SDO HMI 2014-11-06 19:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.58 | 144.37 | 22.84 | 133.79 | 13.32 | 117.12 | 57.66 | 283.33 | 0.8467 | -496.7 | -236.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.14 | 123.65 | 20.02 | 117.06 | 13.94 | 117.89 | 58.43 | 284.03 | 0.8545 | -824.2 | -257.8 | |
| 0.00 | 0.86 | 0.00 | 0.74 | 13.07 | 113.84 | 54.39 | 283.35 | 0.8161 | -440.0 | -334.2 | |
| 0.00 | 2.42 | 0.00 | 1.98 | 7.73 | 112.38 | 52.93 | 276.81 | 0.7985 | -533.0 | -438.4 | |
| 0.60 | 9.41 | 0.50 | 7.68 | 8.00 | 112.38 | 52.93 | 277.15 | 0.7986 | -583.0 | -559.6 | |
| 1.98 | -4.00 | 1.62 | -4.00 | 8.15 | 112.36 | 52.91 | 277.34 | 0.7984 | -520.0 | 999999 | |
| 0.86 | -4.00 | 0.70 | -4.00 | 7.98 | 112.03 | 52.58 | 277.15 | 0.7949 | -616.0 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.78 | 11.91 | 112.30 | 52.84 | 282.06 | 0.7997 | 506.0 | 485.0 | |
| 0.00 | 0.69 | 0.00 | 0.57 | 12.93 | 112.45 | 52.99 | 283.32 | 0.8021 | 367.0 | 357.5 | |
| 0.00 | 1.21 | 0.00 | 0.95 | 8.44 | 110.70 | 51.24 | 277.78 | 0.7808 | 573.0 | 430.9 | |
| 0.00 | 0.78 | 0.00 | 0.62 | 11.97 | 111.17 | 51.71 | 282.25 | 0.7880 | 314.0 | 296.7 | |
| 0.00 | 0.86 | 0.00 | 0.68 | 11.10 | 110.41 | 50.95 | 281.21 | 0.7792 | 539.0 | 462.8 | |
| 0.00 | 2.59 | 0.00 | 1.99 | 8.06 | 109.53 | 50.08 | 277.32 | 0.7679 | 597.0 | 424.6 | |
| 0.00 | 0.95 | 0.00 | 0.74 | 10.82 | 110.10 | 50.64 | 280.87 | 0.7756 | 415.0 | 408.8 | |
| 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. | |