SDO HMI 2014-10-05 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.44 | 32.07 | 5.22 | 19.35 | 13.31 | 91.68 | -34.24 | 76.16 | 0.5654 | 144.6 | 82.4 | |
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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 | 0.52 | 10.00 | 103.52 | -22.39 | 79.50 | 0.3832 | -650.0 | -599.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 9.42 | 102.67 | -23.24 | 81.22 | 0.3956 | -810.0 | -655.0 | |
| 0.00 | 1.32 | 0.00 | 0.71 | 9.44 | 102.41 | -23.51 | 81.23 | 0.3998 | -750.0 | -576.5 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 12.42 | 99.10 | -26.82 | 75.35 | 0.4573 | -737.0 | -471.8 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 10.80 | 96.36 | -29.56 | 79.52 | 0.4948 | -653.0 | -524.3 | |
| 0.00 | 0.97 | 0.00 | 0.55 | 8.19 | 96.46 | -29.46 | 84.83 | 0.4907 | -498.0 | -405.0 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 10.74 | 95.30 | -30.61 | 79.84 | 0.5103 | -644.0 | -532.6 | |
| 0.00 | 3.43 | 0.00 | 1.98 | 11.00 | 94.99 | -30.93 | 79.41 | 0.5153 | -613.0 | -540.0 | |
| 0.00 | 1.49 | 0.00 | 0.94 | 19.45 | 88.89 | -37.03 | 66.60 | 0.6210 | 683.0 | 539.4 | |
| 0.00 | 1.05 | 0.00 | 0.68 | 21.28 | 87.84 | -38.08 | 64.21 | 0.6405 | 626.0 | 555.5 | |
| 0.00 | 1.41 | 0.00 | 0.88 | 16.44 | 89.06 | -36.85 | 71.32 | 0.6094 | 559.0 | 526.2 | |
| 8.44 | 14.33 | 5.22 | 8.86 | 13.21 | 89.16 | -36.76 | 76.58 | 0.6012 | 874.9 | 600.5 | |
| 0.00 | 1.14 | 0.00 | 0.71 | 13.37 | 88.71 | -37.21 | 76.42 | 0.6075 | 523.0 | 436.8 | |
| 0.00 | 1.14 | 0.00 | 0.72 | 13.38 | 88.08 | -37.84 | 76.51 | 0.6160 | 595.0 | 513.2 | |
| 0.00 | 0.70 | 0.00 | 0.48 | 22.20 | 83.37 | -42.55 | 64.53 | 0.6958 | 582.0 | 454.0 | |
| 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. | |