SDO HMI 2014-09-09 18:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.27 | 71.35 | 20.70 | 47.16 | 9.61 | 147.09 | 41.85 | 276.32 | 0.6638 | 70.7 | -38.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.74 | 5.52 | 2.62 | 3.87 | 9.70 | 150.76 | 45.52 | 276.49 | 0.7102 | -670.3 | -466.0 | |
| 0.89 | 1.78 | 0.62 | 1.25 | 10.07 | 150.70 | 45.46 | 277.01 | 0.7094 | -637.5 | -528.9 | |
| 0.00 | 1.60 | 0.00 | 1.12 | 9.21 | 150.42 | 45.18 | 275.79 | 0.7060 | -613.0 | -438.6 | |
| 0.71 | 25.30 | 0.48 | 16.98 | 10.17 | 148.48 | 43.24 | 277.17 | 0.6819 | -337.8 | -602.6 | |
| 5.17 | -4.00 | 3.48 | -4.00 | 10.01 | 148.24 | 43.00 | 276.93 | 0.6788 | -766.2 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.84 | 9.66 | 148.10 | 42.86 | 276.41 | 0.6770 | -681.0 | -532.3 | |
| 2.05 | -4.00 | 1.37 | -4.00 | 10.21 | 148.06 | 42.82 | 277.22 | 0.6766 | -757.7 | 999999 | |
| 2.05 | -4.00 | 1.37 | -4.00 | 10.20 | 147.81 | 42.57 | 277.21 | 0.6734 | -852.6 | 999999 | |
| 11.76 | 17.19 | 7.61 | 11.13 | 9.31 | 145.70 | 40.46 | 275.87 | 0.6460 | 724.3 | 472.1 | |
| 0.98 | 2.85 | 0.63 | 1.84 | 9.56 | 145.33 | 40.09 | 276.25 | 0.6412 | 737.3 | 610.4 | |
| 3.92 | 11.05 | 2.52 | 7.09 | 9.20 | 145.24 | 40.00 | 275.69 | 0.6400 | 953.3 | 711.1 | |
| 0.00 | 0.89 | 0.00 | 0.57 | 9.48 | 145.12 | 39.88 | 276.13 | 0.6384 | 785.0 | 598.7 | |
| 0.00 | 0.98 | 0.00 | 0.63 | 9.82 | 145.13 | 39.89 | 276.66 | 0.6385 | 584.0 | 405.4 | |
| 0.00 | 0.89 | 0.00 | 0.56 | 8.94 | 143.59 | 38.35 | 275.26 | 0.6177 | 459.0 | 432.2 | |
| 0.00 | 2.05 | 0.00 | 1.28 | 7.82 | 143.11 | 37.87 | 273.42 | 0.6114 | 569.0 | 409.9 | |
| 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. | |