SDO HMI 2014-10-10 03:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.91 | 352.43 | 47.79 | 286.33 | -20.58 | 18.53 | -45.79 | 122.05 | 0.7940 | 895.1 | 239.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.48 | -20.27 | 20.53 | -43.79 | 122.77 | 0.7744 | 711.0 | 664.1 | |
| 0.00 | 1.32 | 0.00 | 1.01 | -19.20 | 20.68 | -43.64 | 121.61 | 0.7676 | 510.0 | 351.9 | |
| 0.00 | 5.08 | 0.00 | 3.99 | -20.40 | 20.17 | -44.15 | 122.72 | 0.7783 | 754.0 | 727.8 | |
| 2.89 | 329.46 | 2.30 | 267.99 | -20.49 | 19.42 | -44.91 | 122.42 | 0.7857 | 1010.1 | 233.7 | |
| 0.00 | 1.67 | 0.00 | 1.31 | -19.37 | 19.47 | -44.86 | 121.15 | 0.7798 | 500.0 | 429.1 | |
| 0.00 | 1.49 | 0.00 | 1.15 | -17.88 | 19.66 | -44.67 | 119.51 | 0.7710 | 661.0 | 597.4 | |
| 53.04 | -4.00 | 43.11 | -4.00 | -20.67 | 18.48 | -45.84 | 122.13 | 0.7949 | 1063.4 | 999999 | |
| 1.58 | 4.65 | 1.23 | 3.62 | -17.77 | 19.38 | -44.94 | 119.24 | 0.7732 | 710.7 | 411.3 | |
| 0.96 | -4.00 | 0.80 | -4.00 | -21.19 | 17.86 | -46.47 | 122.40 | 0.8029 | 244.5 | 999999 | |
| 0.00 | 1.49 | 0.00 | 1.31 | -23.71 | 16.33 | -47.99 | 124.42 | 0.8269 | 580.0 | 467.9 | |
| 0.00 | 2.02 | 0.00 | 1.62 | -17.80 | 17.84 | -46.49 | 118.50 | 0.7881 | 185.0 | 215.7 | |
| 0.44 | 1.84 | 0.35 | 1.45 | -16.78 | 18.04 | -46.29 | 117.40 | 0.7818 | -642.8 | -551.0 | |
| 0.00 | 1.84 | 0.00 | 1.48 | -17.95 | 17.55 | -46.77 | 118.55 | 0.7914 | -312.0 | -363.3 | |
| 0.00 | 0.96 | 0.00 | 0.92 | -22.49 | 12.06 | -52.27 | 121.15 | 0.8559 | -232.0 | -314.0 | |
| 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. | |