SDO HMI 2011-10-18 04:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.70 | 179.34 | 14.93 | 108.40 | -26.88 | 36.18 | 12.60 | 199.97 | 0.5749 | 611.7 | 336.1 | |
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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 |
| 24.70 | 162.05 | 14.93 | 98.00 | -26.75 | 37.19 | 13.61 | 201.49 | 0.5756 | 1204.3 | 363.8 | |
| 0.00 | 3.14 | 0.00 | 1.80 | -22.52 | 33.79 | 10.20 | 199.17 | 0.5005 | 834.0 | 741.6 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -27.45 | 33.59 | 10.01 | 195.81 | 0.5686 | 629.0 | 451.5 | |
| 0.00 | 1.40 | 0.00 | 0.84 | -27.40 | 32.50 | 8.92 | 194.18 | 0.5637 | 499.0 | 506.4 | |
| 0.00 | 1.48 | 0.00 | 0.90 | -29.09 | 30.19 | 6.61 | 190.01 | 0.5805 | 710.0 | 588.8 | |
| 0.00 | 3.14 | 0.00 | 1.89 | -28.51 | 29.71 | 6.13 | 189.49 | 0.5711 | 663.0 | 571.4 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -27.61 | 25.23 | 1.65 | 182.66 | 0.5513 | -674.0 | -564.8 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -29.82 | 21.82 | -1.76 | 177.37 | 0.5833 | -731.0 | -679.0 | |
| 0.00 | 0.96 | 0.00 | 0.61 | -33.22 | 19.43 | -4.16 | 174.48 | 0.6327 | -548.0 | -407.3 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -30.20 | 19.46 | -4.13 | 173.94 | 0.5912 | -683.0 | -485.3 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -29.40 | 19.21 | -4.37 | 173.41 | 0.5802 | -731.0 | -591.2 | |
| 0.00 | 1.40 | 0.00 | 0.87 | -31.25 | 18.89 | -4.70 | 173.35 | 0.6067 | -715.0 | -474.3 | |
| 0.00 | 1.22 | 0.00 | 0.75 | -29.64 | 16.79 | -6.80 | 169.90 | 0.5887 | -759.0 | -653.1 | |
| 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. | |