SDO HMI 2014-08-18 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.32 | 72.98 | 11.27 | 36.96 | -4.46 | 31.02 | -2.64 | 167.46 | 0.2044 | 408.1 | 302.5 | |
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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 |
| 15.66 | 28.61 | 7.90 | 14.44 | -4.09 | 33.09 | -0.57 | 177.02 | 0.1903 | 1162.3 | 674.4 | |
| 0.00 | 2.88 | 0.00 | 1.46 | -4.78 | 31.63 | -2.03 | 170.04 | 0.2048 | 619.0 | 553.7 | |
| 0.00 | 2.07 | 0.00 | 1.05 | -4.34 | 31.33 | -2.33 | 168.16 | 0.1985 | 1044.0 | 892.5 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -4.65 | 31.30 | -2.36 | 168.32 | 0.2038 | 821.0 | 624.4 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -4.81 | 31.18 | -2.48 | 167.89 | 0.2069 | 773.0 | 587.5 | |
| 0.00 | 8.10 | 0.00 | 4.09 | -4.28 | 31.00 | -2.67 | 166.45 | 0.1987 | 956.0 | 967.5 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -3.91 | 31.00 | -2.66 | 166.00 | 0.1925 | 947.0 | 767.6 | |
| 1.35 | 5.76 | 0.68 | 2.91 | -4.10 | 30.54 | -3.12 | 163.98 | 0.1977 | 1082.5 | 759.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -4.69 | 30.29 | -3.37 | 163.62 | 0.2086 | 909.0 | 716.9 | |
| 4.68 | 16.38 | 2.37 | 8.30 | -4.39 | 29.04 | -4.62 | 157.52 | 0.2108 | -1156.5 | -819.4 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -5.91 | 28.97 | -4.69 | 159.69 | 0.2354 | -996.0 | -745.5 | |
| 0.63 | -10.00 | 0.32 | -10.00 | -4.58 | 28.92 | -4.74 | 157.32 | 0.2145 | -953.0 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.71 | -12.59 | 27.25 | -6.41 | 161.80 | 0.3505 | -2.0 | 2.5 | |
| 0.00 | 0.72 | 0.00 | 0.37 | -2.49 | 23.91 | -9.75 | 133.39 | 0.2338 | -662.0 | -475.1 | |
| 0.00 | 1.35 | 0.00 | 0.70 | -5.48 | 22.36 | -11.31 | 137.20 | 0.2885 | -832.0 | -589.9 | |
| 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. | |