | 160.08 | 0.3025 | 1109.3 | 741.3 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -4.84 | 330.94 | -8.76 | 143.26 | 0.2547 | 932.0 | 666.9 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -7.77 | 330.45 | -9.24 | 147.82 | 0.3002 | 890.0 | 667.7 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -10.50 | 329.59 | -10.10 | 149.98 | 0.3462 | 771.0 | 583.8 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -6.50 | 328.31 | -11.39 | 139.62 | 0.3042 | 685.0 | 462.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -7.84 | 324.05 | -15.64 | 133.25 | 0.3683 | -741.0 | -626.6 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -11.87 | 323.82 | -15.88 | 139.95 | 0.4178 | -656.0 | -621.2 | |
| 0.00 | 0.45 | 0.00 | 0.24 | -9.66 | 323.40 | -16.30 | 135.49 | 0.3963 | -754.0 | -566.4 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -9.48 | 322.09 | -17.61 | 132.94 | 0.4093 | -647.0 | -538.4 | |
| 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. | |