SDO HMI 2014-05-18 04:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.52 | 279.65 | 23.64 | 151.81 | -24.10 | 191.60 | 10.77 | 204.66 | 0.4108 | 757.8 | 361.5 | |
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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 | 3.15 | 0.00 | 1.68 | -21.57 | 191.80 | 10.97 | 208.18 | 0.3763 | -584.0 | -408.1 | |
| 11.42 | 265.70 | 6.21 | 144.30 | -24.10 | 191.97 | 11.14 | 205.40 | 0.4131 | 1210.8 | 403.3 | |
| 14.48 | -2.00 | 7.85 | -2.00 | -23.90 | 191.65 | 10.82 | 204.98 | 0.4082 | 1448.3 | 999999 | |
| 17.62 | -2.00 | 9.58 | -2.00 | -24.26 | 191.62 | 10.79 | 204.51 | 0.4130 | 1190.7 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.86 | -22.10 | 190.38 | 9.55 | 204.41 | 0.3736 | -816.0 | -527.6 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -22.32 | 190.36 | 9.53 | 204.10 | 0.3768 | -703.0 | -579.1 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -26.81 | 190.43 | 9.60 | 199.73 | 0.4427 | 680.0 | 521.0 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -26.18 | 190.28 | 9.45 | 199.99 | 0.4327 | 694.0 | 460.1 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -24.83 | 189.87 | 9.04 | 200.40 | 0.4106 | 584.0 | 532.8 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -23.89 | 187.46 | 6.63 | 196.01 | 0.3843 | -898.0 | -721.6 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -24.22 | 187.17 | 6.34 | 195.11 | 0.3881 | -937.0 | -727.0 | |
| 0.00 | 0.45 | 0.00 | 0.24 | -24.32 | 186.64 | 5.81 | 193.83 | 0.3875 | -685.0 | -578.6 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -25.70 | 186.10 | 5.27 | 191.77 | 0.4071 | -760.0 | -612.6 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -28.17 | 184.90 | 4.07 | 188.16 | 0.4424 | -620.0 | -533.1 | |
| 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. | |