SDO HMI 2014-07-31 16:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.45 | 86.62 | 26.00 | 60.06 | -18.83 | 237.42 | -37.55 | 124.51 | 0.7018 | -114.7 | -182.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.69 | 10.50 | 5.12 | 6.98 | -18.12 | 240.09 | -34.88 | 125.48 | 0.6696 | 806.9 | 553.7 | |
| 5.79 | 21.45 | 3.90 | 14.48 | -18.43 | 239.35 | -35.62 | 125.33 | 0.6795 | 745.9 | 489.9 | |
| 1.45 | -2.00 | 0.98 | -2.00 | -18.25 | 239.12 | -35.85 | 124.92 | 0.6807 | 756.8 | 999999 | |
| 0.54 | -2.00 | 0.37 | -2.00 | -18.35 | 238.97 | -36.00 | 124.96 | 0.6829 | 528.5 | 999999 | |
| 0.45 | 1.90 | 0.31 | 1.29 | -18.16 | 238.82 | -36.15 | 124.61 | 0.6833 | 535.0 | 451.6 | |
| 0.00 | 1.09 | 0.00 | 0.74 | -18.32 | 238.38 | -36.59 | 124.50 | 0.6889 | 242.0 | 299.9 | |
| 0.54 | 2.35 | 0.38 | 1.64 | -18.82 | 237.29 | -37.68 | 124.38 | 0.7034 | -665.8 | -602.1 | |
| 0.00 | 1.81 | 0.00 | 1.25 | -18.52 | 237.32 | -37.65 | 124.03 | 0.7011 | -766.0 | -656.2 | |
| 0.00 | 1.18 | 0.00 | 0.83 | -19.38 | 236.93 | -38.04 | 124.82 | 0.7104 | -690.0 | -587.1 | |
| 4.07 | 21.09 | 2.87 | 14.83 | -19.18 | 236.45 | -38.52 | 124.26 | 0.7140 | -797.7 | -620.3 | |
| 4.07 | -10.00 | 2.88 | -10.00 | -19.12 | 236.26 | -38.71 | 124.07 | 0.7156 | -694.8 | 999999 | |
| 3.80 | 10.41 | 2.69 | 7.36 | -18.75 | 235.91 | -39.06 | 123.38 | 0.7169 | -602.0 | -657.6 | |
| 9.05 | 14.84 | 6.50 | 10.66 | -19.64 | 235.53 | -39.44 | 124.22 | 0.7260 | -743.6 | -397.8 | |
| 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. | |