SDO HMI 2014-11-13 22:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.47 | 57.02 | 12.86 | 36.03 | 8.60 | 3.70 | 38.20 | 280.10 | 0.6232 | 36.3 | -157.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.41 | 0.00 | 1.58 | 8.27 | 6.20 | 40.70 | 279.17 | 0.6560 | -628.0 | -468.1 | |
| 0.95 | 3.18 | 0.61 | 2.06 | 8.38 | 5.51 | 40.00 | 279.44 | 0.6470 | -656.2 | -513.2 | |
| 0.00 | 2.15 | 0.00 | 1.39 | 7.94 | 5.14 | 39.64 | 278.81 | 0.6416 | -322.0 | -387.5 | |
| 0.00 | 2.06 | 0.00 | 1.33 | 8.13 | 5.08 | 39.58 | 279.10 | 0.6411 | -479.0 | -457.5 | |
| 9.46 | 21.85 | 6.05 | 13.94 | 8.08 | 4.54 | 39.03 | 279.11 | 0.6338 | -928.9 | -593.0 | |
| 0.00 | 1.81 | 0.00 | 1.14 | 8.25 | 3.98 | 38.47 | 279.46 | 0.6265 | -751.0 | -566.4 | |
| 0.00 | 1.29 | 0.00 | 0.81 | 9.58 | 3.49 | 37.99 | 281.67 | 0.6220 | 575.0 | 453.6 | |
| 0.00 | 0.86 | 0.00 | 0.54 | 8.98 | 2.66 | 37.15 | 280.87 | 0.6097 | -215.0 | -164.7 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 9.65 | 2.44 | 36.93 | 282.00 | 0.6079 | 364.0 | 441.8 | |
| 0.60 | 2.58 | 0.37 | 1.60 | 9.26 | 2.31 | 36.81 | 281.40 | 0.6055 | 625.0 | 523.2 | |
| 0.00 | 2.41 | 0.00 | 1.50 | 9.89 | 2.28 | 36.78 | 282.44 | 0.6062 | 872.0 | 693.4 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 9.66 | 2.14 | 36.63 | 282.08 | 0.6038 | 601.0 | 542.7 | |
| 0.00 | 2.41 | 0.00 | 1.49 | 10.11 | 2.16 | 36.65 | 282.82 | 0.6050 | 789.0 | 517.3 | |
| 9.46 | 12.47 | 5.83 | 7.69 | 8.98 | 1.79 | 36.29 | 281.04 | 0.5978 | 896.0 | 595.2 | |
| 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. | |