SDO HMI 2014-07-06 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.45 | 14.71 | 0.75 | 7.67 | 7.14 | 260.37 | 16.84 | 283.95 | 0.2972 | 678.3 | 555.7 | |
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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 | 1.00 | 0.00 | 0.57 | 1.18 | 272.46 | 28.93 | 266.17 | 0.4866 | -577.0 | -445.5 | |
| 0.00 | 0.27 | 0.00 | 0.15 | 13.05 | 270.64 | 27.11 | 291.29 | 0.4784 | 737.0 | 701.7 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 9.35 | 269.71 | 26.18 | 284.01 | 0.4505 | 670.0 | 511.6 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 7.90 | 260.75 | 17.22 | 285.27 | 0.3052 | 854.0 | 633.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 8.21 | 260.57 | 17.04 | 286.40 | 0.3036 | 782.0 | 602.3 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 7.70 | 260.51 | 16.98 | 284.77 | 0.3007 | 858.0 | 625.9 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 5.62 | 260.40 | 16.87 | 277.92 | 0.2929 | 782.0 | 613.2 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 8.23 | 259.60 | 16.07 | 287.31 | 0.2883 | 822.0 | 664.9 | |
| 1.45 | 3.81 | 0.75 | 1.97 | 8.39 | 259.35 | 15.83 | 288.07 | 0.2850 | 1039.8 | 804.9 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 3.55 | 251.46 | 7.94 | 270.86 | 0.1384 | 772.0 | 611.9 | |
| 0.00 | 0.64 | 0.00 | 0.32 | 7.70 | 251.15 | 7.63 | 299.49 | 0.1518 | 807.0 | 735.4 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 6.61 | 250.39 | 6.86 | 294.96 | 0.1315 | 683.0 | 504.9 | |
| 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. | |