SDO HMI 2011-06-08 07:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.41 | 34.50 | 11.11 | 30.77 | 17.69 | 21.05 | 54.37 | 291.33 | 0.8328 | -273.3 | -283.8 | |
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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 | 4.07 | 0.00 | 4.03 | 20.26 | 24.45 | 57.78 | 293.48 | 0.8673 | -566.0 | -413.0 | |
| 6.07 | 9.42 | 5.49 | 8.52 | 17.11 | 21.78 | 55.11 | 290.46 | 0.8388 | -450.4 | -258.2 | |
| 0.00 | 1.09 | 0.00 | 0.99 | 17.85 | 21.95 | 55.27 | 291.28 | 0.8417 | -394.0 | -317.6 | |
| 0.00 | 3.80 | 0.00 | 3.40 | 17.18 | 21.31 | 54.63 | 290.65 | 0.8347 | -579.0 | -483.5 | |
| 0.00 | 1.27 | 0.00 | 1.12 | 17.02 | 21.02 | 54.35 | 290.53 | 0.8318 | -450.0 | -420.1 | |
| 2.81 | 7.88 | 2.47 | 6.91 | 16.67 | 20.82 | 54.14 | 290.16 | 0.8292 | -459.0 | -618.4 | |
| 1.99 | -6.00 | 1.74 | -6.00 | 16.60 | 20.41 | 53.74 | 290.18 | 0.8254 | -743.7 | 999999 | |
| 1.54 | 2.17 | 1.41 | 1.99 | 19.42 | 21.64 | 54.97 | 293.19 | 0.8422 | 375.2 | 308.1 | |
| 0.00 | 1.18 | 0.00 | 0.97 | 16.73 | 17.89 | 51.22 | 290.97 | 0.8016 | -493.0 | -461.9 | |
| 0.00 | 1.81 | 0.00 | 1.42 | 17.44 | 15.22 | 48.54 | 292.61 | 0.7768 | 526.0 | 430.8 | |
| 0.00 | 1.00 | 0.00 | 0.79 | 18.78 | 15.38 | 48.71 | 294.23 | 0.7822 | 497.0 | 403.6 | |
| 0.00 | 0.81 | 0.00 | 0.63 | 19.46 | 14.09 | 47.42 | 295.51 | 0.7715 | 608.0 | 487.2 | |
| 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. | |