SDO HMI 2014-11-04 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.45 | 237.37 | 74.41 | 498.40 | 15.20 | 10.61 | -76.32 | 75.30 | 0.9683 | 65.1 | 154.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 1.23 | 18.72 | 12.55 | -74.38 | 71.66 | 0.9621 | -190.0 | -220.4 | |
| 17.97 | 100.46 | 27.52 | 154.37 | 14.81 | 15.36 | -71.57 | 75.71 | 0.9479 | -506.9 | -147.8 | |
| 0.00 | 0.78 | 0.00 | 1.48 | 14.86 | 11.45 | -75.48 | 75.68 | 0.9668 | 529.0 | 524.3 | |
| 1.90 | 107.98 | 3.75 | 249.50 | 14.70 | 10.86 | -76.07 | 75.84 | 0.9694 | 396.6 | 322.2 | |
| 1.73 | -4.00 | 3.38 | -4.00 | 14.53 | 11.04 | -75.89 | 76.02 | 0.9686 | 415.2 | 999999 | |
| 0.00 | 1.64 | 0.00 | 3.34 | 15.10 | 10.41 | -76.52 | 75.42 | 0.9712 | 439.0 | 352.9 | |
| 5.27 | -4.00 | 11.17 | -4.00 | 15.00 | 9.84 | -77.09 | 75.52 | 0.9734 | 610.7 | 999999 | |
| 0.00 | 1.73 | 0.00 | 4.44 | 16.76 | 7.39 | -79.54 | 73.70 | 0.9820 | 183.0 | 41.0 | |
| 2.16 | -4.00 | 5.29 | -4.00 | 16.26 | 7.84 | -79.09 | 74.21 | 0.9805 | 548.8 | 999999 | |
| 7.17 | -4.00 | 14.95 | -4.00 | 14.41 | 10.11 | -76.82 | 76.14 | 0.9724 | 257.3 | 999999 | |
| 0.00 | 2.33 | 0.00 | 9.18 | 17.73 | 3.32 | -83.61 | 72.62 | 0.9925 | -285.0 | -224.4 | |
| 0.00 | 0.26 | 0.00 | 0.74 | 16.49 | 6.18 | -80.75 | 73.95 | 0.9856 | 397.0 | 400.3 | |
| 2.25 | 11.23 | 8.35 | 41.07 | 17.19 | 3.70 | -83.23 | 73.17 | 0.9917 | 170.2 | 240.2 | |
| 0.00 | 0.60 | 0.00 | 1.49 | 14.84 | 7.92 | -79.02 | 75.66 | 0.9804 | 43.0 | 64.4 | |
| 0.00 | 9.67 | 0.00 | 31.56 | 15.96 | 4.86 | -82.07 | 74.45 | 0.9891 | 311.0 | 264.7 | |
| 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. | |