SDO HMI 2014-10-10 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.24 | 0.00 | 12.33 | 13.30 | 94.03 | 34.63 | 285.67 | 0.5748 | 63.9 | -88.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.24 | 0.00 | 2.21 | 10.33 | 102.99 | 43.59 | 278.51 | 0.6883 | -524.0 | -491.2 | |
| 0.00 | 0.79 | 0.00 | 0.53 | 11.00 | 101.77 | 42.37 | 279.56 | 0.6733 | -395.0 | -371.8 | |
| 0.00 | 1.49 | 0.00 | 0.99 | 11.00 | 101.36 | 41.96 | 279.59 | 0.6680 | -807.0 | -700.8 | |
| 0.00 | 1.31 | 0.00 | 0.84 | 12.46 | 98.56 | 39.16 | 282.17 | 0.6330 | -725.0 | -513.7 | |
| 0.00 | 3.07 | 0.00 | 1.87 | 10.77 | 95.31 | 35.91 | 279.85 | 0.5870 | -612.0 | -550.0 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 11.15 | 95.06 | 35.66 | 280.53 | 0.5840 | -574.0 | -423.7 | |
| 0.00 | 0.88 | 0.00 | 0.53 | 11.92 | 94.87 | 35.47 | 281.87 | 0.5824 | -572.0 | -504.9 | |
| 0.00 | 0.96 | 0.00 | 0.55 | 14.80 | 87.92 | 28.52 | 289.37 | 0.4914 | 641.0 | 528.0 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 14.00 | 87.39 | 27.99 | 288.03 | 0.4808 | 573.0 | 523.6 | |
| 0.00 | 0.35 | 0.00 | 0.21 | 22.18 | 88.72 | 29.32 | 302.45 | 0.5395 | 638.0 | 541.5 | |
| 0.00 | 1.40 | 0.00 | 0.79 | 15.39 | 86.99 | 27.59 | 291.04 | 0.4804 | 824.0 | 682.1 | |
| 0.00 | 2.37 | 0.00 | 1.33 | 19.76 | 85.30 | 25.90 | 300.79 | 0.4805 | 813.0 | 596.1 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 17.01 | 84.37 | 24.97 | 296.06 | 0.4512 | 787.0 | 622.3 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 16.68 | 82.74 | 23.35 | 296.66 | 0.4266 | 828.0 | 720.7 | |
| 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. | |