SDO HMI 2014-10-03 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.51 | 137.70 | 30.65 | 73.53 | -12.28 | 160.15 | 11.15 | 210.35 | 0.3758 | -34.8 | 24.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.44 | -11.45 | 167.64 | 18.63 | 225.87 | 0.4381 | 709.0 | 623.8 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -9.66 | 165.90 | 16.89 | 226.17 | 0.3988 | 911.0 | 660.7 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -13.94 | 165.49 | 16.48 | 218.51 | 0.4442 | 690.0 | 528.8 | |
| 0.00 | 1.58 | 0.00 | 0.85 | -8.57 | 165.05 | 16.05 | 226.75 | 0.3769 | 826.0 | 635.3 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -16.69 | 164.80 | 15.79 | 213.68 | 0.4720 | 745.0 | 598.4 | |
| 0.00 | 2.02 | 0.00 | 1.08 | -10.36 | 163.75 | 14.74 | 221.00 | 0.3832 | -914.0 | -732.3 | |
| 1.93 | 36.93 | 1.04 | 19.80 | -11.90 | 162.40 | 13.40 | 215.82 | 0.3891 | 840.4 | 794.9 | |
| 2.20 | -7.00 | 1.18 | -7.00 | -11.70 | 162.27 | 13.26 | 215.84 | 0.3853 | 1047.2 | 999999 | |
| 3.78 | -7.00 | 2.03 | -7.00 | -11.99 | 162.22 | 13.21 | 215.31 | 0.3885 | 1088.9 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -12.27 | 162.23 | 13.23 | 214.91 | 0.3924 | 766.0 | 564.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -12.75 | 162.16 | 13.16 | 214.07 | 0.3980 | 689.0 | 509.3 | |
| 2.29 | -7.00 | 1.23 | -7.00 | -11.98 | 161.93 | 12.93 | 214.74 | 0.3858 | 1057.5 | 999999 | |
| 6.86 | -7.00 | 3.67 | -7.00 | -11.73 | 161.92 | 12.92 | 215.10 | 0.3824 | 1253.1 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.80 | -12.60 | 161.65 | 12.65 | 213.23 | 0.3916 | 866.0 | 786.1 | |
| 1.93 | -7.00 | 1.04 | -7.00 | -11.84 | 161.52 | 12.51 | 214.07 | 0.3802 | 960.4 | 999999 | |
| 0.00 | 2.55 | 0.00 | 1.36 | -11.73 | 161.08 | 12.07 | 213.28 | 0.3748 | 738.0 | 521.9 | |
| 0.62 | 2.37 | 0.33 | 1.28 | -13.51 | 160.94 | 11.93 | 210.50 | 0.3978 | 879.4 | 705.1 | |
| 0.88 | 2.64 | 0.47 | 1.42 | -13.28 | 160.86 | 11.86 | 210.64 | 0.3941 | 1056.9 | 869.7 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -13.63 | 160.76 | 11.75 | 209.96 | 0.3981 | 708.0 | 477.1 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -11.41 | 160.62 | 11.62 | 212.77 | 0.3664 | -721.0 | -587.2 | |
| 0.00 | 2.46 | 0.00 | 1.31 | -11.33 | 159.97 | 10.96 | 211.38 | 0.3596 | 1012.0 | 828.9 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -11.55 | 159.97 | 10.97 | 211.08 | 0.3628 | 775.0 | 638.4 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -13.34 | 159.39 | 10.39 | 207.35 | 0.3835 | -196.0 | -345.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -13.30 | 159.05 | 10.04 | 206.61 | 0.3804 | 608.0 | 340.8 | |
| 3.78 | 9.76 | 1.99 | 5.15 | -10.93 | 158.93 | 9.92 | 209.47 | 0.3454 | -1098.7 | -797.9 | |
| 6.95 | 56.27 | 3.69 | 29.91 | -12.47 | 158.67 | 9.66 | 206.76 | 0.3656 | -1181.8 | -670.2 | |
| 0.00 | 2.29 | 0.00 | 1.22 | -13.26 | 158.67 | 9.66 | 205.79 | 0.3771 | -546.0 | -389.9 | |
| 17.67 | -26.00 | 9.42 | -26.00 | -12.82 | 158.62 | 9.61 | 206.21 | 0.3703 | -1011.0 | 999999 | |
| 2.64 | -26.00 | 1.40 | -26.00 | -12.28 | 158.57 | 9.56 | 206.77 | 0.3621 | -1152.6 | 999999 | |
| 5.98 | -26.00 | 3.16 | -26.00 | -11.70 | 158.49 | 9.48 | 207.31 | 0.3532 | -1095.6 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -18.79 | 158.68 | 9.68 | 200.43 | 0.4577 | 538.0 | 494.3 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -15.03 | 157.45 | 8.45 | 201.12 | 0.3955 | -837.0 | -541.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.19 | 157.27 | 8.27 | 200.56 | 0.3969 | -679.0 | -545.1 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -14.42 | 155.43 | 6.43 | 196.85 | 0.3756 | -789.0 | -696.6 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -14.47 | 154.37 | 5.37 | 194.17 | 0.3718 | -598.0 | -574.8 | |
| 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. | |