SDO HMI 2014-10-19 04:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.24 | 537.04 | 48.62 | 285.83 | -8.80 | 320.89 | 15.84 | 227.60 | 0.3663 | 680.5 | 333.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.71 | -9.45 | 322.89 | 17.84 | 229.87 | 0.3968 | -753.0 | -634.1 | |
| 0.61 | 495.06 | 0.33 | 263.91 | -9.05 | 322.77 | 17.72 | 230.49 | 0.3913 | -704.9 | 409.6 | |
| 4.01 | -2.00 | 2.15 | -2.00 | -8.87 | 321.97 | 16.92 | 229.54 | 0.3795 | 915.8 | 999999 | |
| 0.26 | -2.00 | 0.14 | -2.00 | -9.17 | 321.77 | 16.71 | 228.58 | 0.3802 | 750.3 | 999999 | |
| 2.53 | -2.00 | 1.35 | -2.00 | -9.23 | 321.64 | 16.59 | 228.25 | 0.3793 | 810.3 | 999999 | |
| 1.40 | -2.00 | 0.75 | -2.00 | -9.26 | 321.42 | 16.37 | 227.82 | 0.3769 | 774.2 | 999999 | |
| 78.77 | -2.00 | 41.95 | -2.00 | -8.69 | 321.24 | 16.19 | 228.64 | 0.3687 | 1434.0 | 999999 | |
| 2.70 | -2.00 | 1.44 | -2.00 | -9.22 | 321.14 | 16.08 | 227.40 | 0.3731 | 874.2 | 999999 | |
| 0.96 | -2.00 | 0.51 | -2.00 | -9.27 | 320.76 | 15.71 | 226.62 | 0.3692 | 986.9 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -5.40 | 320.41 | 15.35 | 234.68 | 0.3245 | 721.0 | 525.2 | |
| 0.00 | 1.22 | 0.00 | 0.65 | -9.10 | 319.25 | 14.20 | 224.05 | 0.3499 | 738.0 | 633.3 | |
| 0.00 | 1.48 | 0.00 | 0.79 | -11.43 | 319.26 | 14.21 | 219.73 | 0.3780 | 727.0 | 575.8 | |
| 0.00 | 1.48 | 0.00 | 0.78 | -9.25 | 319.07 | 14.02 | 223.38 | 0.3496 | 713.0 | 557.1 | |
| 0.00 | 1.22 | 0.00 | 0.64 | -8.79 | 318.96 | 13.90 | 224.09 | 0.3428 | 883.0 | 751.8 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -11.98 | 318.76 | 13.70 | 217.79 | 0.3798 | 864.0 | 699.7 | |
| 0.00 | 2.09 | 0.00 | 1.10 | -9.76 | 318.15 | 13.10 | 220.47 | 0.3457 | -827.0 | -624.2 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -9.63 | 317.99 | 12.94 | 220.37 | 0.3424 | -421.0 | -295.3 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -11.95 | 317.37 | 12.32 | 214.94 | 0.3661 | 742.0 | 642.1 | |
| 0.00 | 1.31 | 0.00 | 0.69 | -10.68 | 316.51 | 11.46 | 215.08 | 0.3411 | -805.0 | -586.9 | |
| 0.00 | 1.57 | 0.00 | 0.82 | -8.53 | 315.76 | 10.71 | 217.22 | 0.3052 | -982.0 | -804.7 | |
| 0.00 | 3.58 | 0.00 | 1.86 | -8.13 | 315.75 | 10.70 | 218.01 | 0.2998 | -838.0 | -707.4 | |
| 0.00 | 1.31 | 0.00 | 0.68 | -9.26 | 315.32 | 10.27 | 214.66 | 0.3107 | -723.0 | -560.1 | |
| 0.00 | 1.40 | 0.00 | 0.72 | -8.91 | 314.82 | 9.77 | 213.98 | 0.3013 | -933.0 | -762.8 | |
| 0.00 | 1.13 | 0.00 | 0.59 | -9.03 | 314.34 | 9.28 | 212.42 | 0.2984 | -1063.0 | -905.9 | |
| 0.00 | 0.70 | 0.00 | 0.36 | -8.59 | 314.20 | 9.15 | 212.85 | 0.2911 | -789.0 | -715.1 | |
| 0.00 | 1.83 | 0.00 | 0.95 | -9.27 | 313.88 | 8.83 | 210.71 | 0.2979 | -902.0 | -823.1 | |
| 0.00 | 2.88 | 0.00 | 1.50 | -9.98 | 313.81 | 8.75 | 209.31 | 0.3075 | -821.0 | -675.4 | |
| 0.00 | 1.05 | 0.00 | 0.54 | -8.80 | 313.78 | 8.72 | 211.24 | 0.2903 | -851.0 | -665.9 | |
| 0.00 | 2.44 | 0.00 | 1.27 | -9.05 | 313.72 | 8.67 | 210.64 | 0.2934 | -976.0 | -797.1 | |
| 0.00 | 1.31 | 0.00 | 0.68 | -9.26 | 313.70 | 8.64 | 210.19 | 0.2963 | -849.0 | -702.1 | |
| 0.00 | 0.96 | 0.00 | 0.50 | -9.63 | 313.55 | 8.50 | 209.16 | 0.3004 | -754.0 | -570.2 | |
| 0.00 | 1.40 | 0.00 | 0.72 | -9.23 | 313.51 | 8.46 | 209.72 | 0.2942 | -756.0 | -641.2 | |
| 0.00 | 1.66 | 0.00 | 0.86 | -8.95 | 313.17 | 8.12 | 209.19 | 0.2873 | -1018.0 | -729.5 | |
| 0.00 | 1.57 | 0.00 | 0.81 | -9.90 | 312.86 | 7.80 | 206.70 | 0.2989 | -748.0 | -539.3 | |
| 0.00 | 2.01 | 0.00 | 1.03 | -8.38 | 312.70 | 7.65 | 208.72 | 0.2752 | -951.0 | -782.2 | |
| 0.00 | 1.13 | 0.00 | 0.59 | -10.73 | 312.14 | 7.09 | 203.41 | 0.3064 | -607.0 | -381.7 | |
| 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. | |