SDO HMI 2014-05-31 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.57 | 72.63 | 13.57 | 38.35 | -9.07 | 24.47 | 18.37 | 244.59 | 0.3458 | 561.6 | 307.8 | |
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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 |
| 0.45 | 13.64 | 0.24 | 7.28 | -8.91 | 26.61 | 20.52 | 247.60 | 0.3761 | 858.4 | 717.2 | |
| 2.98 | -1.00 | 1.59 | -1.00 | -8.64 | 26.43 | 20.34 | 248.13 | 0.3718 | 1042.2 | 999999 | |
| 22.14 | 40.12 | 11.74 | 21.26 | -8.89 | 25.40 | 19.30 | 246.48 | 0.3577 | 1102.6 | 617.3 | |
| 0.00 | 2.26 | 0.00 | 1.19 | -10.31 | 23.50 | 17.40 | 240.49 | 0.3395 | 719.0 | 632.2 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -9.94 | 23.25 | 17.15 | 241.13 | 0.3331 | 747.0 | 557.9 | |
| 0.00 | 2.17 | 0.00 | 1.14 | -10.06 | 23.03 | 16.93 | 240.50 | 0.3309 | 972.0 | 780.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -9.17 | 20.65 | 14.55 | 239.38 | 0.2895 | -753.0 | -611.9 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -8.22 | 20.52 | 14.42 | 242.13 | 0.2801 | -860.0 | -692.3 | |
| 0.00 | 2.35 | 0.00 | 1.21 | -9.20 | 20.52 | 14.43 | 239.07 | 0.2880 | -860.0 | -710.9 | |
| 0.00 | 2.80 | 0.00 | 1.45 | -8.59 | 20.47 | 14.37 | 240.88 | 0.2822 | -940.0 | -775.4 | |
| 0.00 | 4.34 | 0.00 | 2.24 | -9.42 | 20.28 | 14.18 | 238.00 | 0.2863 | -780.0 | -636.6 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -14.28 | 20.21 | 14.11 | 225.24 | 0.3342 | 748.0 | 616.9 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -10.88 | 14.13 | 8.03 | 217.95 | 0.2240 | -861.0 | -642.4 | |
| 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. | |