SDO HMI 2014-10-05 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.08 | 181.75 | 35.04 | 118.00 | -12.24 | 163.76 | 35.65 | 242.10 | 0.6463 | 262.4 | 78.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.85 | 0.00 | 1.40 | -20.67 | 169.84 | 41.74 | 235.40 | 0.7591 | 571.0 | 495.6 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -10.32 | 166.29 | 38.18 | 246.40 | 0.6660 | 446.0 | 518.0 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -13.62 | 166.60 | 38.50 | 242.11 | 0.6868 | 552.0 | 385.8 | |
| 27.26 | 95.14 | 18.02 | 62.98 | -12.29 | 165.27 | 37.17 | 243.09 | 0.6643 | 885.4 | 160.5 | |
| 0.00 | 2.46 | 0.00 | 1.61 | -11.66 | 164.90 | 36.80 | 243.72 | 0.6566 | 680.0 | 626.2 | |
| 0.00 | 1.67 | 0.00 | 1.09 | -11.88 | 164.86 | 36.76 | 243.39 | 0.6573 | 949.0 | 773.3 | |
| 4.13 | -4.00 | 2.71 | -4.00 | -12.24 | 164.65 | 36.55 | 242.75 | 0.6568 | 962.2 | 999999 | |
| 4.31 | 6.59 | 2.80 | 4.28 | -11.28 | 164.39 | 36.28 | 243.93 | 0.6484 | 974.6 | 806.8 | |
| 0.70 | 3.61 | 0.46 | 2.35 | -11.79 | 164.43 | 36.32 | 243.25 | 0.6516 | 847.9 | 748.4 | |
| 0.00 | 2.02 | 0.00 | 1.33 | -12.78 | 164.58 | 36.48 | 241.98 | 0.6591 | 517.0 | 347.1 | |
| 0.00 | 2.64 | 0.00 | 1.71 | -12.05 | 164.12 | 36.02 | 242.69 | 0.6496 | 854.0 | 740.6 | |
| 0.70 | 1.93 | 0.45 | 1.25 | -11.19 | 163.96 | 35.85 | 243.79 | 0.6427 | 759.1 | 689.1 | |
| 2.73 | 5.54 | 1.76 | 3.58 | -11.93 | 163.73 | 35.62 | 242.60 | 0.6442 | 864.9 | 710.7 | |
| 0.00 | 2.20 | 0.00 | 1.41 | -11.45 | 163.62 | 35.51 | 243.20 | 0.6401 | 873.0 | 671.1 | |
| 0.00 | 2.99 | 0.00 | 1.91 | -10.62 | 163.43 | 35.32 | 244.26 | 0.6331 | -726.0 | -568.6 | |
| 0.00 | 1.76 | 0.00 | 1.12 | -10.35 | 163.17 | 35.06 | 244.48 | 0.6285 | -726.0 | -642.8 | |
| 0.00 | 3.34 | 0.00 | 2.11 | -10.69 | 162.69 | 34.59 | 243.67 | 0.6246 | -612.0 | -561.8 | |
| 0.00 | 2.02 | 0.00 | 1.28 | -10.95 | 162.32 | 34.21 | 243.04 | 0.6216 | -280.0 | -329.5 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -13.69 | 162.73 | 34.62 | 239.45 | 0.6433 | 662.0 | 491.5 | |
| 0.00 | 2.64 | 0.00 | 1.67 | -12.14 | 162.26 | 34.15 | 241.29 | 0.6281 | 639.0 | 625.4 | |
| 7.65 | 13.45 | 4.80 | 8.45 | -11.02 | 161.92 | 33.81 | 242.67 | 0.6171 | -803.5 | -454.1 | |
| 0.00 | 1.32 | 0.00 | 0.83 | -11.99 | 161.90 | 33.80 | 241.25 | 0.6229 | 654.0 | 538.1 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -11.02 | 161.55 | 33.45 | 242.40 | 0.6127 | -604.0 | -461.6 | |
| 2.02 | 3.78 | 1.25 | 2.34 | -11.08 | 160.46 | 32.36 | 241.53 | 0.5998 | -780.5 | -607.7 | |
| 0.00 | 1.76 | 0.00 | 1.10 | -14.43 | 159.81 | 31.71 | 236.19 | 0.6149 | -666.0 | -538.7 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -15.33 | 159.45 | 31.34 | 234.63 | 0.6174 | -580.0 | -462.8 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -15.49 | 159.40 | 31.30 | 234.38 | 0.6181 | -434.0 | -290.4 | |
| 0.00 | 2.73 | 0.00 | 1.69 | -14.48 | 158.62 | 30.52 | 235.10 | 0.6017 | -406.0 | -338.5 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -13.72 | 158.22 | 30.12 | 235.83 | 0.5914 | -537.0 | -500.1 | |
| 1.85 | 3.78 | 1.13 | 2.31 | -13.49 | 158.08 | 29.98 | 236.04 | 0.5880 | -852.2 | -569.2 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -11.76 | 157.83 | 29.72 | 238.37 | 0.5722 | -730.0 | -571.6 | |
| 0.62 | 2.37 | 0.38 | 1.45 | -13.50 | 157.77 | 29.66 | 235.74 | 0.5844 | -801.7 | -673.4 | |
| 0.00 | 2.29 | 0.00 | 1.39 | -13.39 | 157.50 | 29.40 | 235.67 | 0.5805 | -747.0 | -662.3 | |
| 2.11 | 4.22 | 1.28 | 2.56 | -13.16 | 157.40 | 29.30 | 235.91 | 0.5775 | -1012.8 | -875.0 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -12.33 | 157.30 | 29.19 | 237.05 | 0.5700 | -558.0 | -610.8 | |
| 0.00 | 0.53 | 0.00 | 0.32 | -12.57 | 157.01 | 28.90 | 236.43 | 0.5684 | -202.0 | -357.3 | |
| 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. | |