SDO HMI 2014-10-12 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.20 | 0.00 | 11.41 | -21.67 | 69.74 | 36.17 | 230.65 | 0.7134 | -177.9 | -228.1 | |
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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 | 1.05 | 0.00 | 0.79 | -16.79 | 77.31 | 43.75 | 241.45 | 0.7560 | 513.0 | 483.8 | |
| 0.00 | 1.40 | 0.00 | 1.04 | -16.67 | 76.54 | 42.98 | 241.19 | 0.7477 | 725.0 | 580.9 | |
| 0.00 | 1.23 | 0.00 | 0.90 | -19.38 | 74.11 | 40.55 | 236.52 | 0.7376 | 578.0 | 471.1 | |
| 0.00 | 1.66 | 0.00 | 1.16 | -16.21 | 72.93 | 39.37 | 239.70 | 0.7078 | 563.0 | 326.4 | |
| 0.00 | 0.88 | 0.00 | 0.61 | -22.47 | 69.20 | 35.63 | 229.53 | 0.7100 | -416.0 | -392.3 | |
| 0.00 | 4.46 | 0.00 | 3.12 | -23.55 | 68.13 | 34.56 | 227.47 | 0.7081 | -789.0 | -671.8 | |
| 0.00 | 0.79 | 0.00 | 0.55 | -24.23 | 68.02 | 34.45 | 226.62 | 0.7121 | -466.0 | -397.6 | |
| 0.00 | 0.96 | 0.00 | 0.67 | -23.67 | 67.80 | 34.24 | 227.09 | 0.7060 | -767.0 | -624.8 | |
| 0.00 | 1.05 | 0.00 | 0.74 | -24.15 | 67.75 | 34.19 | 226.51 | 0.7091 | -504.0 | -451.2 | |
| 0.00 | 1.58 | 0.00 | 1.09 | -24.30 | 66.89 | 33.32 | 225.65 | 0.7026 | -668.0 | -547.3 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -26.64 | 58.19 | 24.63 | 215.02 | 0.6514 | -726.0 | -656.5 | |
| 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. | |