SDO HMI 2014-10-11 13:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.54 | 468.37 | 41.83 | 294.88 | -20.55 | 18.08 | -27.58 | 135.27 | 0.6181 | 866.0 | 281.5 | |
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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 | 1.31 | 0.00 | 0.82 | -21.85 | 20.40 | -25.26 | 139.24 | 0.6089 | -668.0 | -625.1 | |
| 0.00 | 1.58 | 0.00 | 0.98 | -21.34 | 20.46 | -25.20 | 138.72 | 0.6033 | -708.0 | -560.4 | |
| 0.00 | 0.44 | 0.00 | 0.27 | -21.72 | 20.17 | -25.48 | 138.85 | 0.6097 | -603.0 | -494.0 | |
| 0.00 | 2.01 | 0.00 | 1.22 | -18.29 | 20.35 | -25.31 | 134.84 | 0.5745 | 777.0 | 638.3 | |
| 1.66 | 4.82 | 1.01 | 2.92 | -18.37 | 20.09 | -25.56 | 134.65 | 0.5779 | 899.7 | 732.4 | |
| 0.00 | 2.28 | 0.00 | 1.39 | -18.77 | 19.96 | -25.70 | 135.02 | 0.5831 | 676.0 | 600.5 | |
| 0.70 | 447.96 | 0.44 | 282.20 | -20.43 | 19.13 | -26.53 | 136.21 | 0.6070 | 1004.8 | 280.7 | |
| 0.00 | 2.71 | 0.00 | 1.68 | -19.86 | 19.24 | -26.42 | 135.62 | 0.6005 | 942.0 | 649.2 | |
| 0.00 | 1.84 | 0.00 | 1.12 | -18.53 | 19.44 | -26.22 | 134.15 | 0.5861 | 761.0 | 645.2 | |
| 3.15 | -7.00 | 1.96 | -7.00 | -20.32 | 18.80 | -26.86 | 135.71 | 0.6091 | 1259.2 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -19.28 | 18.99 | -26.67 | 134.63 | 0.5975 | 149.0 | 114.9 | |
| 60.77 | -7.00 | 38.25 | -7.00 | -20.59 | 17.99 | -27.67 | 135.22 | 0.6194 | 1081.7 | 999999 | |
| 0.26 | -7.00 | 0.17 | -7.00 | -21.01 | 17.58 | -28.08 | 135.32 | 0.6272 | 501.7 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.68 | -20.60 | 15.35 | -30.31 | 132.70 | 0.6451 | 519.0 | 416.8 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -21.47 | 12.99 | -32.66 | 131.70 | 0.6750 | -664.0 | -452.2 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -26.28 | 9.70 | -35.96 | 134.51 | 0.7407 | -485.0 | -439.3 | |
| 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. | |