SDO HMI 2014-05-19 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.74 | 40.76 | 6.36 | 33.07 | -18.16 | 217.45 | 50.95 | 248.64 | 0.7943 | -70.8 | -92.4 | |
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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 |
| 3.42 | 19.79 | 2.85 | 16.44 | -18.42 | 218.56 | 52.06 | 248.59 | 0.8059 | 661.1 | 178.4 | |
| 0.99 | 1.89 | 0.82 | 1.56 | -18.01 | 218.39 | 51.88 | 249.05 | 0.8034 | 692.6 | 519.7 | |
| 1.53 | -1.00 | 1.27 | -1.00 | -18.46 | 218.27 | 51.76 | 248.47 | 0.8031 | 747.5 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.39 | -18.74 | 217.51 | 51.00 | 247.95 | 0.7963 | -363.0 | -334.5 | |
| 0.00 | 1.71 | 0.00 | 1.39 | -18.86 | 217.46 | 50.95 | 247.78 | 0.7961 | -640.0 | -475.7 | |
| 0.00 | 1.62 | 0.00 | 1.26 | -15.77 | 216.05 | 49.54 | 251.31 | 0.7753 | -687.0 | -455.7 | |
| 0.00 | 2.88 | 0.00 | 2.32 | -18.65 | 217.06 | 50.56 | 247.94 | 0.7917 | -719.0 | -536.3 | |
| 0.00 | 0.54 | 0.00 | 0.42 | -16.59 | 216.13 | 49.62 | 250.29 | 0.7778 | -485.0 | -450.7 | |
| 0.81 | 2.97 | 0.65 | 2.37 | -18.38 | 216.55 | 50.05 | 248.15 | 0.7860 | -548.0 | -390.1 | |
| 0.00 | 1.08 | 0.00 | 0.86 | -18.36 | 216.24 | 49.74 | 248.10 | 0.7829 | -195.0 | -215.3 | |
| 0.99 | 2.16 | 0.77 | 1.67 | -17.14 | 215.40 | 48.89 | 249.41 | 0.7714 | -313.2 | -290.9 | |
| 0.00 | 1.44 | 0.00 | 1.12 | -17.40 | 215.49 | 48.98 | 249.11 | 0.7729 | -488.0 | -324.2 | |
| 0.00 | 1.71 | 0.00 | 1.32 | -17.43 | 215.26 | 48.75 | 249.01 | 0.7706 | -775.0 | -610.8 | |
| 0.00 | 1.26 | 0.00 | 0.95 | -17.47 | 213.93 | 47.43 | 248.60 | 0.7567 | 461.0 | 393.9 | |
| 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. | |