SDO HMI 2011-03-06 00:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.44 | 43.29 | 5.66 | 33.32 | -23.03 | 181.44 | 49.41 | 245.90 | 0.7678 | 139.4 | 101.7 | |
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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 | 2.42 | 0.00 | 1.91 | -22.03 | 182.93 | 50.90 | 247.48 | 0.7810 | 474.0 | 351.5 | |
| 1.12 | 3.28 | 0.88 | 2.58 | -21.86 | 182.74 | 50.71 | 247.67 | 0.7788 | 558.7 | 610.7 | |
| 0.00 | 5.96 | 0.00 | 4.68 | -22.18 | 182.64 | 50.62 | 247.24 | 0.7784 | 689.0 | 644.5 | |
| 0.00 | 1.04 | 0.00 | 0.81 | -22.13 | 182.21 | 50.18 | 247.23 | 0.7740 | 662.0 | 581.6 | |
| 0.00 | 1.38 | 0.00 | 1.08 | -22.32 | 182.21 | 50.18 | 246.98 | 0.7742 | 468.0 | 378.4 | |
| 1.56 | 2.85 | 1.21 | 2.22 | -22.53 | 182.26 | 50.23 | 246.72 | 0.7752 | 497.3 | 539.3 | |
| 0.00 | 4.41 | 0.00 | 3.44 | -22.88 | 182.24 | 50.21 | 246.27 | 0.7756 | 518.0 | 432.7 | |
| 0.00 | 1.12 | 0.00 | 0.87 | -23.18 | 181.78 | 49.75 | 245.80 | 0.7715 | 531.0 | 398.2 | |
| 1.99 | 13.57 | 1.50 | 10.25 | -23.59 | 180.40 | 48.37 | 244.96 | 0.7583 | -305.6 | -420.9 | |
| 0.00 | 1.30 | 0.00 | 0.99 | -24.24 | 180.57 | 48.55 | 244.17 | 0.7616 | -396.0 | -314.1 | |
| 1.30 | 2.07 | 0.97 | 1.56 | -23.75 | 179.99 | 47.96 | 244.65 | 0.7545 | -592.5 | -447.4 | |
| 0.00 | 0.78 | 0.00 | 0.59 | -24.23 | 180.23 | 48.20 | 244.08 | 0.7581 | -496.0 | -456.1 | |
| 1.47 | 3.11 | 1.10 | 2.34 | -24.36 | 179.85 | 47.82 | 243.82 | 0.7546 | -550.8 | -529.3 | |
| 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. | |