SDO HMI 2014-05-18 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.80 | 264.62 | 23.59 | 145.78 | -24.24 | 191.20 | 14.21 | 210.79 | 0.4391 | 738.0 | 324.8 | |
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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 |
| 23.38 | 247.79 | 12.88 | 136.62 | -24.06 | 191.64 | 14.65 | 211.82 | 0.4398 | 1316.4 | 397.7 | |
| 19.42 | -1.00 | 10.71 | -1.00 | -24.33 | 191.43 | 14.44 | 211.11 | 0.4415 | 1196.2 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -24.14 | 190.15 | 13.15 | 209.09 | 0.4289 | 766.0 | 550.4 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -24.26 | 187.30 | 10.31 | 203.53 | 0.4104 | -613.0 | -531.5 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -24.13 | 187.16 | 10.16 | 203.37 | 0.4076 | -906.0 | -701.0 | |
| 0.00 | 2.97 | 0.00 | 1.61 | -24.23 | 186.52 | 9.53 | 201.97 | 0.4052 | -895.0 | -744.3 | |
| 0.00 | 2.88 | 0.00 | 1.56 | -24.46 | 186.54 | 9.55 | 201.78 | 0.4086 | -823.0 | -721.8 | |
| 0.00 | 1.98 | 0.00 | 1.07 | -24.46 | 186.27 | 9.28 | 201.22 | 0.4071 | -878.0 | -756.5 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -25.71 | 186.20 | 9.20 | 199.90 | 0.4250 | -852.0 | -678.1 | |
| 0.00 | 3.33 | 0.00 | 1.84 | -27.95 | 184.54 | 7.54 | 194.98 | 0.4506 | -781.0 | -581.4 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -24.21 | 180.13 | 3.14 | 187.61 | 0.3784 | -732.0 | -517.3 | |
| 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. | |