| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.86 | 364.33 | 61.97 | 249.37 | -17.83 | 105.36 | 36.45 | 235.07 | 0.6915 | 111.6 | 67.2 | |
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back to the solar disc SDO HMI 2014-08-16 06:00:38 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.09 | 169.66 | 14.90 | 119.32 | -17.33 | 107.97 | 39.05 | 237.56 | 0.7150 | 951.3 | 353.6 | |
| 16.23 | -1.00 | 11.39 | -1.00 | -17.05 | 107.78 | 38.86 | 237.78 | 0.7113 | 1211.6 | 999999 | |
| 1.35 | -1.00 | 0.94 | -1.00 | -16.54 | 107.53 | 38.61 | 238.26 | 0.7058 | 831.3 | 999999 | |
| 1.53 | -1.00 | 1.07 | -1.00 | -17.19 | 107.04 | 38.12 | 237.12 | 0.7045 | 1031.5 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.38 | -17.86 | 107.12 | 38.21 | 236.35 | 0.7095 | 431.0 | 436.8 | |
| 0.00 | 1.98 | 0.00 | 1.38 | -17.74 | 106.81 | 37.89 | 236.29 | 0.7055 | 532.0 | 435.7 | |
| 0.00 | 2.25 | 0.00 | 1.56 | -17.26 | 106.65 | 37.73 | 236.78 | 0.7009 | 680.0 | 583.4 | |
| 4.60 | 13.70 | 3.18 | 9.46 | -17.41 | 106.44 | 37.53 | 236.45 | 0.6997 | 824.9 | 463.6 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -18.05 | 106.52 | 37.60 | 235.72 | 0.7045 | -361.0 | -280.2 | |
| 0.00 | 1.80 | 0.00 | 1.25 | -17.98 | 106.10 | 37.18 | 235.51 | 0.6998 | 521.0 | 467.5 | |
| 0.00 | 0.99 | 0.00 | 0.69 | -18.42 | 106.21 | 37.29 | 235.04 | 0.7037 | 557.0 | 418.4 | |
| 0.00 | 1.26 | 0.00 | 0.88 | -18.72 | 106.16 | 37.25 | 234.65 | 0.7052 | 514.0 | 406.0 | |
| 0.00 | 2.79 | 0.00 | 1.94 | -19.16 | 105.84 | 36.92 | 233.88 | 0.7047 | 129.0 | -31.2 | |
| 0.00 | 3.52 | 0.00 | 2.41 | -18.00 | 105.50 | 36.59 | 235.06 | 0.6938 | 179.0 | 123.9 | |
| 0.00 | 1.26 | 0.00 | 0.88 | -19.41 | 105.62 | 36.70 | 233.42 | 0.7043 | 492.0 | 276.1 | |
| 0.00 | 0.63 | 0.00 | 0.43 | -18.21 | 105.20 | 36.28 | 234.58 | 0.6920 | 450.0 | 351.1 | |
| 0.00 | 1.08 | 0.00 | 0.74 | -18.87 | 105.08 | 36.16 | 233.69 | 0.6952 | 211.0 | 194.5 | |
| 4.06 | 12.80 | 2.81 | 8.84 | -19.48 | 105.16 | 36.24 | 233.01 | 0.7001 | 761.0 | 583.0 | |
| 0.00 | 1.62 | 0.00 | 1.10 | -18.08 | 104.73 | 35.81 | 234.41 | 0.6863 | -198.0 | -324.0 | |
| 0.00 | 0.81 | 0.00 | 0.56 | -19.02 | 104.80 | 35.88 | 233.30 | 0.6934 | 534.0 | 507.6 | |
| 0.00 | 1.89 | 0.00 | 1.27 | -17.51 | 104.21 | 35.29 | 234.73 | 0.6771 | -450.0 | -200.3 | |
| 0.00 | 1.80 | 0.00 | 1.23 | -19.20 | 104.57 | 35.65 | 232.91 | 0.6923 | 183.0 | 189.3 | |
| 0.00 | 1.35 | 0.00 | 0.91 | -18.20 | 104.05 | 35.13 | 233.76 | 0.6801 | 466.0 | 447.2 | |
| 0.45 | 1.62 | 0.30 | 1.09 | -17.71 | 103.78 | 34.87 | 234.16 | 0.6740 | -529.2 | -305.8 | |
| 3.25 | 6.13 | 2.16 | 4.08 | -17.87 | 103.23 | 34.32 | 233.54 | 0.6695 | -719.6 | -477.5 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -19.86 | 103.47 | 34.55 | 231.27 | 0.6861 | 678.0 | 533.3 | |
| 0.00 | 1.08 | 0.00 | 0.73 | -20.06 | 103.36 | 34.44 | 230.95 | 0.6864 | 564.0 | 473.8 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -18.34 | 102.84 | 33.92 | 232.64 | 0.6687 | -440.0 | -369.7 | |
| 0.72 | 2.97 | 0.48 | 1.97 | -18.06 | 102.66 | 33.74 | 232.85 | 0.6649 | -747.9 | -597.6 | |
| 0.00 | 1.98 | 0.00 | 1.31 | -17.73 | 102.59 | 33.67 | 233.21 | 0.6617 | -689.0 | -655.1 | |
| 0.00 | 1.53 | 0.00 | 1.01 | -17.70 | 102.24 | 33.32 | 232.97 | 0.6578 | -626.0 | -650.4 | |
| 1.35 | 124.32 | 0.90 | 81.93 | -18.81 | 102.36 | 33.45 | 231.68 | 0.6673 | -241.5 | -469.0 | |
| 2.79 | -32.00 | 1.85 | -32.00 | -19.00 | 102.25 | 33.34 | 231.35 | 0.6676 | -488.3 | 999999 | |
| 32.90 | -32.00 | 21.64 | -32.00 | -18.48 | 101.90 | 32.99 | 231.72 | 0.6601 | -1095.4 | 999999 | |
| 0.54 | -32.00 | 0.35 | -32.00 | -17.67 | 101.70 | 32.78 | 232.57 | 0.6519 | -814.3 | 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. | |