SDO HMI 2014-11-14 03:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.72 | 52.31 | 11.59 | 34.56 | 8.58 | 3.99 | 41.24 | 279.64 | 0.6634 | 18.8 | -282.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 0.94 | 8.34 | 6.44 | 43.69 | 278.95 | 0.6942 | -594.0 | -478.9 | |
| 0.00 | 2.15 | 0.00 | 1.46 | 8.39 | 5.74 | 42.99 | 279.11 | 0.6856 | -552.0 | -402.0 | |
| 0.00 | 2.67 | 0.00 | 1.80 | 8.38 | 5.37 | 42.62 | 279.13 | 0.6809 | -630.0 | -531.4 | |
| 7.14 | 18.67 | 4.80 | 12.55 | 8.12 | 5.17 | 42.42 | 278.77 | 0.6781 | -851.2 | -589.9 | |
| 0.00 | 5.59 | 0.00 | 3.71 | 8.17 | 4.41 | 41.66 | 278.94 | 0.6684 | -348.0 | -672.6 | |
| 0.00 | 1.12 | 0.00 | 0.74 | 8.06 | 4.20 | 41.44 | 278.80 | 0.6655 | -929.0 | -721.2 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 8.27 | 4.06 | 41.31 | 279.14 | 0.6640 | -498.0 | -438.8 | |
| 0.00 | 1.20 | 0.00 | 0.79 | 9.55 | 3.56 | 40.81 | 281.14 | 0.6592 | 549.0 | 462.3 | |
| 0.00 | 0.60 | 0.00 | 0.39 | 9.56 | 3.09 | 40.33 | 281.24 | 0.6531 | 431.0 | 378.3 | |
| 0.00 | 1.38 | 0.00 | 0.89 | 9.41 | 2.43 | 39.68 | 281.12 | 0.6443 | 548.0 | 451.6 | |
| 1.20 | 2.32 | 0.78 | 1.50 | 10.04 | 2.21 | 39.46 | 282.14 | 0.6424 | 865.7 | 720.5 | |
| 0.00 | 1.03 | 0.00 | 0.67 | 10.22 | 2.20 | 39.45 | 282.43 | 0.6426 | 706.0 | 596.8 | |
| 1.81 | 3.36 | 1.16 | 2.16 | 9.51 | 2.02 | 39.27 | 281.35 | 0.6390 | 864.9 | 721.1 | |
| 7.57 | 9.81 | 4.85 | 6.28 | 8.83 | 1.81 | 39.06 | 280.32 | 0.6352 | 851.5 | 606.9 | |
| 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. | |