SDO HMI 2014-11-06 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.82 | 184.40 | 31.21 | 97.57 | -5.01 | 87.07 | 18.29 | 243.63 | 0.3502 | -3.1 | 63.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.37 | 0.00 | 1.83 | -5.42 | 91.08 | 22.30 | 247.49 | 0.4107 | 913.0 | 810.7 | |
| 0.00 | 1.73 | 0.00 | 0.93 | -3.94 | 90.80 | 22.03 | 250.68 | 0.3982 | 576.0 | 432.8 | |
| 9.93 | 41.55 | 5.37 | 22.40 | -4.57 | 90.76 | 21.98 | 249.16 | 0.4010 | 883.6 | 584.6 | |
| 12.18 | -3.00 | 6.56 | -3.00 | -4.17 | 90.43 | 21.65 | 249.81 | 0.3937 | 1034.1 | 999999 | |
| 3.97 | -3.00 | 2.14 | -3.00 | -4.35 | 90.30 | 21.53 | 249.28 | 0.3929 | 1103.6 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.03 | -5.97 | 90.26 | 21.49 | 245.45 | 0.4022 | 899.0 | 617.5 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -3.83 | 89.94 | 21.16 | 250.21 | 0.3844 | 895.0 | 613.2 | |
| 0.00 | 7.77 | 0.00 | 4.17 | -4.60 | 89.70 | 20.92 | 248.11 | 0.3853 | 1165.0 | 902.8 | |
| 3.80 | 9.50 | 2.02 | 5.06 | -3.56 | 89.01 | 20.23 | 250.03 | 0.3688 | 1077.8 | 808.3 | |
| 0.00 | 1.38 | 0.00 | 0.73 | -2.09 | 88.54 | 19.76 | 253.52 | 0.3539 | 775.0 | 599.1 | |
| 0.00 | 1.90 | 0.00 | 1.01 | -5.20 | 88.42 | 19.64 | 245.30 | 0.3700 | 765.0 | 643.3 | |
| 0.69 | 14.94 | 0.37 | 7.98 | -5.65 | 88.18 | 19.40 | 243.93 | 0.3696 | 1121.4 | 816.5 | |
| 0.00 | 1.38 | 0.00 | 0.73 | -3.68 | 87.43 | 18.65 | 248.15 | 0.3454 | 907.0 | 790.8 | |
| 0.00 | 1.47 | 0.00 | 0.78 | -5.73 | 86.73 | 17.95 | 241.90 | 0.3492 | -732.0 | -691.2 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -3.66 | 86.68 | 17.90 | 247.36 | 0.3338 | 846.0 | 706.3 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -5.58 | 86.57 | 17.79 | 242.08 | 0.3457 | -616.0 | -518.6 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -5.60 | 86.22 | 17.45 | 241.55 | 0.3408 | -703.0 | -542.1 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -4.15 | 85.78 | 17.00 | 244.88 | 0.3235 | 811.0 | 555.5 | |
| 0.00 | 1.04 | 0.00 | 0.54 | -4.57 | 85.76 | 16.98 | 243.68 | 0.3262 | -861.0 | -731.9 | |
| 6.13 | 23.75 | 3.22 | 12.47 | -5.83 | 85.54 | 16.76 | 239.99 | 0.3329 | -1039.4 | -450.8 | |
| 0.00 | 1.64 | 0.00 | 0.86 | -5.41 | 85.53 | 16.75 | 241.08 | 0.3293 | -792.0 | -717.4 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -5.26 | 85.49 | 16.72 | 241.44 | 0.3276 | -778.0 | -614.3 | |
| 0.00 | 1.73 | 0.00 | 0.90 | -4.74 | 85.45 | 16.67 | 242.78 | 0.3230 | -802.0 | -642.2 | |
| 0.00 | 2.16 | 0.00 | 1.13 | -5.10 | 85.30 | 16.53 | 241.58 | 0.3236 | -832.0 | -672.8 | |
| 0.00 | 3.45 | 0.00 | 1.80 | -4.44 | 85.23 | 16.45 | 243.31 | 0.3174 | 814.0 | 692.4 | |
| 1.73 | -20.00 | 0.91 | -20.00 | -5.88 | 85.23 | 16.45 | 239.38 | 0.3289 | -1005.8 | 999999 | |
| 0.00 | 1.55 | 0.00 | 0.81 | -5.82 | 85.07 | 16.30 | 239.30 | 0.3261 | -850.0 | -524.9 | |
| 6.74 | 41.20 | 3.51 | 21.45 | -4.97 | 84.74 | 15.96 | 241.10 | 0.3144 | -1131.1 | -618.3 | |
| 3.37 | 5.36 | 1.76 | 2.80 | -5.60 | 84.69 | 15.92 | 239.29 | 0.3189 | -947.8 | -748.5 | |
| 1.73 | -28.00 | 0.90 | -28.00 | -5.06 | 84.53 | 15.75 | 240.53 | 0.3119 | -1080.8 | 999999 | |
| 0.43 | 2.16 | 0.23 | 1.13 | -5.26 | 84.38 | 15.60 | 239.71 | 0.3115 | -889.0 | -706.1 | |
| 8.12 | -28.00 | 4.22 | -28.00 | -4.90 | 84.24 | 15.47 | 240.52 | 0.3066 | -1166.9 | 999999 | |
| 0.00 | 1.73 | 0.00 | 0.89 | -6.88 | 80.39 | 11.61 | 227.15 | 0.2738 | -867.0 | -734.5 | |
| 0.00 | 1.47 | 0.00 | 0.76 | -8.46 | 80.12 | 11.34 | 222.50 | 0.2893 | -770.0 | -570.0 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -8.55 | 78.20 | 9.42 | 217.06 | 0.2698 | -774.0 | -674.6 | |
| 0.00 | 2.68 | 0.00 | 1.38 | -8.91 | 77.81 | 9.04 | 215.12 | 0.2709 | -881.0 | -695.7 | |
| 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. | |