SDO HMI 2014-07-03 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.63 | 16.62 | 1.06 | 10.32 | -12.65 | 252.92 | -33.64 | 115.97 | 0.6032 | 274.2 | 248.1 | |
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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 | 1.00 | 0.00 | 0.59 | -11.12 | 257.47 | -29.09 | 116.63 | 0.5358 | 744.0 | 559.0 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -12.57 | 256.25 | -30.31 | 118.11 | 0.5606 | 650.0 | 599.4 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -15.40 | 255.20 | -31.36 | 121.71 | 0.5920 | 664.0 | 567.7 | |
| 0.00 | 3.00 | 0.00 | 1.81 | -12.56 | 255.31 | -31.26 | 117.41 | 0.5727 | 699.0 | 537.4 | |
| 0.00 | 0.73 | 0.00 | 0.44 | -11.73 | 254.69 | -31.88 | 115.65 | 0.5758 | 726.0 | 619.0 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -11.54 | 254.60 | -31.96 | 115.29 | 0.5758 | 671.0 | 563.1 | |
| 0.00 | 0.82 | 0.00 | 0.50 | -9.63 | 252.50 | -34.06 | 110.96 | 0.5935 | 437.0 | 375.1 | |
| 0.00 | 0.82 | 0.00 | 0.53 | -15.21 | 250.04 | -36.52 | 117.91 | 0.6521 | -654.0 | -635.6 | |
| 0.00 | 2.63 | 0.00 | 1.65 | -9.87 | 250.89 | -35.68 | 110.49 | 0.6156 | 584.0 | 378.4 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -14.95 | 249.98 | -36.59 | 117.51 | 0.6515 | -593.0 | -575.3 | |
| 1.63 | 3.72 | 1.06 | 2.43 | -14.79 | 249.93 | -36.63 | 117.26 | 0.6512 | -844.2 | -669.4 | |
| 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. | |