SDO HMI 2014-05-31 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.69 | 54.90 | 10.30 | 30.04 | -9.10 | 24.23 | 23.65 | 249.49 | 0.4252 | 476.6 | 230.1 | |
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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 | 1.63 | 0.00 | 0.91 | -8.81 | 26.66 | 26.07 | 251.92 | 0.4588 | 769.0 | 629.0 | |
| 0.00 | 4.24 | 0.00 | 2.36 | -8.56 | 26.60 | 26.02 | 252.41 | 0.4570 | 938.0 | 760.4 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -11.06 | 26.02 | 25.44 | 246.82 | 0.4605 | 718.0 | 484.7 | |
| 18.69 | 29.53 | 10.30 | 16.27 | -8.81 | 25.39 | 24.81 | 251.13 | 0.4401 | 1036.3 | 630.3 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -9.98 | 24.43 | 23.85 | 247.88 | 0.4317 | 365.0 | 343.1 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -10.05 | 24.13 | 23.55 | 247.50 | 0.4276 | 744.0 | 644.3 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -9.86 | 23.88 | 23.30 | 247.71 | 0.4230 | 810.0 | 659.2 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -10.02 | 23.69 | 23.11 | 247.21 | 0.4210 | 794.0 | 544.1 | |
| 0.00 | 4.79 | 0.00 | 2.55 | -9.14 | 20.81 | 20.23 | 246.71 | 0.3733 | -840.0 | -752.5 | |
| 0.00 | 1.72 | 0.00 | 0.91 | -4.37 | 20.48 | 19.90 | 259.29 | 0.3469 | -839.0 | -593.8 | |
| 0.00 | 1.72 | 0.00 | 0.91 | -8.80 | 20.53 | 19.95 | 247.29 | 0.3671 | -961.0 | -716.6 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -9.60 | 20.45 | 19.87 | 245.19 | 0.3707 | -769.0 | -607.6 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -9.91 | 19.91 | 19.33 | 243.83 | 0.3648 | -639.0 | -495.2 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -17.27 | 18.39 | 17.81 | 225.66 | 0.4100 | 636.0 | 513.6 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -13.64 | 13.21 | 12.63 | 223.53 | 0.3099 | -818.0 | -674.7 | |
| 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. | |