SDO HMI 2011-10-14 19:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 139.57 | 789.32 | 77.18 | 436.80 | -12.12 | 48.81 | -19.30 | 133.63 | 0.4463 | -59.7 | -51.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.63 | -16.19 | 53.60 | -14.51 | 147.20 | 0.4460 | 664.0 | 440.6 | |
| 1.14 | 262.29 | 0.61 | 141.57 | -12.27 | 52.68 | -15.42 | 139.90 | 0.4052 | 740.2 | 482.9 | |
| 48.30 | -2.00 | 26.08 | -2.00 | -11.71 | 52.59 | -15.52 | 138.80 | 0.3994 | 1258.8 | 999999 | |
| 1.57 | -2.00 | 0.85 | -2.00 | -11.76 | 51.86 | -16.25 | 137.57 | 0.4079 | 776.7 | 999999 | |
| 0.00 | 1.40 | 0.00 | 0.76 | -11.80 | 51.50 | -16.60 | 137.03 | 0.4121 | 566.0 | 475.2 | |
| 2.27 | 73.46 | 1.24 | 40.15 | -11.72 | 51.19 | -16.92 | 136.35 | 0.4146 | 1058.5 | 504.6 | |
| 2.97 | -6.00 | 1.62 | -6.00 | -11.94 | 51.11 | -17.00 | 136.60 | 0.4180 | 1066.6 | 999999 | |
| 2.36 | 7.51 | 1.29 | 4.11 | -12.85 | 51.02 | -17.09 | 137.94 | 0.4295 | 621.7 | 180.8 | |
| 3.23 | -6.00 | 1.76 | -6.00 | -12.13 | 50.94 | -17.17 | 136.63 | 0.4221 | 1089.1 | 999999 | |
| 1.40 | -6.00 | 0.77 | -6.00 | -12.48 | 50.79 | -17.32 | 136.96 | 0.4277 | 895.4 | 999999 | |
| 0.00 | 2.18 | 0.00 | 1.18 | -10.83 | 50.73 | -17.37 | 134.04 | 0.4097 | 760.0 | 660.4 | |
| 0.00 | 4.02 | 0.00 | 2.21 | -13.28 | 50.57 | -17.54 | 137.87 | 0.4391 | -287.0 | -558.2 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -10.33 | 48.84 | -19.27 | 130.19 | 0.4267 | 768.0 | 539.6 | |
| 0.00 | 0.52 | 0.00 | 0.29 | -10.37 | 48.61 | -19.49 | 129.93 | 0.4299 | 716.0 | 580.5 | |
| 1.05 | 2.10 | 0.58 | 1.16 | -11.21 | 47.62 | -20.49 | 130.02 | 0.4503 | 750.9 | 666.2 | |
| 1.31 | 425.62 | 0.73 | 239.56 | -11.47 | 47.53 | -20.58 | 130.34 | 0.4538 | 301.9 | -463.1 | |
| 1.57 | -16.00 | 0.88 | -16.00 | -11.99 | 46.93 | -21.17 | 130.41 | 0.4660 | -1066.2 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.75 | -14.51 | 46.50 | -21.61 | 133.82 | 0.4961 | -852.0 | -694.0 | |
| 2.62 | -16.00 | 1.47 | -16.00 | -12.54 | 46.62 | -21.48 | 130.90 | 0.4750 | -1232.9 | 999999 | |
| 1.75 | -16.00 | 0.98 | -16.00 | -12.07 | 46.63 | -21.48 | 130.14 | 0.4702 | -1149.5 | 999999 | |
| 1.92 | -16.00 | 1.08 | -16.00 | -11.91 | 46.58 | -21.53 | 129.81 | 0.4694 | -1007.2 | 999999 | |
| 0.70 | -16.00 | 0.40 | -16.00 | -13.27 | 46.36 | -21.75 | 131.74 | 0.4853 | -532.2 | 999999 | |
| 34.85 | -16.00 | 19.66 | -16.00 | -12.68 | 46.25 | -21.86 | 130.64 | 0.4807 | -1124.1 | 999999 | |
| 2.97 | -16.00 | 1.66 | -16.00 | -11.61 | 46.24 | -21.86 | 128.87 | 0.4705 | -1461.1 | 999999 | |
| 11.79 | -16.00 | 6.63 | -16.00 | -12.12 | 46.20 | -21.91 | 129.66 | 0.4758 | -1226.1 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.25 | -14.37 | 45.95 | -22.16 | 132.90 | 0.5007 | -788.0 | -680.6 | |
| 4.72 | -16.00 | 2.65 | -16.00 | -11.78 | 46.00 | -22.11 | 128.84 | 0.4750 | -1114.4 | 999999 | |
| 0.96 | -16.00 | 0.54 | -16.00 | -12.85 | 45.90 | -22.21 | 130.48 | 0.4864 | -382.0 | 999999 | |
| 1.48 | -16.00 | 0.83 | -16.00 | -11.53 | 45.95 | -22.15 | 128.37 | 0.4732 | -1009.1 | 999999 | |
| 1.92 | -16.00 | 1.08 | -16.00 | -11.95 | 45.62 | -22.49 | 128.65 | 0.4811 | -951.2 | 999999 | |
| 0.96 | -16.00 | 0.54 | -16.00 | -12.11 | 45.54 | -22.57 | 128.82 | 0.4836 | -667.6 | 999999 | |
| 5.76 | -16.00 | 3.25 | -16.00 | -11.74 | 45.51 | -22.60 | 128.16 | 0.4805 | -874.0 | 999999 | |
| 0.00 | 2.88 | 0.00 | 1.64 | -13.32 | 45.32 | -22.78 | 130.49 | 0.4975 | 109.0 | 82.2 | |
| 0.00 | 2.18 | 0.00 | 1.26 | -14.81 | 44.66 | -23.45 | 131.95 | 0.5193 | -717.0 | -545.7 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -15.13 | 44.45 | -23.65 | 132.19 | 0.5248 | -722.0 | -522.1 | |
| 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. | |