SDO HMI 2014-10-04 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 |
| 0.00 | 13.55 | 0.00 | 6.87 | -4.63 | 141.44 | -3.70 | 163.50 | 0.2188 | -350.9 | -267.1 | |
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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 | 0.62 | 0.00 | 0.31 | -4.70 | 148.80 | 3.66 | 198.02 | 0.2066 | 651.0 | 545.1 | |
| 0.00 | 1.76 | 0.00 | 0.89 | -3.99 | 148.37 | 3.24 | 197.06 | 0.1928 | 1087.0 | 883.6 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -4.27 | 148.29 | 3.15 | 196.21 | 0.1969 | 861.0 | 691.8 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -4.11 | 141.07 | -4.07 | 159.09 | 0.1994 | -883.0 | -776.5 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -4.67 | 140.13 | -5.01 | 155.92 | 0.2144 | -785.0 | -584.8 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -2.81 | 139.87 | -5.27 | 150.61 | 0.1878 | -874.0 | -727.5 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -5.44 | 139.73 | -5.41 | 155.70 | 0.2292 | -796.0 | -606.3 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -5.96 | 139.45 | -5.69 | 155.54 | 0.2393 | -895.0 | -660.1 | |
| 0.00 | 1.67 | 0.00 | 0.85 | -5.94 | 138.90 | -6.24 | 153.46 | 0.2429 | -700.0 | -580.5 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -4.86 | 136.88 | -8.26 | 144.07 | 0.2449 | -846.0 | -715.9 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -3.62 | 136.08 | -9.06 | 138.22 | 0.2370 | -680.0 | -523.6 | |
| 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. | |