SDO HMI 2011-06-14 13:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.17 | 30.10 | 2.15 | 15.53 | 15.69 | 250.35 | 6.39 | 337.52 | 0.2794 | -236.2 | -282.9 | |
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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 | 1.63 | 0.00 | 0.85 | 15.19 | 256.21 | 12.25 | 320.34 | 0.3222 | -807.0 | -645.5 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 15.36 | 252.75 | 8.79 | 329.44 | 0.2911 | -730.0 | -461.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.99 | 251.79 | 7.83 | 333.29 | 0.2926 | -799.0 | -578.1 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 12.61 | 251.58 | 7.61 | 327.48 | 0.2416 | 919.0 | 682.1 | |
| 0.00 | 2.63 | 0.00 | 1.36 | 15.65 | 250.60 | 6.63 | 336.38 | 0.2789 | -970.0 | -732.2 | |
| 0.73 | 11.51 | 0.37 | 5.95 | 16.28 | 250.46 | 6.50 | 337.72 | 0.2876 | -926.4 | -878.4 | |
| 1.45 | -6.00 | 0.75 | -6.00 | 16.09 | 250.42 | 6.46 | 337.57 | 0.2845 | -924.8 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.53 | 250.18 | 6.22 | 338.91 | 0.2898 | -771.0 | -554.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.03 | 248.86 | 4.90 | 342.54 | 0.2745 | 888.0 | 766.5 | |
| 1.99 | 6.89 | 1.03 | 3.55 | 16.34 | 248.55 | 4.59 | 343.91 | 0.2781 | 792.4 | 743.6 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 7.71 | 245.14 | 1.18 | 350.22 | 0.1206 | 783.0 | 565.7 | |
| 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. | |