SDO HMI 2014-10-10 10:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.47 | 0.00 | 9.78 | 13.65 | 92.40 | 31.90 | 287.34 | 0.5368 | 217.9 | 102.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.49 | 0.00 | 1.00 | 10.33 | 103.01 | 42.52 | 278.55 | 0.6747 | -611.0 | -514.9 | |
| 0.00 | 0.79 | 0.00 | 0.52 | 11.02 | 101.82 | 41.32 | 279.67 | 0.6598 | -520.0 | -411.3 | |
| 0.00 | 2.28 | 0.00 | 1.49 | 11.11 | 101.35 | 40.85 | 279.86 | 0.6538 | -693.0 | -584.7 | |
| 0.00 | 1.14 | 0.00 | 0.72 | 12.45 | 98.52 | 38.02 | 282.32 | 0.6180 | -777.0 | -583.5 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 10.76 | 95.29 | 34.79 | 279.97 | 0.5714 | -503.0 | -433.6 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 13.99 | 91.25 | 30.76 | 286.85 | 0.5206 | 611.0 | 544.2 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 12.38 | 89.09 | 28.59 | 284.46 | 0.4847 | 736.0 | 573.8 | |
| 0.00 | 1.93 | 0.00 | 1.08 | 13.94 | 87.37 | 26.87 | 288.43 | 0.4644 | 566.0 | 383.4 | |
| 0.00 | 1.75 | 0.00 | 0.98 | 15.33 | 87.00 | 26.50 | 291.52 | 0.4646 | 862.0 | 786.0 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 19.76 | 85.31 | 24.81 | 301.70 | 0.4661 | 752.0 | 653.6 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 17.01 | 84.33 | 23.84 | 296.94 | 0.4354 | 839.0 | 683.8 | |
| 0.00 | 1.49 | 0.00 | 0.81 | 16.62 | 82.72 | 22.22 | 297.49 | 0.4103 | 847.0 | 662.9 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 17.07 | 82.13 | 21.64 | 299.06 | 0.4050 | 724.0 | 556.1 | |
| 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. | |