SDO HMI 2014-07-07 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 |
| 2.00 | 16.80 | 1.23 | 10.53 | -21.56 | 201.75 | -28.54 | 133.54 | 0.6136 | -44.2 | -39.2 | |
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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 | 0.61 | -23.87 | 207.57 | -22.73 | 142.26 | 0.5794 | -701.0 | -587.3 | |
| 0.00 | 1.63 | 0.00 | 0.99 | -21.68 | 205.37 | -24.92 | 137.10 | 0.5773 | 759.0 | 548.7 | |
| 0.00 | 1.36 | 0.00 | 0.82 | -21.32 | 205.15 | -25.14 | 136.39 | 0.5759 | 813.0 | 615.1 | |
| 2.00 | 3.99 | 1.23 | 2.46 | -22.95 | 204.72 | -25.57 | 137.97 | 0.5959 | -860.6 | -685.0 | |
| 0.00 | 0.91 | 0.00 | 0.55 | -21.49 | 204.98 | -25.32 | 136.42 | 0.5793 | 667.0 | 574.9 | |
| 0.00 | 2.09 | 0.00 | 1.29 | -20.70 | 202.13 | -28.17 | 132.47 | 0.6008 | 635.0 | 598.3 | |
| 0.00 | 0.91 | 0.00 | 0.58 | -22.56 | 199.75 | -30.55 | 132.66 | 0.6405 | 506.0 | 428.6 | |
| 0.00 | 0.82 | 0.00 | 0.51 | -19.93 | 200.20 | -30.09 | 129.67 | 0.6146 | -521.0 | -497.7 | |
| 0.00 | 1.36 | 0.00 | 0.88 | -18.39 | 196.15 | -34.14 | 124.33 | 0.6472 | -713.0 | -620.0 | |
| 0.00 | 0.82 | 0.00 | 0.55 | -21.30 | 195.22 | -35.07 | 127.45 | 0.6767 | -599.0 | -512.9 | |
| 0.00 | 1.91 | 0.00 | 1.29 | -21.25 | 194.79 | -35.50 | 127.08 | 0.6807 | -284.0 | -367.4 | |
| 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. | |