SDO HMI 2012-10-15 05:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102.69 | 557.57 | 69.33 | 377.96 | 7.34 | 228.61 | -43.25 | 85.48 | 0.6836 | -673.4 | -126.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.01 | 343.89 | 41.53 | 226.87 | 7.41 | 230.31 | -41.55 | 85.40 | 0.6622 | -1292.1 | -311.8 | |
| 0.00 | 1.05 | 0.00 | 0.72 | 10.86 | 227.51 | -44.35 | 80.40 | 0.6986 | -550.0 | -433.7 | |
| 1.22 | 1.57 | 0.84 | 1.08 | 7.00 | 227.80 | -44.06 | 85.96 | 0.6943 | -760.7 | -818.0 | |
| 0.44 | 5.51 | 0.30 | 3.79 | 7.26 | 227.68 | -44.18 | 85.57 | 0.6957 | -906.8 | -668.6 | |
| 0.00 | 1.57 | 0.00 | 1.09 | 7.24 | 227.30 | -44.55 | 85.60 | 0.7004 | -439.0 | -421.6 | |
| 17.39 | 39.33 | 12.04 | 27.26 | 5.14 | 227.36 | -44.50 | 88.61 | 0.7007 | -842.6 | -311.5 | |
| 1.57 | 2.71 | 1.09 | 1.88 | 7.67 | 227.08 | -44.78 | 84.98 | 0.7031 | -620.9 | -518.9 | |
| 0.00 | 1.22 | 0.00 | 0.86 | 9.44 | 226.60 | -45.26 | 82.46 | 0.7091 | -473.0 | -382.9 | |
| 0.00 | 1.31 | 0.00 | 0.91 | 6.93 | 226.83 | -45.03 | 86.02 | 0.7063 | -671.0 | -459.7 | |
| 0.00 | 0.96 | 0.00 | 0.67 | 9.19 | 226.47 | -45.39 | 82.82 | 0.7107 | -256.0 | -240.2 | |
| 1.05 | 47.37 | 0.73 | 33.26 | 7.40 | 226.69 | -45.17 | 85.35 | 0.7080 | -502.2 | -44.6 | |
| 1.49 | -11.00 | 1.04 | -11.00 | 7.19 | 226.63 | -45.23 | 85.66 | 0.7087 | -784.6 | 999999 | |
| 0.00 | 1.49 | 0.00 | 1.04 | 5.28 | 226.75 | -45.11 | 88.37 | 0.7081 | 124.0 | 109.9 | |
| 0.00 | 1.14 | 0.00 | 0.79 | 5.09 | 226.72 | -45.14 | 88.62 | 0.7085 | 203.0 | 150.4 | |
| 1.31 | -11.00 | 0.92 | -11.00 | 7.39 | 226.43 | -45.43 | 85.37 | 0.7111 | -440.3 | 999999 | |
| 1.57 | -11.00 | 1.11 | -11.00 | 6.93 | 226.36 | -45.50 | 86.01 | 0.7121 | -464.7 | 999999 | |
| 2.97 | 35.13 | 2.11 | 24.87 | 8.42 | 225.81 | -46.05 | 83.91 | 0.7186 | 837.0 | 484.5 | |
| 1.49 | -17.00 | 1.06 | -17.00 | 8.20 | 225.66 | -46.19 | 84.22 | 0.7203 | 734.8 | 999999 | |
| 4.72 | 6.90 | 3.35 | 4.90 | 7.28 | 225.75 | -46.11 | 85.51 | 0.7194 | -552.7 | -348.5 | |
| 0.00 | 12.06 | 0.00 | 8.58 | 7.84 | 225.63 | -46.23 | 84.72 | 0.7207 | 469.0 | 389.3 | |
| 0.00 | 1.66 | 0.00 | 1.18 | 6.82 | 225.63 | -46.22 | 86.14 | 0.7209 | -294.0 | -221.3 | |
| 1.31 | -17.00 | 0.94 | -17.00 | 8.15 | 225.41 | -46.45 | 84.28 | 0.7234 | 857.2 | 999999 | |
| 1.40 | 2.97 | 1.01 | 2.14 | 9.55 | 225.09 | -46.77 | 82.36 | 0.7272 | 663.2 | 539.9 | |
| 0.00 | 0.61 | 0.00 | 0.44 | 8.75 | 224.87 | -46.99 | 83.46 | 0.7297 | 591.0 | 477.7 | |
| 0.70 | 15.64 | 0.50 | 11.31 | 7.19 | 225.01 | -46.84 | 85.60 | 0.7282 | -336.8 | 234.6 | |
| 1.05 | 20.01 | 0.76 | 14.44 | 8.17 | 224.83 | -47.03 | 84.25 | 0.7303 | 695.8 | 559.7 | |
| 0.00 | 1.92 | 0.00 | 1.39 | 8.04 | 224.63 | -47.23 | 84.44 | 0.7327 | 776.0 | 618.1 | |
| 0.00 | 0.96 | 0.00 | 0.70 | 9.08 | 224.46 | -47.40 | 83.01 | 0.7346 | 625.0 | 496.6 | |
| 0.00 | 0.70 | 0.00 | 0.51 | 6.75 | 224.76 | -47.10 | 86.20 | 0.7314 | 499.0 | 545.6 | |
| 0.00 | 1.84 | 0.00 | 1.34 | 8.62 | 224.40 | -47.46 | 83.64 | 0.7353 | 724.0 | 588.4 | |
| 0.00 | 1.66 | 0.00 | 1.21 | 8.35 | 224.35 | -47.50 | 84.01 | 0.7358 | 725.0 | 607.5 | |
| 0.00 | 1.75 | 0.00 | 1.28 | 8.07 | 224.26 | -47.59 | 84.39 | 0.7369 | 754.0 | 641.8 | |
| 0.00 | 1.05 | 0.00 | 0.77 | 7.83 | 224.25 | -47.60 | 84.72 | 0.7371 | 536.0 | 486.4 | |
| 0.00 | 1.14 | 0.00 | 0.84 | 7.50 | 223.90 | -47.96 | 85.15 | 0.7413 | 495.0 | 489.4 | |
| 0.00 | 1.14 | 0.00 | 0.85 | 7.66 | 222.73 | -49.13 | 84.92 | 0.7547 | 566.0 | 475.8 | |
| 0.00 | 1.31 | 0.00 | 0.99 | 5.16 | 222.77 | -49.09 | 88.23 | 0.7553 | 641.0 | 524.5 | |
| 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. | |