SDO HMI 2014-05-09 23:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.12 | 256.39 | 35.45 | 174.84 | 14.77 | 249.58 | -39.81 | 64.37 | 0.6889 | -749.1 | -216.2 | |
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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 |
| 8.24 | 245.56 | 5.62 | 167.16 | 15.26 | 249.79 | -39.60 | 63.61 | 0.6888 | -808.4 | -257.4 | |
| 10.57 | -1.00 | 7.18 | -1.00 | 15.04 | 249.80 | -39.59 | 63.90 | 0.6876 | -997.9 | 999999 | |
| 32.06 | -1.00 | 21.80 | -1.00 | 14.66 | 249.68 | -39.71 | 64.48 | 0.6873 | -1067.4 | 999999 | |
| 1.25 | -1.00 | 0.85 | -1.00 | 14.32 | 249.59 | -39.80 | 64.99 | 0.6867 | -793.0 | 999999 | |
| 0.00 | 1.70 | 0.00 | 1.18 | 13.11 | 247.53 | -41.86 | 67.61 | 0.7052 | 717.0 | 653.1 | |
| 0.00 | 2.69 | 0.00 | 1.92 | 14.66 | 246.59 | -42.80 | 65.97 | 0.7220 | 553.0 | 439.1 | |
| 0.00 | 1.07 | 0.00 | 0.77 | 14.61 | 246.39 | -43.00 | 66.13 | 0.7240 | 516.0 | 502.0 | |
| 0.00 | 0.90 | 0.00 | 0.64 | 14.29 | 246.42 | -42.97 | 66.53 | 0.7224 | 628.0 | 615.8 | |
| 0.00 | 1.16 | 0.00 | 0.82 | 13.18 | 246.59 | -42.80 | 67.93 | 0.7162 | 315.0 | 307.8 | |
| 0.00 | 1.25 | 0.00 | 0.90 | 14.39 | 246.22 | -43.17 | 66.48 | 0.7250 | 593.0 | 529.0 | |
| 0.00 | 2.06 | 0.00 | 1.45 | 11.67 | 246.55 | -42.84 | 69.96 | 0.7111 | 531.0 | 444.7 | |
| 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. | |