SDO HMI 2014-10-05 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.88 | 0.00 | 8.81 | -13.25 | 138.62 | 17.66 | 221.54 | 0.4485 | -62.4 | -106.2 | |
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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 | 1.32 | 0.00 | 0.75 | -13.66 | 143.30 | 22.34 | 227.69 | 0.5015 | 634.0 | 433.0 | |
| 0.00 | 1.32 | 0.00 | 0.76 | -15.14 | 142.65 | 21.69 | 224.68 | 0.5095 | 536.0 | 458.3 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -11.97 | 141.56 | 20.60 | 228.04 | 0.4649 | 687.0 | 512.6 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -10.16 | 140.36 | 19.40 | 229.41 | 0.4324 | 561.0 | 484.2 | |
| 0.00 | 2.37 | 0.00 | 1.34 | -15.71 | 139.46 | 18.50 | 219.37 | 0.4835 | -735.0 | -639.7 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -10.17 | 138.15 | 17.19 | 225.92 | 0.4067 | 674.0 | 484.7 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -10.18 | 137.67 | 16.71 | 225.09 | 0.4014 | 642.0 | 392.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -12.10 | 136.67 | 15.71 | 220.08 | 0.4129 | -673.0 | -431.8 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -15.89 | 136.35 | 15.39 | 214.11 | 0.4571 | -732.0 | -575.6 | |
| 0.00 | 0.61 | 0.00 | 0.33 | -12.51 | 135.77 | 14.81 | 217.78 | 0.4090 | -775.0 | -644.1 | |
| 0.00 | 2.20 | 0.00 | 1.18 | -11.55 | 135.46 | 14.50 | 218.71 | 0.3941 | -1008.0 | -768.9 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -18.45 | 133.44 | 12.48 | 206.06 | 0.4686 | -560.0 | -461.7 | |
| 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. | |