SDO HMI 2014-05-19 02:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.65 | 255.96 | 23.49 | 147.74 | -24.39 | 190.86 | 22.15 | 222.08 | 0.5145 | 724.2 | 326.7 | |
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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 |
| 38.13 | 240.66 | 22.04 | 139.09 | -24.32 | 191.19 | 22.48 | 222.61 | 0.5168 | 1177.3 | 385.2 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -20.96 | 190.27 | 21.56 | 226.67 | 0.4738 | -555.0 | -556.9 | |
| 2.16 | -1.00 | 1.24 | -1.00 | -24.04 | 190.45 | 21.75 | 222.13 | 0.5065 | 957.8 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -24.11 | 190.04 | 21.33 | 221.51 | 0.5030 | 863.0 | 681.8 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -25.16 | 189.72 | 21.02 | 219.62 | 0.5111 | 706.0 | 501.5 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -25.96 | 186.32 | 17.62 | 213.96 | 0.4892 | -687.0 | -543.8 | |
| 0.00 | 2.79 | 0.00 | 1.56 | -24.61 | 185.88 | 17.18 | 215.07 | 0.4692 | -693.0 | -597.3 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -25.73 | 185.97 | 17.27 | 213.74 | 0.4835 | -605.0 | -514.0 | |
| 0.00 | 3.15 | 0.00 | 1.78 | -26.37 | 185.29 | 16.59 | 211.93 | 0.4856 | -874.0 | -748.0 | |
| 0.36 | 1.62 | 0.21 | 0.92 | -27.38 | 185.23 | 16.53 | 210.64 | 0.4976 | -837.2 | -746.5 | |
| 0.00 | 2.70 | 0.00 | 1.53 | -27.12 | 184.19 | 15.49 | 209.39 | 0.4864 | -747.0 | -630.7 | |
| 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. | |