SDO HMI 2014-09-12 19:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.06 | 165.44 | 16.19 | 89.18 | -15.91 | 65.66 | 0.58 | 181.54 | 0.3961 | 513.3 | 380.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.23 | 147.02 | 7.67 | 79.15 | -15.88 | 66.55 | 1.47 | 183.60 | 0.3949 | 1168.4 | 509.1 | |
| 15.83 | -1.00 | 8.52 | -1.00 | -15.68 | 66.14 | 1.06 | 182.63 | 0.3914 | 1282.7 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.67 | -16.17 | 64.04 | -1.04 | 177.49 | 0.3993 | 773.0 | 566.4 | |
| 0.00 | 1.51 | 0.00 | 0.81 | -14.83 | 64.01 | -1.06 | 177.27 | 0.3776 | 861.0 | 663.9 | |
| 0.00 | 1.51 | 0.00 | 0.82 | -16.87 | 62.30 | -2.78 | 173.52 | 0.4126 | -828.0 | -698.3 | |
| 0.00 | 1.33 | 0.00 | 0.73 | -17.13 | 62.13 | -2.94 | 173.22 | 0.4171 | -770.0 | -642.7 | |
| 0.00 | 1.42 | 0.00 | 0.77 | -17.03 | 61.98 | -3.10 | 172.84 | 0.4158 | -898.0 | -729.0 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -16.58 | 60.95 | -4.13 | 170.30 | 0.4110 | -739.0 | -608.0 | |
| 0.00 | 1.87 | 0.00 | 1.03 | -18.69 | 59.90 | -5.17 | 168.94 | 0.4467 | -986.0 | -783.9 | |
| 0.00 | 1.96 | 0.00 | 1.04 | -13.78 | 59.91 | -5.16 | 166.29 | 0.3702 | -1073.0 | -877.8 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -19.02 | 59.77 | -5.31 | 168.80 | 0.4523 | -705.0 | -542.3 | |
| 0.00 | 1.07 | 0.00 | 0.61 | -22.07 | 58.74 | -6.34 | 168.18 | 0.5014 | 502.0 | 366.2 | |
| 0.00 | 2.67 | 0.00 | 1.45 | -16.25 | 57.99 | -7.09 | 163.41 | 0.4166 | -719.0 | -561.9 | |
| 0.00 | 1.96 | 0.00 | 1.08 | -17.60 | 56.56 | -8.51 | 161.37 | 0.4436 | -837.0 | -617.4 | |
| 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. | |