SDO HMI 2011-06-08 06:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.30 | 42.02 | 15.52 | 37.10 | 17.53 | 21.27 | 54.05 | 291.23 | 0.8296 | -283.7 | -238.7 | |
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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 |
| 0.00 | 1.54 | 0.00 | 1.52 | 15.89 | 25.87 | 58.65 | 288.35 | 0.8673 | -441.0 | -359.0 | |
| 2.81 | 2.90 | 2.74 | 2.82 | 20.23 | 24.49 | 57.27 | 293.56 | 0.8631 | -419.6 | -228.0 | |
| 0.00 | 1.27 | 0.00 | 1.24 | 21.40 | 24.28 | 57.06 | 294.94 | 0.8637 | 121.0 | 190.4 | |
| 6.97 | 14.67 | 6.22 | 13.04 | 17.11 | 21.77 | 54.55 | 290.59 | 0.8338 | -473.8 | -398.9 | |
| 2.63 | 12.95 | 2.28 | 11.21 | 16.66 | 20.82 | 53.60 | 290.29 | 0.8242 | -493.3 | -444.1 | |
| 0.00 | 1.54 | 0.00 | 1.35 | 17.01 | 20.96 | 53.74 | 290.67 | 0.8263 | -453.0 | -427.6 | |
| 3.26 | -5.00 | 2.81 | -5.00 | 16.66 | 20.44 | 53.22 | 290.38 | 0.8207 | -739.7 | 999999 | |
| 1.63 | 2.44 | 1.47 | 2.20 | 19.45 | 21.64 | 54.42 | 293.37 | 0.8375 | 467.1 | 359.9 | |
| 0.00 | 1.00 | 0.00 | 0.81 | 16.73 | 17.93 | 50.71 | 291.11 | 0.7966 | -679.0 | -505.2 | |
| 0.00 | 1.00 | 0.00 | 0.82 | 19.91 | 17.34 | 50.12 | 295.15 | 0.7992 | 473.0 | 391.7 | |
| 0.00 | 1.99 | 0.00 | 1.54 | 17.47 | 15.24 | 48.02 | 292.81 | 0.7715 | 594.0 | 471.5 | |
| 0.00 | 0.72 | 0.00 | 0.55 | 18.85 | 13.56 | 46.34 | 295.13 | 0.7584 | 610.0 | 521.1 | |
| 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. | |