SDO HMI 2014-10-05 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.53 | 18.02 | 0.45 | 13.67 | 11.05 | 169.82 | 49.42 | 279.34 | 0.7552 | 142.3 | 72.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 1.06 | 8.56 | 175.82 | 55.42 | 275.92 | 0.8207 | -493.0 | -415.6 | |
| 0.00 | 1.14 | 0.00 | 0.97 | 8.57 | 175.40 | 54.99 | 275.92 | 0.8165 | -566.0 | -548.9 | |
| 0.53 | 2.99 | 0.45 | 2.53 | 9.23 | 175.17 | 54.77 | 276.72 | 0.8140 | -553.5 | -500.3 | |
| 0.00 | 0.97 | 0.00 | 0.82 | 9.39 | 175.00 | 54.60 | 276.92 | 0.8123 | -594.0 | -532.2 | |
| 0.00 | 0.26 | 0.00 | 0.21 | 9.20 | 172.85 | 52.44 | 276.62 | 0.7901 | 344.0 | 344.7 | |
| 0.00 | 1.67 | 0.00 | 1.32 | 8.43 | 172.25 | 51.84 | 275.63 | 0.7838 | 552.0 | 530.2 | |
| 0.00 | 0.97 | 0.00 | 0.73 | 10.90 | 170.01 | 49.61 | 278.81 | 0.7591 | 365.0 | 370.3 | |
| 0.00 | 0.97 | 0.00 | 0.72 | 12.10 | 169.03 | 48.63 | 280.45 | 0.7484 | -509.0 | -493.0 | |
| 0.00 | 1.76 | 0.00 | 1.25 | 12.89 | 166.49 | 46.09 | 281.69 | 0.7194 | 564.0 | 427.9 | |
| 0.00 | 0.97 | 0.00 | 0.66 | 11.82 | 163.87 | 43.46 | 280.38 | 0.6868 | 659.0 | 555.4 | |
| 0.00 | 1.23 | 0.00 | 0.83 | 11.97 | 163.60 | 43.20 | 280.61 | 0.6836 | 596.0 | 576.9 | |
| 0.00 | 1.23 | 0.00 | 0.83 | 11.99 | 163.35 | 42.95 | 280.66 | 0.6805 | 685.0 | 540.1 | |
| 0.00 | 1.14 | 0.00 | 0.78 | 19.66 | 163.30 | 42.90 | 291.79 | 0.6927 | 608.0 | 451.4 | |
| 0.00 | 1.49 | 0.00 | 0.96 | 14.35 | 160.18 | 39.78 | 284.65 | 0.6430 | 648.0 | 569.6 | |
| 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. | |