SDO HMI 2014-10-05 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.23 | 33.03 | 6.22 | 21.65 | 13.40 | 91.24 | -40.70 | 77.20 | 0.6512 | 115.4 | 21.6 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.55 | 10.27 | 102.72 | -29.22 | 80.63 | 0.4888 | -649.0 | -565.8 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 9.75 | 102.63 | -29.31 | 81.70 | 0.4896 | -778.0 | -645.2 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 9.65 | 102.50 | -29.44 | 81.92 | 0.4914 | -667.0 | -506.0 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 12.46 | 98.84 | -33.10 | 77.19 | 0.5490 | -732.0 | -555.1 | |
| 0.00 | 1.76 | 0.00 | 1.06 | 14.49 | 97.18 | -34.77 | 74.04 | 0.5764 | -639.0 | -526.2 | |
| 0.00 | 1.85 | 0.00 | 1.11 | 7.86 | 97.11 | -34.83 | 85.63 | 0.5697 | -852.0 | -666.0 | |
| 0.00 | 1.93 | 0.00 | 1.20 | 10.98 | 95.01 | -36.94 | 80.39 | 0.6005 | -620.0 | -498.6 | |
| 0.00 | 1.23 | 0.00 | 0.76 | 11.29 | 94.62 | -37.33 | 79.93 | 0.6062 | -340.0 | -248.4 | |
| 0.00 | 1.14 | 0.00 | 0.76 | 14.39 | 90.32 | -41.62 | 75.67 | 0.6664 | -614.0 | -428.3 | |
| 0.00 | 1.14 | 0.00 | 0.78 | 16.26 | 88.84 | -43.10 | 73.17 | 0.6877 | 566.0 | 440.0 | |
| 9.23 | 13.71 | 6.22 | 9.24 | 13.26 | 89.07 | -42.88 | 77.52 | 0.6807 | 889.4 | 555.3 | |
| 0.00 | 1.32 | 0.00 | 0.89 | 13.41 | 88.69 | -43.25 | 77.34 | 0.6854 | 474.0 | 384.6 | |
| 0.00 | 2.72 | 0.00 | 1.90 | 14.87 | 87.04 | -44.90 | 75.46 | 0.7072 | 710.0 | 574.3 | |
| 0.00 | 1.49 | 0.00 | 1.09 | 19.61 | 85.26 | -46.68 | 69.24 | 0.7353 | 417.0 | 320.8 | |
| 0.00 | 0.70 | 0.00 | 0.54 | 22.15 | 82.84 | -49.10 | 66.43 | 0.7661 | 525.0 | 453.4 | |
| 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. | |