SDO HMI 2014-10-11 23:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.46 | 480.75 | 38.17 | 289.71 | -20.64 | 17.72 | -22.42 | 141.14 | 0.5707 | 1031.3 | 343.6 | |
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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 | 0.88 | 0.00 | 0.51 | -18.66 | 19.99 | -20.15 | 141.68 | 0.5285 | 859.0 | 714.9 | |
| 0.00 | 3.94 | 0.00 | 2.28 | -18.10 | 19.99 | -20.15 | 140.98 | 0.5221 | 791.0 | 718.7 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -18.27 | 19.90 | -20.24 | 141.07 | 0.5248 | 779.0 | 637.6 | |
| 0.00 | 0.70 | 0.00 | 0.41 | -19.45 | 19.35 | -20.80 | 141.77 | 0.5431 | -399.0 | -229.9 | |
| 0.00 | 1.84 | 0.00 | 1.08 | -19.15 | 19.32 | -20.82 | 141.37 | 0.5401 | 916.0 | 781.5 | |
| 0.00 | 0.96 | 0.00 | 0.57 | -19.72 | 19.21 | -20.94 | 141.91 | 0.5474 | 843.0 | 726.8 | |
| 2.80 | 461.31 | 1.67 | 277.59 | -20.37 | 18.60 | -21.54 | 141.90 | 0.5601 | 1455.1 | 361.3 | |
| 1.40 | -7.00 | 0.85 | -7.00 | -21.04 | 17.91 | -22.23 | 141.82 | 0.5734 | 906.2 | 999999 | |
| 59.00 | -7.00 | 35.49 | -7.00 | -20.61 | 17.84 | -22.30 | 141.23 | 0.5694 | 1373.3 | 999999 | |
| 0.26 | -7.00 | 0.16 | -7.00 | -20.50 | 17.09 | -23.05 | 140.20 | 0.5751 | 709.7 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.63 | -18.56 | 15.32 | -24.82 | 135.72 | 0.5723 | -639.0 | -502.9 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -22.27 | 11.79 | -28.35 | 136.53 | 0.6411 | -717.0 | -650.0 | |
| 0.00 | 1.40 | 0.00 | 0.95 | -25.94 | 10.34 | -29.80 | 139.22 | 0.6865 | -669.0 | -586.9 | |
| 0.00 | 3.41 | 0.00 | 2.34 | -26.43 | 9.81 | -30.33 | 139.26 | 0.6951 | -575.0 | -584.1 | |
| 0.00 | 1.40 | 0.00 | 0.88 | -18.23 | 10.76 | -29.38 | 130.59 | 0.6159 | -627.0 | -555.9 | |
| 0.00 | 1.75 | 0.00 | 1.20 | -23.16 | 6.99 | -33.15 | 133.26 | 0.6927 | -554.0 | -480.8 | |
| 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. | |