SDO HMI 2014-05-19 14:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.96 | 39.94 | 10.90 | 36.11 | -17.96 | 217.83 | 55.71 | 249.89 | 0.8389 | 323.2 | 139.6 | |
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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 | 1.80 | 0.00 | 1.67 | -18.17 | 218.73 | 56.61 | 249.80 | 0.8474 | 601.0 | 462.6 | |
| 7.73 | 19.33 | 7.21 | 17.98 | -18.58 | 218.88 | 56.76 | 249.35 | 0.8493 | 698.8 | 235.5 | |
| 0.63 | 1.62 | 0.57 | 1.46 | -17.12 | 217.77 | 55.65 | 250.86 | 0.8373 | 467.1 | 413.9 | |
| 0.00 | 1.08 | 0.00 | 0.97 | -17.28 | 217.78 | 55.67 | 250.68 | 0.8377 | 329.0 | 296.2 | |
| 0.00 | 3.51 | 0.00 | 3.13 | -17.00 | 217.43 | 55.32 | 250.94 | 0.8341 | 694.0 | 558.4 | |
| 0.00 | 0.99 | 0.00 | 0.87 | -16.93 | 216.73 | 54.62 | 250.90 | 0.8275 | 167.0 | 127.5 | |
| 0.00 | 0.81 | 0.00 | 0.72 | -18.25 | 217.00 | 54.88 | 249.38 | 0.8321 | 634.0 | 536.2 | |
| 0.00 | 3.42 | 0.00 | 2.92 | -15.63 | 215.78 | 53.66 | 252.29 | 0.8165 | -745.0 | -513.2 | |
| 1.35 | 2.52 | 1.18 | 2.21 | -18.27 | 216.45 | 54.33 | 249.25 | 0.8271 | -389.5 | -241.3 | |
| 1.44 | 2.97 | 1.25 | 2.58 | -18.37 | 216.17 | 54.05 | 249.07 | 0.8247 | -548.4 | -412.8 | |
| 0.81 | 1.89 | 0.69 | 1.60 | -17.35 | 215.18 | 53.06 | 250.09 | 0.8136 | -548.2 | -434.5 | |
| 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. | |