SDO HMI 2014-03-24 16:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.83 | 42.71 | 7.42 | 29.60 | 3.09 | 137.33 | -43.35 | 78.37 | 0.7019 | -171.2 | 130.1 | |
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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 |
| 0.00 | 0.79 | 0.00 | 0.53 | 6.28 | 140.47 | -40.20 | 72.72 | 0.6743 | -471.0 | -408.0 | |
| 1.66 | 2.79 | 1.12 | 1.88 | 3.12 | 139.22 | -41.45 | 77.73 | 0.6788 | -823.1 | -672.2 | |
| 2.44 | 5.33 | 1.65 | 3.59 | 3.46 | 139.21 | -41.47 | 77.25 | 0.6800 | -835.1 | -631.2 | |
| 0.87 | 2.10 | 0.59 | 1.41 | 2.87 | 139.00 | -41.68 | 78.17 | 0.6809 | -534.4 | -438.5 | |
| 0.00 | 0.96 | 0.00 | 0.65 | 3.42 | 138.93 | -41.75 | 77.40 | 0.6834 | -387.0 | -324.1 | |
| 3.41 | 8.03 | 2.32 | 5.48 | 3.91 | 138.54 | -42.14 | 76.85 | 0.6897 | -627.4 | -347.6 | |
| 0.00 | 1.05 | 0.00 | 0.72 | 5.16 | 138.08 | -42.59 | 75.27 | 0.6993 | -561.0 | -445.9 | |
| 0.00 | 1.40 | 0.00 | 0.96 | 2.63 | 137.87 | -42.81 | 78.88 | 0.6941 | 779.0 | 639.3 | |
| 0.00 | 1.48 | 0.00 | 1.04 | 3.77 | 136.86 | -43.81 | 77.62 | 0.7096 | -532.0 | -436.9 | |
| 0.00 | 3.49 | 0.00 | 2.45 | 2.67 | 136.63 | -44.05 | 79.21 | 0.7093 | 600.0 | 502.5 | |
| 0.87 | 3.41 | 0.62 | 2.40 | 2.26 | 136.18 | -44.49 | 79.91 | 0.7136 | 774.8 | 654.9 | |
| 1.14 | 9.26 | 0.81 | 6.61 | 2.37 | 135.24 | -45.43 | 80.03 | 0.7250 | 668.9 | 640.5 | |
| 0.00 | 1.31 | 0.00 | 0.94 | 2.20 | 135.12 | -45.55 | 80.30 | 0.7261 | 435.0 | 343.7 | |
| 0.44 | 1.31 | 0.31 | 0.94 | 2.48 | 134.98 | -45.69 | 79.95 | 0.7284 | 416.0 | 377.5 | |
| 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. | |