SDO HMI 2014-01-13 18:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.03 | 191.68 | 29.90 | 98.80 | -17.92 | 30.22 | 8.63 | 211.12 | 0.2767 | 238.7 | 58.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.62 | -19.22 | 32.29 | 10.71 | 214.32 | 0.3126 | 675.0 | 543.6 | |
| 25.74 | 76.55 | 13.32 | 39.64 | -18.13 | 31.56 | 9.98 | 214.63 | 0.2912 | 1202.1 | 399.8 | |
| 4.25 | 29.74 | 2.19 | 15.33 | -17.35 | 31.36 | 9.78 | 215.76 | 0.2787 | 1173.5 | 833.2 | |
| 2.21 | -3.00 | 1.14 | -3.00 | -17.62 | 31.28 | 9.70 | 214.95 | 0.2816 | 1181.3 | 999999 | |
| 0.93 | -2.00 | 0.48 | -2.00 | -18.23 | 31.03 | 9.45 | 213.01 | 0.2876 | 932.5 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -17.20 | 30.82 | 9.24 | 214.58 | 0.2715 | 842.0 | 583.0 | |
| 3.23 | -3.00 | 1.66 | -3.00 | -17.65 | 30.82 | 9.23 | 213.58 | 0.2777 | 1136.2 | 999999 | |
| 0.00 | 2.21 | 0.00 | 1.14 | -18.05 | 30.49 | 8.91 | 211.85 | 0.2802 | 630.0 | 505.1 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -18.30 | 30.38 | 8.79 | 211.05 | 0.2827 | 888.0 | 772.3 | |
| 0.00 | 0.68 | 0.00 | 0.35 | -17.82 | 29.70 | 8.11 | 209.99 | 0.2700 | -486.0 | -330.6 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -15.92 | 29.46 | 7.88 | 213.34 | 0.2410 | 873.0 | 793.8 | |
| 0.68 | 1.87 | 0.35 | 0.96 | -17.34 | 29.24 | 7.66 | 209.52 | 0.2593 | -1222.4 | -1000.1 | |
| 11.56 | 30.84 | 5.93 | 15.84 | -17.82 | 29.17 | 7.58 | 208.35 | 0.2657 | -1057.7 | -632.4 | |
| 0.00 | 3.74 | 0.00 | 1.92 | -18.16 | 28.87 | 7.28 | 206.80 | 0.2684 | -874.0 | -766.0 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -17.68 | 28.41 | 6.83 | 206.20 | 0.2577 | -1154.0 | -993.7 | |
| 8.75 | 38.49 | 4.48 | 19.73 | -17.86 | 27.89 | 6.31 | 204.14 | 0.2568 | -1291.6 | -550.8 | |
| 0.68 | -16.00 | 0.35 | -16.00 | -18.23 | 27.81 | 6.22 | 203.27 | 0.2619 | -829.1 | 999999 | |
| 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. | |