SDO HMI 2014-10-11 10:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.95 | 449.40 | 40.85 | 287.62 | -20.53 | 18.03 | -29.27 | 133.59 | 0.6344 | 844.4 | 292.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.35 | 0.00 | 0.22 | -21.86 | 20.45 | -26.85 | 137.57 | 0.6236 | -573.0 | -480.8 | |
| 0.00 | 1.23 | 0.00 | 0.77 | -21.28 | 20.57 | -26.74 | 137.01 | 0.6171 | -649.0 | -449.0 | |
| 0.00 | 2.72 | 0.00 | 1.67 | -18.31 | 20.33 | -26.97 | 133.08 | 0.5918 | 581.0 | 583.4 | |
| 0.53 | 3.15 | 0.32 | 1.94 | -18.42 | 20.06 | -27.24 | 132.95 | 0.5955 | 770.5 | 698.3 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -17.32 | 19.79 | -27.52 | 131.22 | 0.5886 | 608.0 | 512.0 | |
| 0.00 | 2.72 | 0.00 | 1.70 | -19.94 | 19.31 | -27.99 | 134.12 | 0.6167 | 701.0 | 670.8 | |
| 0.70 | 3.07 | 0.43 | 1.90 | -18.55 | 19.36 | -27.94 | 132.41 | 0.6039 | 749.1 | 584.6 | |
| 2.28 | 425.48 | 1.44 | 272.24 | -20.33 | 18.87 | -28.43 | 134.16 | 0.6245 | 1230.5 | 296.2 | |
| 0.00 | 0.96 | 0.00 | 0.60 | -17.82 | 18.99 | -28.31 | 131.09 | 0.6013 | 655.0 | 507.9 | |
| 60.44 | -8.00 | 38.66 | -8.00 | -20.58 | 18.06 | -29.24 | 133.67 | 0.6346 | 1098.0 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.76 | -17.64 | 18.05 | -29.25 | 129.95 | 0.6097 | 490.0 | 352.6 | |
| 0.00 | 1.14 | 0.00 | 0.77 | -24.20 | 15.70 | -31.60 | 135.75 | 0.6872 | 258.0 | 225.6 | |
| 0.00 | 1.14 | 0.00 | 0.76 | -20.86 | 14.93 | -32.37 | 131.22 | 0.6674 | 498.0 | 383.2 | |
| 0.00 | 0.79 | 0.00 | 0.56 | -22.66 | 11.43 | -35.87 | 130.56 | 0.7141 | -221.0 | -246.3 | |
| 0.00 | 1.40 | 0.00 | 1.05 | -26.36 | 9.84 | -37.47 | 133.50 | 0.7538 | -502.0 | -494.0 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -18.14 | 10.81 | -36.49 | 124.69 | 0.6896 | -479.0 | -472.0 | |
| 0.00 | 2.80 | 0.00 | 1.91 | -17.85 | 10.76 | -36.54 | 124.29 | 0.6882 | -516.0 | -445.2 | |
| 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. | |